Updated on 2024/04/19

写真a

 
TAJIMA, Hiroyasu
 
Organization
Institute for Space-Earth Environmental Research Center for Orbital and Suborbital Research Professor
Graduate School
Graduate School of Science
Title
Professor

Degree 1

  1. 理学博士 ( 1991.6   名古屋大学 ) 

Research Interests 7

  1. Imaging Atmospheric Cherenkov telescope

  2. Compton telescope

  3. gamma-ray polarization

  4. gamma-ray burst

  5. supernova remnant

  6. gamma-ray astrophysics

  7. Cosmic-ray acceleration and propagation

Research Areas 1

  1. Others / Others  / Elementary Particle/Cosmic Ray/Astrophysics

Research History 6

  1. The University of Tokyo   Visiting Professor   Visiting Professor

    2022.4

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    Country:Japan

  2. SLAC National Accelerator Laboratory   Particle Astrophysics   Senior Staff Scientist

    2009.7 - 2010.8

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    Country:United States

  3. SLAC National Accelerator Laboratory   Particle Astrophysics   Staff Scientist

    2001.8 - 2009.6

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    Country:United States

  4. The University of Tokyo   Assistant

    1996.1 - 2001.8

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    Country:Japan

  5. University of California Santa Barbara   Department of Physics   Assistant

    1993.2 - 1995.12

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    Country:United States

  6. University of California Santa Barbara   Department of Physics   Researcher

    1991.4 - 1993.1

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    Country:United States

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Education 2

  1. Nagoya University   Graduate School, Division of Science

    1988.4 - 1991.3

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    Country: Japan

  2. Nagoya University   Faculty of Science   Department of Physics

    1982.4 - 1986.3

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    Country: Japan

Professional Memberships 1

  1. 日本物理学会

Committee Memberships 16

  1. Science organizing comittee for SiPM workshop: from fundamental research to industrial applications   Comittee member  

    2018.10 - 2020.5   

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    Committee type:Municipal

  2. 5th Fermi Symposium   LOC Chairperson  

    2014.10   

  3. KEK B-Factory Program Committee   Committee Member  

    2014.4   

  4. Fermi Symposium Scientific Organizing Committee   Committee Member  

    2014.4 - 2015.12   

  5. NASA Astrophysics Explorer Mission of Opportunity   Reviewer, Gamma-ray panel  

    2013.4   

  6. KEK Detector Technology Project International Review Committee   Chairperson  

    2013   

  7. Vienna Conference on Instrumentation Science Organizing Committee   Committee Member  

    2012.4   

  8. KEK Institute for Particle and Nuclear Physics, Steering Committee   Committee Member  

    2012.4 - 2015.3   

  9. KEK SOI International Review Committee   Chairperson  

    2011   

  10. NASA ROSES Solicitation for the Astronomy and Physics Research and Analysis   Reviewer, Gamma-ray panel  

    2009 - 2012   

  11. IEEE Nuclear Science Symposium Program Convener   Topic Convener, Astrophysics and Space Instrumentation  

    2007   

  12. Joint Meeting of Pacific Region Particle Physics Communities   Topic Convener, Particle Astrophysics  

    2006   

  13. NASA NuSTAR project Shield Review Committee   Committee Member  

    2005   

  14. IEEE Nuclear Science Symposium Program Committee   Committee Member  

    2003   

  15. Thematic Research Program of Academia Sinica   Reviewer  

    2001 - 2005   

  16. Fermi National Accelerator Laboratory Technical Review Committee   Reviewer  

    2001 - 2002   

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Papers 113

  1. Fine-Pitch Semiconductor Detector for the FOXSI Mission Reviewed

    Ishikawa, S.; Saito, S.; Tajima, H.; Tanaka, T.; Watanabe, S.; Odaka, H.; Fukuyama, T.; Kokubun, M.; Takahashi, T.; Terada, Y.; Krucker, S.; Christe, S.; McBride, S.; Glesener, L.

    IEEE Transactions on Nuclear Science   Vol. 58   page: 2039-2046   2011.8

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    Authorship:Lead author   Language:English   Publishing type:Research paper (scientific journal)  

    The Focusing Optics X-ray Solar Imager (FOXSI) is a NASA sounding rocket mission which will study particle acceleration and coronal heating on the Sun through high sensitivity observations in the hard X-ray energy band (5-15 keV). Combining high-resolution focusing X-ray optics and fine-pitch imaging sensors, FOXSI will achieve superior sensitivity; two orders of magnitude better than that of the RHESSI satellite. As the focal plane detector, a Double-sided Si Strip Detector (DSSD) with a front-end ASIC (Application Specific Integrated Circuit) will fulfill the scientific requirements of spatial and energy resolution, low energy threshold and time resolution. We have designed and fabricated a DSSD with a thickness of 500 µm and a dimension of 9.6 mm x 9.6 mm, containing 128 strips with a pitch of 75 µm, which corresponds to 8 arcsec at the focal length of 2 m. We also developed a low-noise ASIC specified to FOXSI. The detector was successfully operated in the laboratory at a temperature of -20 C and with an applied bias voltage of 300 V, and the energy resolution of 430 eV at a 14 keV line was achieved. We also demonstrated fine-pitch imaging successfully by obtaining a shadow image, hence the implementation of scientific requirements was confirmed.

    DOI: 10.1109/TNS.2011.2154342

  2. Gamma-Ray Emission from the Shell of Supernova Remnant W44 Revealed by the Fermi LAT Reviewed International coauthorship

    Fermi LAT collaboration

    Science   Vol. 327   page: 1103   2010.2

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    Authorship:Corresponding author   Language:English   Publishing type:Research paper (scientific journal)  

    Recent observations of supernova remnants (SNRs) hint that they accelerate cosmic rays to energies close to ~1015 electron volts. However, the nature of the particles that produce the emission remains ambiguous. We report observations of SNR W44 with the Fermi Large Area Telescope at energies between 2 × 10^8 electron volts and 3 ×10^q11 electron volts. The detection of a source with a morphology corresponding to the SNR shell implies that the emission is produced by particles accelerated there. The gamma-ray spectrum is well modeled with emission from protons and nuclei. Its steepening above ~10^9 electron volts provides a probe with which to study how particle acceleration responds to environmental effects such as shock propagation in dense clouds and how accelerated particles are released into interstellar space.

    DOI: 10.1126/science.1182787

  3. A limit on the variation of the speed of light arising from quantum gravity effects Reviewed International coauthorship

    Fermi LAT/GBM collaborations

    Nature   Vol. 462   page: 331-334   2009.11

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    Language:English   Publishing type:Research paper (scientific journal)  

    A cornerstone of Einstein's special relativity is Lorentz invariance - the postulate that all observers measure exactly the same speed of light in vacuum, independent of photon-energy. While special relativity assumes that there is no fundamental length-scale associated with such invariance, there is a fundamental scale (the Planck scale, lPlanck~1.62×10^-33cm or EPlanck = MPlanck~1.22×10^19GeV/c2), at which quantum effects are expected to strongly affect the nature of space-time. There is great interest in the (not yet validated) idea that Lorentz invariance might break near the Planck scale. A key test of such violation of Lorentz invariance is a possible variation of photon speed with energy. Even a tiny variation in photon speed, when accumulated over cosmological light-travel times, may be revealed by observing sharp features in γ-ray burst (GRB) light-curves. Here we report the detection of emission up to ~31GeV from the distant and short GRB090510. We find no evidence for the violation of Lorentz invariance, and place a lower limit of 1.2EPlanck on the scale of a linear energy dependence (or an inverse wavelength dependence), subject to reasonable assumptions about the emission (equivalently we have an upper limit of lPlanck/1.2 on the length scale of the effect). Our results disfavour quantum-gravity theories in which the quantum nature of space-time on a very small scale linearly alters the speed of light.

    DOI: 10.1038/nature08574

  4. The on-orbit calibration of the Fermi Large Area Telescope Reviewed International coauthorship

    Fermi LAT collaboration

    Astroparticle Physics   Vol. 32   page: 193-219   2009.10

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    Language:English   Publishing type:Research paper (scientific journal)  

    The Large Area Telescope (LAT) on-board the Fermi Gamma-ray Space Telescope began its on-orbit operations on June 23, 2008. Calibrations, defined in a generic sense, correspond to synchronization of trigger signals, optimization of delays for latching data, determination of detector thresholds, gains and responses, evaluation of the perimeter of the South Atlantic Anomaly (SAA), measurements of live time, of absolute time, and internal and spacecraft boresight alignments. Here we describe on-orbit calibration results obtained using known astrophysical sources, galactic cosmic rays, and charge injection into the front-end electronics of each detector. Instrument response functions will be described in a separate publication. This paper demonstrates the stability of calibrations and describes minor changes observed since launch. These results have been used to calibrate the LAT datasets to be publicly released in August 2009.

    DOI: 10.1016/j.astropartphys.2009.08.002

  5. Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C Reviewed International coauthorship

    Fermi LAT/GBM collaborations

    Science   Vol. 323   page: 1688-1693   2009.3

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    Authorship:Corresponding author   Language:English   Publishing type:Research paper (scientific journal)  

    Gamma-ray bursts (GRBs) are highly energetic explosions signaling the death of massive stars in distant galaxies. The Gamma-ray Burst Monitor and Large Area Telescope onboard the Fermi Observatory together record GRBs over a broad energy range spanning about 7 decades of gamma-ray energy. In September 2008, Fermi observed the exceptionally luminous GRB 080916C, with the largest apparent energy release yet measured. The high-energy gamma rays are observed to start later and persist longer than the lower energy photons. A simple spectral form fits the entire GRB spectrum, providing strong constraints on emission models. The known distance of the burst enables placing lower limits on the bulk Lorentz factor of the outflow and on the quantum gravity mass.

    DOI: 10.1126/science.1169101

  6. AstroPix4 — a novel HV-CMOS sensor developed for space based experiments Reviewed

    Striebig N., Leys R., Peric I., Caputo R., Steinhebel A.L., Suda Y., Fukazawa Y., Jadhav M., Violette D., Kierans C., Tajima H., Metcalfe J., Perkins J.S.

    Journal of Instrumentation   Vol. 19 ( 4 )   2024.4

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Journal of Instrumentation  

    For the proposed space based gamma-ray observatory All-sky Medium-Energy Gamma-ray Observatory eXplorer (AMEGO-X), a silicon tracker based on a novel High Voltage-CMOS (HV-CMOS) sensor called AstroPix, is currently being developed. Preliminary measurements with the first full reticle prototype AstroPix3 show that the power target of 1.5 mW/cm2 can currently not be reached due to the digital consumption of 3.08 mW/cm2, while the analog power consumption of 1.04 mW/cm2 and a break down voltage of over 350 V look promising. Based on these results, the design changes in AstroPix4, submitted in May 2023, are presented, containing changes to the time stamp generation and readout architecture. A digital power consumption below 0.25 mW/cm2 is expected by removing the fast 200 MHz clock used to measure the time-over-threshold (ToT) and an LVDS receiver. A maximum resolution of 3.125 ns for time-of-arrival (ToA) and ToT is reached by adding per-pixel Flash-Time-to-Digital Converter (TDCs) controlled by a global delay-locked loop (DLL).

    DOI: 10.1088/1748-0221/19/04/C04010

    Scopus

  7. The variability patterns of the TeV blazar PG 1553 + 113 from a decade of MAGIC and multiband observations Reviewed

    Abe H., Abe S., Abhir J., Acciari V.A., Agudo I., Aniello T., Ansoldi S., Antonelli L.A., Arbet Engels A., Arcaro C., Artero M., Asano K., Baack D., Babić A., Baquero A., Barres de Almeida U., Batković I., Baxter J., Becerra González J., Bernardini E., Bernete J., Berti A., Besenrieder J., Bigongiari C., Biland A., Blanch O., Bonnoli G., Bošnjak , Burelli I., Busetto G., Campoy-Ordaz A., Carosi A., Carosi R., Carretero-Castrillo M., Castro-Tirado A.J., Chai Y., Cifuentes A., Cikota S., Colombo E., Contreras J.L., Cortina J., Covino S., D’Amico G., D’Elia V., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Del Popolo A., Delfino M., Delgado J., Delgado Mendez C., Depaoli D., Di Pierro F., Di Venere L., Dominis Prester D., Donini A., Dorner D., Doro M., Elsaesser D., Emery G., Escudero J., Fariña L., Fattorini A., Foffano L., Font L., Fukami S., Fukazawa Y., García López R.J., Gasparyan S., Gaug M., Giesbrecht Paiva J.G., Giglietto N., Giordano F., Gliwny P., Grau R., Green J.G., Hadasch D., Hahn A., Heckmann L., Herrera J., Hovatta T., Hrupec D., Hütten M., Imazawa R., Inada T., Iotov R., Ishio K., Jimenez Martínez I., Jormanainen J., Kerszberg D., Kluge G.W., Kobayashi Y., Kouch P.M., Kubo H., Kushida J., Láinez Lezáun M., Lamastra A., Leone F., Lindfors E.

    Monthly Notices of the Royal Astronomical Society   Vol. 529 ( 4 ) page: 3894 - 3911   2024.4

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Monthly Notices of the Royal Astronomical Society  

    PG 1553 + 113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high energy (VHE; >100 GeV) gamma-ray emitter. To better understand its properties and identify the underlying physical processes driving its variability, the MAGIC Collaboration initiated a multiyear, multiwavelength monitoring campaign in 2015 involving the OVRO 40-m and Medicina radio telescopes, REM, KVA, and the MAGIC telescopes, Swift and Fermi satellites, and the WEBT network. The analysis presented in this paper uses data until 2017 and focuses on the characterization of the variability. The gamma-ray data show a (hint of a) periodic signal compatible with literature, but the X-ray and VHE gamma-ray data do not show statistical evidence for a periodic signal. In other bands, the data are compatible with the gamma-ray period, but with a relatively high p-value. The complex connection between the low- and high-energy emission and the non-monochromatic modulation and changes in flux suggests that a simple one-zone model is unable to explain all the variability. Instead, a model including a periodic component along with multiple emission zones is required.

    DOI: 10.1093/mnras/stae649

    Scopus

  8. Silicon photomultipliers for the SST camera of the Cherenkov Telescope Array Reviewed

    Depaoli D., Lapington J., Leach S., Okumura A., Sofia I., Tajima H.

    Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment   Vol. 1060   2024.3

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment  

    The Cherenkov Telescope Array Observatory (CTAO) will be the major global observatory for gamma-ray astronomy over the next decade and beyond. It will consist of two arrays of telescopes of different sizes, one for each hemisphere, and will be sensitive to gamma rays in the energy range from a few tens of GeV to hundreds of TeV. The Small-Sized Telescopes (SSTs) are a crucial component of the southern array, as they will extend the sensitivity of the observatory to the highest energies. Their focal plane will be equipped with 2048 Silicon Photomultiplier (SiPM) pixels, each one read independently by a state-of-the-art full waveform sampling readout. These solid-state sensors offer advantages over the traditional photomultiplier tubes, such as lower operating voltage, higher photon detection efficiency, and tolerance to bright illumination. In particular, they are the best choice for a small and compact camera such as the SST one. After a detailed comparative study, LVR3-type SiPMs from Hamamatsu Photonics were selected, with an active area of 6 mm × 6 mm, a microcell of 50 μm and without a protective coating, for optimum performance. The sensors demonstrated to have a higher photon detection efficiency and a lower crosstalk compared to the competitors, alongside a low dark count rate. In this contribution, we present the selection process and the latest measurements performed on the SiPMs mounted on the SST Camera module.

    DOI: 10.1016/j.nima.2023.169047

    Scopus

  9. Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES 2344+514 Invited International coauthorship

    Abe, H. et al.

    Astronomy & Astrophysics, Volume   Vol. 682   page: A114   2024.2

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1051/0004-6361/202347845

  10. MAGIC detection of GRB 201216C at z = 1.1 Reviewed

    Abe H., Abe S., Acciari V.A., Agudo I., Aniello T., Ansoldi S., Antonelli L.A., Arbet Engels A., Arcaro C., Artero M., Asano K., Baack D., Babić A., Baquero A., Barres de Almeida U., Barrio J.A., Batković I., Baxter J., Becerra González J., Bednarek W., Bernardini E., Bernete J., Berti A., Besenrieder J., Bigongiari C., Biland A., Blanch O., Bonnoli G., Bošnjak , Burelli I., Busetto G., Campoy-Ordaz A., Carosi A., Carosi R., Carretero-Castrillo M., Castro-Tirado A.J., Ceribella G., Chai Y., Cifuentes A., Cikota S., Colombo E., Contreras J.L., Cortina J., Covino S., D’Amico G., D’Elia V., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Del Popolo A., Delfino M., Delgado J., Delgado Mendez C., Depaoli D., Di Pierro F., Di Venere L., Dominis Prester D., Donini A., Dorner D., Doro M., Elsaesser D., Emery G., Escudero J., Fariña L., Fattorini A., Foffano L., Font L., Fukami S., Fukazawa Y., García López R.J., Garczarczyk M., Gasparyan S., Gaug M., Giesbrecht Paiva J.G., Giglietto N., Giordano F., Gliwny P., Godinović N., Grau R., Green D., Green J.G., Hadasch D., Hahn A., Hassan T., Heckmann L., Herrera J., Hrupec D., Hütten M., Imazawa R., Inada T., Iotov R., Ishio K., Jiménez Martínez I., Jormanainen J., Kerszberg D., Kluge G.W., Kobayashi Y., Kouch P.M., Kubo H.

    Monthly Notices of the Royal Astronomical Society   Vol. 527 ( 3 ) page: 5856 - 5867   2024.1

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Monthly Notices of the Royal Astronomical Society  

    Gamma-ray bursts (GRBs) are explosive transient events occurring at cosmological distances, releasing a large amount of energy as electromagnetic radiation over several energy bands. We report the detection of the long GRB 201216C by the MAGIC telescopes. The source is located at z = 1.1 and thus it is the farthest one detected at very high energies. The emission above 70 GeV of GRB 201216C is modelled together with multiwavelength data within a synchrotron and synchrotron self-Compton (SSC) scenario. We find that SSC can explain the broad-band data well from the optical to the very-high-energy band. For the late-time radio data, a different component is needed to account for the observed emission. Differently from previous GRBs detected in the very-high-energy range, the model for GRB 201216C strongly favours a wind-like medium. The model parameters have values similar to those found in past studies of the afterglows of GRBs detected up to GeV energies.

    DOI: 10.1093/mnras/stad2958

    Scopus

  11. Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data Reviewed

    Abe H., Abe K., Abe S., Acciari V.A., Aguasca-Cabot A., Agudo I., Alvarez Crespo N., Aniello T., Ansoldi S., Antonelli L.A., Aramo C., Arbet-Engels A., Arcaro C., Artero M., Asano K., Aubert P., Baack D., Babić A., Baktash A., Bamba A., Baquero Larriva A., Baroncelli L., Barres De Almeida U., Barrio J.A., Batković I., Baxter J., Becerra González J., Bednarek W., Bernardini E., Bernardos M.I., Bernete Medrano J., Berti A., Besenrieder J., Bhattacharjee P., Biederbeck N., Bigongiari C., Biland A., Bissaldi E., Blanch O., Bonnoli G., Bordas P., Bošnjak , Bulgarelli A., Burelli I., Burmistrov L., Buscemi M., Busetto G., Campoy Ordaz A., Cardillo M., Caroff S., Carosi A., Carosi R., Carrasco M.S., Carretero-Castrillo M., Cassol F., Castro-Tirado A.J., Cauz D., Cerasole D., Ceribella G., Chai Y., Cheng K., Chiavassa A., Chikawa M., Chytka L., Cifuentes A., Cikota S., Colombo E., Contreras J.L., Cornelia A., Cortina J., Costantini H., Covino S., D'Amico G., D'Elia V., Da Vela P., Dalchenko M., Dazzi F., De Angelis A., De Bony De Lavergne M., De Lotto B., De Lucia M., De Menezes R., Del Peral L., Del Popolo A., Deleglise G., Delfino M., Delgado Mendez C., Delgado Mengual J., Della Volpe D., Dellaiera M., Depaoli D., De Angelis A., Di Piano A., Di Pierro F., Di Pilato A., Di Tria R., Di Venere L., Dominik R.M., Dominis Prester D., Donini A.

    Astronomy and Astrophysics   Vol. 680   2023.12

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Astronomy and Astrophysics  

    Aims. Large-Sized Telescope 1 (LST-1), the prototype for the Large-Sized Telescope at the upcoming Cherenkov Telescope Array Observatory, is concluding its commissioning phase at the Observatorio del Roque de los Muchachos on the island of La Palma. The proximity of LST-1 to the two MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes makes it possible to carry out observations of the same gamma-ray events with both systems. Methods. We describe the joint LST-1+MAGIC analysis pipeline and used simultaneous Crab Nebula observations and Monte Carlo simulations to assess the performance of the three-telescope system. The addition of the LST-1 telescope allows for the recovery of events in which one of the MAGIC images is too dim to survive analysis quality cuts. Results. Thanks to the resulting increase in the collection area and stronger background rejection, we found a significant improvement in sensitivity, allowing for the detection of 30% weaker fluxes in the energy range between 200 GeV and 3 TeV. The spectrum of the Crab Nebula, reconstructed in the energy range between ∼60 GeV and ∼10 TeV, is in agreement with previous measurements.

    DOI: 10.1051/0004-6361/202346927

    Scopus

  12. The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars Reviewed

    Smith, D. A. et al.

    Astrophysical Journal   Vol. 958 ( 2 ) page: 191   2023.12

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/acee67

  13. Star tracking for pointing determination of Imaging Atmospheric Cherenkov Telescopes: Application to the Large-Sized Telescope of the Cherenkov Telescope Array Reviewed

    Abe K., Abe S., Aguasca-Cabot A., Agudo I., Alvarez Crespo N., Antonelli L.A., Aramo C., Arbet-Engels A., Cornelia A., Artero M., Asano K., Aubert P., Baktash A., Bamba A., Baquero Larriva A., Baroncelli L., Barres De Almeida U., Barrio J.A., Batkovic I., Baxter J., Becerra González J., Bernardini E., Bernardos M.I., Bernete Medrano J., Berti A., Bhattacharjee P., Biederbeck N., Bigongiari C., Bissaldi E., Blanch O., Bonnoli G., Bordas P., Bulgarelli A., Burelli I., Burmistrov L., Buscemi M., Cardillo M., Caroff S., Carosi A., Cassol F., Cauz D., Ceribella G., Chai Y., Cheng K., Chiavassa A., Chikawa M., Chytka L., Cifuentes A., Contreras J.L., Cortina J., Costantini H., Dalchenko M., De Angelis A., De Bony De Lavergne M., De Lotto B., De Menezes R., Deleglise G., Delgado C., Delgado Mengual J., Della Volpe D., Dellaiera M., Di Piano A., Di Pierro F., Di Tria R., Di Venere L., Díaz C., Dominik R.M., Dominis Prester D., Donini A., Dorner D., Doro M., Elsässer D., Emery G., Escudero J., Fallah Ramazani V., Ferrara G., Ferrarotto F., Fiasson A., Freixas Coromina L., Fröse S., Fukami S., Fukazawa Y., Garcia E., Garcia López R., Gasbarra C., Gasparrini D., Geyer D., Giesbrecht Paiva J., Giglietto N., Giordano F., Giro E., Gliwny P., Godinovic N., Grau R., Green D., Green J., Gunji S., Günther P., Hackfeld J., Hadasch D.

    Astronomy and Astrophysics   Vol. 679   2023.11

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Astronomy and Astrophysics  

    We present a novel approach to the determination of the pointing of Imaging Atmospheric Cherenkov Telescopes (IACTs) using the trajectories of the stars in their camera s field of view. The method starts with the reconstruction of the star positions from the Cherenkov camera data, taking into account the point spread function of the telescope, to achieve a satisfying reconstruction accuracy of the pointing position. A simultaneous fit of all reconstructed star trajectories is then performed with the orthogonal distance regression (ODR) method. ODR allows us to correctly include the star position uncertainties and use the time as an independent variable. Having the time as an independent variable in the fit makes it better suitable for various star trajectories. This method can be applied to any IACT and requires neither specific hardware nor interface or special data-taking mode. In this paper, we use the Large-Sized Telescope (LST) data to validate it as a useful tool to improve the determination of the pointing direction during regular data taking. The simulation studies show that the accuracy and precision of the method are comparable with the design requirements on the pointing accuracy of the LST (=14''). With the typical LST event acquisition rate of 10 kHz, the method can achieve up to 50 Hz pointing monitoring rate, compared to O(1) Hz achievable with standard techniques. The application of the method to the LST prototype (LST-1) commissioning data shows the stable pointing performance of the telescope.

    DOI: 10.1051/0004-6361/202347128

    Scopus

  14. Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope Array Invited International coauthorship

    The Astrophysical Journal   Vol. 956 ( 2 ) page: 80   2023.10

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    DOI: 10.3847/1538-4357/ace89d

  15. Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants Reviewed

    Acero F., Acharyya A., Adam R., Aguasca-Cabot A., Agudo I., Aguirre-Santaella A., Alfaro J., Aloisio R., Crespo N.Á., Batista R.A., Amati L., Amato E., Ambrosi G., Angüner E.O., Aramo C., Arcaro C., Armstrong T., Asano K., Ascasibar Y., Aschersleben J., Backes M., Baktash A., Balazs C., Balbo M., Ballet J., Larriva A.B., Martins V.B., de Almeida U.B., Barrio J.A., Bastieri D., Baxter J.R., Tjus J.B., Benbow W., Bernardos-Martín M.I., Bernete J., Berti A., Bertucci B., Beshley V., Bhattacharjee P., Bhattacharyya S., Biland A., Bissaldi E., Biteau J., Blanch O., Bordas P., Bottacini E., Bregeon J., Brose R., Bucciantini N., Bulgarelli A., Capasso M., Dolcetta R.A.C., Caraveo P., Cardillo M., Carosi R., Casanova S., Cascone E., Cassol F., Catalani F., Cerruti M., Chadwick P., Chaty S., Chen A., Chernyakova M., Chiavassa A., Chudoba J., Coimbra-Araujo C., Conforti V., Contreras J.L., Costa A., Costantini H., Cristofari P., Crocker R., D'Amico G., D'Ammando F., De Angelis A., De Caprio V., de Gouveia Dal Pino E.M., de Ona Wilhelmi E., de Souza V., Delgado C., della Volpe D., Depaoli D., Di Girolamo T., Di Pierro F., Di Tria R., Di Venere L., Diebold S., Djuvsland J.I., Donini A., Doro M., Dos Anjos R.D.C., Dwarkadas V.V., Einecke S., Elsässer D., Emery G., Evoli C., Falceta-Goncalves D., Fedorova E., Fegan S.

    Astroparticle Physics   Vol. 150   2023.8

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Astroparticle Physics  

    The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ-ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ-ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O(100) hours of exposure per source.

    DOI: 10.1016/j.astropartphys.2023.102850

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  16. Fermi-GBM Discovery of GRB 221009A: An Extraordinarily Bright GRB from Onset to Afterglow Reviewed International coauthorship

    Lesage, S. et al.

    The Astrophysical Journal Letters   Vol. 952 ( 2 ) page: L42   2023.8

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    DOI: 10.3847/2041-8213/ace5b4

  17. Multimessenger Characterization of Markarian 501 during Historically Low X-Ray and γ-Ray Activity Reviewed International coauthorship

    Abe, H. et al.

      Vol. 266 ( 2 ) page: 37   2023.6

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    DOI: 10.3847/1538-4365/acc181

  18. AstroPix: CMOS pixels in space Reviewed

    Steinhebel A.L., Caputo R., Fleischhack H., Striebig N., Jadhav M., Suda Y., Luz R., Violette D., Kierans C., Tajima H., Fukazawa Y., Leys R., Perić I., Metcalfe J., Negro M., Perkins J.S.

    Proceedings of Science   Vol. 420   2023.5

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    Space-based gamma-ray telescopes such as the Fermi Large Area Telescope have used single sided silicon strip detectors to measure the position of charged particles produced by incident gamma rays with high resolution. At energies in the Compton regime and below, two dimensional position information within a single detector is required. Double sided silicon strip detectors are one option; however, this technology is difficult to fabricate and large arrays are susceptible to noise. This work outlines the development and implementation of monolithic CMOS active pixel silicon sensors, AstroPix, for use in future gamma-ray telescopes. Based upon detectors designed using the HVCMOS process at the Karlsruhe Institute of Technology, AstroPix has the potential to maintain the high energy and angular resolution required of a medium-energy gamma-ray telescope while reducing noise with the dual detection-and-readout capabilities of a CMOS chip. The status of AstroPix development and testing as well as outlook for application in future telescopes is presented.

    Scopus

  19. Multiwavelength study of the galactic PeVatron candidate LHAASO J2108+5157 Reviewed International coauthorship

    Abe, S. et al.

    Astronomy & Astrophysics   Vol. 673   page: A75   2023.5

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    DOI: 10.1051/0004-6361/202245086

  20. Studies of propagation mechanism of optical crosstalk in silicon photomultipliers Reviewed

    Tajima H., Okumura A., Furuta K.

    Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment   Vol. 1049   2023.4

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    Silicon photomultipliers (SiPMs) are now replacing photomultiplier tubes where low voltage operations, compactness, and cost per channel are important. However, optical crosstalk (OCT) is still one of the major disadvantages of SiPMs since it increases accidental triggers and degrades the accuracy of photon counting. Previously, we reported that OCTs can be suppressed by either thicker or no protection resin coating. Although no resin coating heavily suppresses OCTs, we still observe some OCTs at a few % levels. In this study, we have investigated the properties of OCTs and delayed OCTs for several types of SiPMs with different device sizes, cell sizes, and resin coating thickness. We observe that delayed OCTs have very similar properties compared with OCTs with no resin coating. Furthermore, we find that the sizable amount of delayed OCTs is overlapping with the original pulse and may be treated as OCTs when the delay is less than 8 ns in our analysis. Since the properties and rate of overlaps of delayed OCTs match those of OCTs with no resin coating, we conclude that the remaining OCTs for SiPMs with no coating can be fully explained by overlaps of delayed OCTs.

    DOI: 10.1016/j.nima.2023.168029

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  21. The Fermi-LAT Lightcurve Repository Reviewed International coauthorship

    Abdollahi, S. et al.

    The Astrophysical Journal Supplement Series   Vol. 265 ( 2 ) page: 31   2023.4

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    DOI: 10.3847/1538-4365/acbb6a

  22. MAGIC observations provide compelling evidence of hadronic multi-TeV emission from the putative PeVatron SNR G106.3+2.7 Reviewed

    Abe H., Abe S., Acciari V.A., Agudo I., Aniello T., Ansoldi S., Antonelli L.A., Arbet Engels A., Arcaro C., Artero M., Asano K., Baack D., Babić A., Baquero A., Barres De Almeida U., Barrio J.A., Batković I., Baxter J., Becerra González J., Bednarek W., Bernardini E., Bernardos M., Berti A., Besenrieder J., Bhattacharyya W., Bigongiari C., Biland A., Blanch O., Bonnoli G., Bošnjak , Burelli I., Busetto G., Carosi R., Carretero-Castrillo M., Castro-Tirado A.J., Ceribella G., Chai Y., Chilingarian A., Cikota S., Colombo E., Contreras J.L., Cortina J., Covino S., D'Amico G., D'Elia V., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Del Popolo A., Delfino M., Delgado J., Delgado Mendez C., Depaoli D., Di Pierro F., Di Venere L., Do Souto Espiñeira E., Dominis Prester D., Donini A., Dorner D., Doro M., Elsaesser D., Emery G., Escudero J., Fallah Ramazani V., Fariña L., Fattorini A., Font L., Fruck C., Fukami S., Fukazawa Y., García López R.J., Garczarczyk M., Gasparyan S., Gaug M., Giesbrecht Paiva J.G., Giglietto N., Giordano F., Gliwny P., Godinović N., Grau R., Green D., Green J.G., Hadasch D., Hahn A., Hassan T., Heckmann L., Herrera J., Hrupec D., Hütten M., Imazawa R., Inada T., Iotov R., Ishio K., Jiménez Martínez I., Jormanainen J., Kerszberg D., Kobayashi Y., Kubo H., Kushida J.

    Astronomy and Astrophysics   Vol. 671   2023.3

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    Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capable of accelerating cosmic rays (CRs) to ∼ PeV energies. However, conclusive observational evidence for this has not yet been found. The SNR G106.3+2.7, detected at 1- 100 TeV energies by different γ-ray facilities, is one of the most promising PeVatron candidates. This SNR has a cometary shape, which can be divided into a head and a tail region with different physical conditions. However, in which region the 100 TeV emission is produced has not yet been identified because of the limited position accuracy and/or angular resolution of existing observational data. Additionally, it remains unclear as to whether the origin of the γ-ray emission is leptonic or hadronic. Aims. With the better angular resolution provided by new MAGIC data compared to earlier γ-ray datasets, we aim to reveal the acceleration site of PeV particles and the emission mechanism by resolving the SNR G106.3+2.7 with 0.1 resolution at TeV energies. Methods. We observed the SNR G106.3+2.7 using the MAGIC telescopes for 121.7 h in total - after quality cuts - between May 2017 and August 2019. The analysis energy threshold is ∼0.2 TeV, and the angular resolution is 0.07-0.1. We examined the γ-ray spectra of different parts of the emission, whilst benefitting from the unprecedented statistics and angular resolution at these energies provided by our new data. We also used measurements at other wavelengths such as radio, X-rays, GeV γ-rays, and 10 TeV γ-rays to model the emission mechanism precisely. Results. We detect extended γ-ray emission spatially coincident with the radio continuum emission at the head and tail of SNR G106.3+2.7. The fact that we detect a significant γ-ray emission with energies above 6.0 TeV from only the tail region suggests that the emissions above 10 TeV detected with air shower experiments (Milagro, HAWC, Tibet ASγ and LHAASO) are emitted only from the SNR tail. Under this assumption, the multi-wavelength spectrum of the head region can be explained with either hadronic or leptonic models, while the leptonic model for the tail region is in contradiction with the emission above 10 TeV and X-rays. In contrast, the hadronic model could reproduce the observed spectrum at the tail by assuming a proton spectrum with a cutoff energy of ∼1 PeV for that region. Such high-energy emission in this middle-aged SNR (4-10 kyr) can be explained by considering a scenario where protons escaping from the SNR in the past interact with surrounding dense gases at present. Conclusions. The γ-ray emission region detected with the MAGIC telescopes in the SNR G106.3+2.7 is extended and spatially coincident with the radio continuum morphology. The multi-wavelength spectrum of the emission from the tail region suggests proton acceleration up to ∼PeV, while the emission mechanism of the head region could either be hadronic or leptonic.

    DOI: 10.1051/0004-6361/202244931

    Scopus

  23. The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope: Data Release 3 Reviewed

    Ajello M., Baldini L., Ballet J., Bastieri D., Gonzalez J. Becerra, Bellazzini R., Berretta A., Bissaldi E., Bonino R., Brill A., Bruel P., Buson S., Caputo R., Caraveo P. A., Cheung C. C., Chiaro G., Cibrario N., Ciprini S., Crnogorcevic M., Cutini S., D'Ammando F., De Gaetano S., Di Lalla N., Di Venere L., Dominguez A., Ramazani V. Fallah, Ferrara E. C., Fiori A., Fukazawa Y., Funk S., Fusco P., Gammaldi V, Gargano F., Garrappa S., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guiriec S., Horan D., Hou X., Kayanoki T., Kuss M., Larsson S., Latronico L., Lewis T., Li J., Liodakis I, Longo F., Loparco F., Lott B., Lovellette M. N., Lubrano P., Madejski G. M., Maldera S., Manfreda A., Marti-Devesa G., Mazziotta M. N., Mereu I, Michelson P. F., Mirabal N., Mitthumsiri W., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V, Negro M., Ojha R., Orienti M., Orlando E., Ormes J. F., Pei Z., Pena-Herazo H., Persic M., Pesce-Rollins M., Petrosian V, Pillera R., Poon H., Porter T. A., Principe G., Raino S., Rando R., Rani B., Razzano M., Razzaque S., Reimer A., Reimer O., Scotton L., Serini D., Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Torres D. F., Valverde J., Yassin H., Zaharijas G.

    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   Vol. 263 ( 2 )   2022.12

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    DOI: 10.3847/1538-4365

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  24. Gamma-ray observations of MAXI J1820+070 during the 2018 outburst Reviewed

    Abe, H; Abe, S; Acciari, VA; Aniello, T; Ansoldi, S; Antonelli, LA; Engels, AA; Arcaro, C; Artero, M; Asano, K; Baack, D; Babic, A; Baquero, A; de Almeida, UB; Barrio, JA; Batkovic, ; Baxter, J; González, JB; Bednarek, W; Bernardini, E; Bernardos, M; Berti, A; Besenrieder, J; Bhattacharyya, W; Bigongiari, C; Biland, A; Blanch, O; Bonnoli, G; Bosnjak, Z; Burelli, ; Busetto, G; Carosi, R; Carretero-Castrillo, M; Ceribella, G; Chai, Y; Chilingarian, A; Cikota, S; Colombo, E; Contreras, JL; Cortina, J; Covino, S; D'Amico, G; D'Elia, ; Da Vela, P; Dazzi, F; De Angelis, A; De Lotto, B; Del Popolo, A; Delfino, M; Delgado, J; Mendez, CD; Depaoli, D; Di Pierro, F; Di Venere, L; Prester, DD; Donini, A; Dorner, D; Doro, M; Elsaesser, D; Emery, G; Ramazani, VF; Fariña, L; Fattorini, A; Font, L; Fruck, C; Fukami, S; Fukazawa, Y; López, RJG; Garczarczyk, M; Gasparyan, S; Gaug, M; Paiva, JGG; Giglietto, N; Giordano, F; Gliwny, P; Godinovic, N; Grau, R; Green, D; Green, JG; Hadasch, D; Hahn, A; Hassan, T; Heckmann, L; Herrera, J; Hoang, J; Hrupec, D; Hütten, M; Imazawa, R; Inada, T; Iotov, R; Ishio, K; Martínez, IJ; Jormanainen, J; Kerszberg, D; Kobayashi, Y; Kubo, H; Kushida, J; Lamastra, A; Lelas, D; Leone, F; Lindfors, E; Linhoff, L; Lombardi, S; Longo, F; López-Coto, R; López-Moya, M; López-Oramas, A; Loporchio, S; Lorini, A; Lyard, E; Fraga, BMD; Majumdar, P; Makariev, M; Maneva, G; Mang, N; Manganaro, M; Mangano, S; Mannheim, K; Mariotti, M; Martínez, M; Aguilar, AM; Mazin, D; Menchiari, S; Mender, S; Micanovic, S; Miceli, D; Miener, T; Miranda, JM; Mirzoyan, R; Molina, E; Mondal, HA; Moralejo, A; Morcuende, D; Moreno, ; Nakamori, T; Nanci, C; Nava, L; Neustroev, ; Rosillo, MN; Nigro, C; Nilsson, K; Nishijima, K; Ekoume, TN; Noda, K; Nozaki, S; Ohtani, Y; Oka, T; Okumura, A; Otero-Santos, J; Paiano, S; Palatiello, M; Paneque, D; Paoletti, R; Paredes, JM; Pavletic, L; Persic, M; Pihet, M; Pirola, G; Podobnik, F; Moroni, PGP; Prandini, E; Principe, G; Priyadarshi, C; Puljak, ; Rhode, W; Ribó, M; Rico, J; Righi, C; Rugliancich, A; Sahakyan, N; Saito, T; Sakurai, S; Satalecka, K; Saturni, FG; Schleicher, B; Schmidt, K; Schmuckermaier, F; Schubert, JL; Schweizer, T; Sitarek, J; Sliusar, ; Sobczynska, D; Spolon, A; Stamerra, A; Striskovic, J; Strom, D; Strzys, M; Suda, Y; Suric, T; Tajima, H; Takahashi, M; Takeishi, R; Tavecchio, F; Temnikov, P; Terauchi, K; Terzic, T; Teshima, M; Tosti, L; Truzzi, S; Tutone, A; Ubach, S; van Scherpenberg, J; Acosta, MV; Ventura, S; Verguilov, V; Viale, ; Vigorito, CF; Vitale, V; Vovk, ; Walter, R; Will, M; Wunderlich, C; Yamamoto, T; Zaric, D; Abdalla, H; Aharonian, F; Benkhali, FA; Angüner, EO; Ashkar, H; Backes, M; Baghmanyan, ; Martins, VB; Batzofin, R; Becherini, Y; Berge, D; Bernlöhr, K; Böttcher, M; Boisson, C; Bolmont, J; de Lavergne, MD; Bradascio, F; Breuhaus, M; Brose, R; Brun, F; Bulik, T; Bylund, T; Cangemi, F; Caroff, S; Casanova, S; Cerruti, M; Chand, T; Chandra, S; Chen, A; Chibueze, OU; Cotter, G; Cristofari, P; Mbarubucyeye, JD; Devin, J; Djannati-Ataï, A; Dmytriiev, A; Egberts, K; Ernenwein, JP; Fiasson, A; de Clairfontaine, GF; Fontaine, G; Füssling, M; Funk, S; Gabici, S; Ghafourizadeh, S; Giavitto, G; Glawion, D; Glicenstein, JF; Goswami, P; Grolleron, G; Hinton, JA; Hörbe, M; Hoischen, C; Holch, TL; Holler, M; Horns, D; Huang, ZQ; Jamrozy, M; Jankowsky, F; Joshi, ; Jung-Richardt, ; Kasai, E; Katarzynski, K; Katz, U; Khélifi, B; Kluzniak, W; Komin, N; Kosack, K; Kostunin, D; Lang, RG; Le Stum, S; Lemière, A; Lemoine-Goumard, M; Lenain, JP; Leuschner, F; Lohse, T; Luashvili, A; Lypova, ; Mackey, J; Majumdar, J; Malyshev, D; Malyshev, D; Marandon, ; Marchegiani, P; Martí-Devesa, G; Marx, R; Maurin, G; Meyer, M; Mitchell, A; Moderski, R; Mohrmann, L; Montanari, A; Moulin, E; Muller, J; Murach, T; Nakashima, K; de Naurois, M; Nayerhoda, A; Niemiec, J; Noel, AP; O'Brien, P; Ohm, S; Olivera-Nieto, L; Wilhelmi, ED; Ostrowski, M; Panny, S; Panter, M; Parsons, RD; Poireau, ; Prokhorov, DA; Prokoph, H; Pühlhofer, G; Punch, M; Quirrenbach, A; Reichherzer, P; Reimer, A; Reimer, O; Renaud, M; Rieger, F; Rowell, G; Rudak, B; Ricarte, HR; Ruiz-Velasco, E; Sahakian, ; Salzmann, H; Santangelo, A; Sasaki, M; Schäfer, J; Schüssler, F; Schutte, HM; Schwanke, U; Shapopi, JNS; Sol, H; Specovius, A; Spencer, S; Stawarz, L; Steenkamp, R; Steinmassl, S; Steppa, C; Sushch, ; Suzuki, H; Takahashi, T; Tanaka, T; Thorpe-Morgan, C; Tluczykont, M; Tomankova, L; Tsuji, N; Uchiyama, Y; van Eldik, C; van Soelen, B; Vecchi, M; Veh, J; Venter, C; Vink, J; Wagner, SJ; White, R; Wierzcholska, A; Wong, YW; Yusafzai, A; Zacharias, M; Zanin, R; Zargaryan, D; Zdziarski, AA; Zech, A; Zhu, SJ; Zouari, S; Zywucka, N; Acharyya, A; Adams, CB; Batista, P; Benbow, W; Capasso, M; Christiansen, JL; Chromey, AJ; Errando, M; Falcone, A; Feng, Q; Finley, JP; Foote, GM; Fortson, L; Furniss, A; Gent, A; Hanlon, WE; Hervet, O; Holder, J; Hona, B; Humensky, TB; Jin, W; Kaaret, P; Kertzman, M; Kherlakian, M; Kleiner, TK; Kumar, S; Lang, MJ; Lundy, M; Maier, G; McGrath, CE; Millis, J; Moriarty, P; Mukherjee, R; O'Brien, S; Ong, RA; Park, N; Patel, SR; Pfrang, K; Pohl, M; Pueschel, E; Quinn, J; Ragan, K; Reynolds, PT; Ribeiro, D; Roache, E; Ryan, JL; Sadeh, ; Saha, L; Santander, M; Sembroski, GH; Shang, R; Splettstoesser, M; Tak, D; Tucci, J; Weinstein, A; Williams, DA; Williamson, TJ; Bosch-Ramon, ; Celma, C; Linares, M; Russell, DM; Sala, G

    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY   Vol. 517 ( 4 ) page: 4736 - 4751   2022.12

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    MAXI J1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018 March to October, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 h of observations of the MAXI J1820+070 outburst with the H.E.S.S., MAGIC and VERITAS experiments at energies above 200 GeV are presented, together with Fermi-LAT data between 0.1 and 500 GeV, and multiwavelength observations from radio to X-rays. Gamma-ray emission is not detected from MAXI J1820+070, but the obtained upper limits and the multiwavelength data allow us to put meaningful constraints on the source properties under reasonable assumptions regarding the non-thermal particle population and the jet synchrotron spectrum. In particular, it is possible to show that, if a high-energy (HE) gamma-ray emitting region is present during the hard state of the source, its predicted flux should be at most a factor of 20 below the obtained Fermi-LAT upper limits, and closer to them for magnetic fields significantly below equipartition. During the state transitions, under the plausible assumption that electrons are accelerated up to ∼500 GeV, the multiwavelength data and the gamma-ray upper limits lead consistently to the conclusion that a potential HE and very-HE gamma-ray emitting region should be located at a distance from the BH ranging between 1011 and 1013 cm. Similar outbursts from low-mass X-ray binaries might be detectable in the near future with upcoming instruments such as CTA.

    DOI: 10.1093/mnras/stac2686

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  25. All-sky Medium Energy Gamma-ray Observatory eXplorer mission concept Reviewed

    Caputo Regina, Ajello Marco, Kierans Carolyn A., Perkins Jeremy S., Racusin Judith L., Baldini Luca, Baring Matthew G., Bissaldi Elisabetta, Burns Eric, Cannady Nicholas, Charles Eric, da Silva Rui M. Curado, Fang Ke, Fleischhack Henrike, Fryer Chris, Fukazawa Yasushi, Grove J. Eric, Hartmann Dieter, Howell Eric J., Jadhav Manoj, Karwin Christopher M., Kocevski Daniel, Kurahashi Naoko, Latronico Luca, Lewis Tiffany R., Leys Richard, Lien Amy, Marcotulli Lea, Martinez-Castellanos Israel, Mazziotta Mario Nicola, McEnery Julie, Metcalfe Jessica, Murase Kohta, Negro Michela, Parker Lucas, Phlips Bernard, Prescod-Weinstein Chanda, Razzaque Soebur, Shawhan Peter S., Sheng Yong, Shutt Tom A., Shy Daniel, Sleator Clio, Steinhebel Amanda L., Striebig Nicolas, Suda Yusuke, Tak Donggeun, Tajima Hiro, Valverde Janeth, Venters Tonia M., Wadiasingh Zorawar, Woolf Richard S., Wulf Eric A., Zhang Haocheng, Zoglauer Andreas

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 8 ( 4 )   2022.10

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    DOI: 10.1117/1.JATIS.8.4.044003

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  26. Search for New Cosmic-Ray Acceleration Sites within the 4FGL Catalog Galactic Plane Sources Reviewed International coauthorship International journal

    Abdollahi, S; Acero, F; Ackermann, M; Baldini, L; Ballet, J; Barbiellini, G; Bastieri, D; Bellazzini, R; Berenji, B; Berretta, A; Bissaldi, E; Blandford, RD; Bonino, R; Bruel, P; Buson, S; Cameron, RA; Caputo, R; Caraveo, PA; Castro, D; Chiaro, G; Cibrario, N; Ciprini, S; Coronado-Blázquez, J; Crnogorcevic, M; Cutini, S; D'Ammando, F; De Gaetano, S; Di Lalla, N; Dirirsa, F; Di Venere, L; Domínguez, A; Fegan, SJ; Fiori, A; Fleischhack, H; Franckowiak, A; Fukazawa, Y; Fusco, P; Gammaldi, V; Gargano, F; Gasparrini, D; Giacchino, F; Giglietto, N; Giordano, F; Giroletti, M; Glanzman, T; Green, D; Grenier, IA; Grondin, MH; Guiriec, S; Gustafsson, M; Harding, AK; Hays, E; Hewitt, JW; Horan, D; Hou, X; Jóhannesson, G; Kayanoki, T; Kerr, M; Kuss, M; Larsson, S; Latronico, L; Lemoine-Goumard, M; Li, J; Longo, F; Loparco, F; Lubrano, P; Maldera, S; Malyshev, D; Manfreda, A; Martí-Devesa, G; Mazziotta, MN; Mereu, I; Michelson, PF; Mirabal, N; Mitthumsiri, W; Mizuno, T; Monzani, ME; Morselli, A; Moskalenko, IV; Nuss, E; Omodei, N; Orienti, M; Orlando, E; Ormes, JF; Paneque, D; Pei, Z; Persic, M; Pesce-Rollins, M; Pillera, R; Poon, H; Porter, TA; Principe, G; Rainò, S; Rando, R; Rani, B; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Reposeur, T; Sánchez-Conde, M; Parkinson, PMS; Scotton, L; Serini, D; Sgrò, C; Siskind, EJ; Spandre, G; Spinelli, P; Sueoka, K; Suson, DJ; Tajima, H; Tak, D; Thayer, JB; Torres, DF; Troja, E; Valverde, J; Wadiasingh, Z; Wood, K; Zaharijas, G

    ASTROPHYSICAL JOURNAL   Vol. 933 ( 2 )   2022.7

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    DOI: 10.3847/1538-4357/ac704f

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  27. Incremental Fermi Large Area Telescope Fourth Source Catalog Reviewed International coauthorship International journal

    Abdollahi, S; Acero, F; Baldini, L; Ballet, J; Bastieri, D; Bellazzini, R; Berenji, B; Berretta, A; Bissaldi, E; Blandford, RD; Bloom, E; Bonino, R; Brill, A; Britto, RJ; Bruel, P; Burnett, TH; Buson, S; Cameron, RA; Caputo, R; Caraveo, PA; Castro, D; Chaty, S; Cheung, CC; Chiaro, G; Cibrario, N; Ciprini, S; Coronado-Blázquez, J; Crnogorcevic, M; Cutini, S; D'Ammando, F; De Gaetano, S; Digel, SW; Di Lalla, N; Dirirsa, F; Di Venere, L; Domínguez, A; Ramazani, VF; Fegan, SJ; Ferrara, EC; Fiori, A; Fleischhack, H; Franckowiak, A; Fukazawa, Y; Funk, S; Fusco, P; Galanti, G; Gammaldi, V; Gargano, F; Garrappa, S; Gasparrini, D; Giacchino, F; Giglietto, N; Giordano, F; Giroletti, M; Glanzman, T; Green, D; Grenier, IA; Grondin, MH; Guillemot, L; Guiriec, S; Gustafsson, M; Harding, AK; Hays, E; Hewitt, JW; Horan, D; Hou, X; Jóhannesson, G; Karwin, C; Kayanoki, T; Kerr, M; Kuss, M; Landriu, D; Larsson, S; Latronico, L; Lemoine-Goumard, M; Li, J; Liodakis, I; Longo, F; Loparco, F; Lott, B; Lubrano, P; Maldera, S; Malyshev, D; Manfreda, A; Martí-Devesa, G; Mazziotta, MN; Mereu, I; Meyer, M; Michelson, PF; Mirabal, N; Mitthumsiri, W; Mizuno, T; Moiseev, AA; Monzani, ME; Morselli, A; Moskalenko, IV; Negro, M; Nuss, E; Omodei, N; Orienti, M; Orlando, E; Paneque, D; Pei, Z; Perkins, JS; Persic, M; Pesce-Rollins, M; Petrosian, V; Pillera, R; Poon, H; Porter, TA; Principe, G; Rainò, S; Rando, R; Rani, B; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Reposeur, T; Sánchez-Conde, M; Parkinson, PMS; Scotton, L; Serini, D; Sgrò, C; Siskind, EJ; Smith, DA; Spandre, G; Spinelli, P; Sueoka, K; Suson, DJ; Tajima, H; Tak, D; Thayer, JB; Thompson, DJ; Torres, DF; Troja, E; Valverde, J; Wood, K; Zaharijas, G

    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   Vol. 260 ( 2 )   2022.6

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    DOI: 10.3847/1538-4365/ac6751

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  28. Design and performance of the prototype Schwarzschild-Couder telescope camera Reviewed International coauthorship International journal

    Adams, CB; Ambrosi, G; Ambrosio, M; Aramo, C; Arlen, T; Benbow, W; Bertucci, B; Bissaldi, E; Biteau, J; Bitossi, M; Boiano, A; Bonavolontà, C; Bose, R; Bouvier, A; Buscemi, M; Brill, A; Brown, AM; Buckley, JH; Canestrari, R; Capasso, M; Caprai, M; Coppi, P; Covault, CE; Depaoli, D; Di Venere, L; Errando, M; Fegan, S; Feng, Q; Fiandrini, E; Furniss, A; Garczarczyk, M; Gent, A; Giglietto, N; Giordano, F; Giro, E; Halliday, R; Hervet, O; Hughes, G; Incardona, S; Humensky, TB; Ionica, M; Jin, WD; Johnson, CA; Kieda, D; Krennrich, F; Kuznetsov, A; Lapington, J; Licciulli, F; Loporchio, S; Marsella, G; Masone, V; Meagher, K; Meures, T; Mode, BAW; Mognet, SAI; Mukherjee, R; Okumura, A; Pantaleo, FR; Paoletti, R; Di Pierro, F; Ribeiro, D; Riitano, L; Roache, E; Ross, D; Rousselle, J; Rugliancich, A; Santander, M; Schneider, M; Schoorlemmer, H; Shang, RY; Stevenson, B; Stiaccini, L; Tajima, H; Taylor, LP; Thornhill, J; Tosti, L; Tripodo, G; Vagelli, V; Valentino, M; Vandenbroucke, J; Vassiliev, VV; Wakely, SP; Watson, JJ; White, R; Wilcox, P; Williams, DA; Wood, M; Yu, P; Zink, A

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 8 ( 1 )   2022.1

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    The prototype Schwarzschild-Couder Telescope (pSCT) is a candidate for a medium-sized telescope in the Cherenkov Telescope Array. The pSCT is based on a dual-mirror optics design that reduces the plate scale and allows for the use of silicon photomultipliers as photodetectors. The prototype pSCT camera currently has only the central sector instrumented with 25 camera modules (1600 pixels), providing a 2.68-deg field of view (FoV). The camera electronics are based on custom TARGET (TeV array readout with GSa/s sampling and event trigger) application-specific integrated circuits. Field programmable gate arrays sample incoming signals at a gigasample per second. A single backplane provides camera-wide triggers. An upgrade of the pSCT camera that will fully populate the focal plane is in progress. This will increase the number of pixels to 11,328, the number of backplanes to 9, and the FoV to 8.04 deg. Here, we give a detailed description of the pSCT camera, including the basic concept, mechanical design, detectors, electronics, current status, and first light.

    DOI: 10.1117/1.JATIS.8.1.014007

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  29. AstroPix: Novel monolithic active pixel silicon sensors for future gamma-ray telescopes Reviewed

    Steinhebel, AL; Fleischhack, H; Striebig, N; Jadhav, M; Suda, Y; Luz, R; Kierans, C; Caputo, R; Tajima, H; Leys, R; Peric, I; Metcalfe, J; Perkins, JS

    SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY   Vol. 12181   2022

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    Space-based γ-ray telescopes such as the Fermi Large Area Telescope have used single sided silicon strip detectors to track secondary charged particles produced by primary γ-rays with high resolution. At the lower energies targeted by keV-MeV telescopes, two dimensional position information within a single detector is required for event reconstruction - especially in the Compton regime. This work describes the development of monolithic CMOS active pixel silicon sensors – AstroPix – as a novel technology for use in future γ-ray telescopes. Based upon sensors (ATLASPix) designed for use in the ATLAS detector at the Large Hadron Collider, AstroPix has the potential to maintain high performance while reducing noise with low power consumption. This is achieved with the dual detection and readout capabilities in each CMOS pixel. The status of AstroPix development and testing, as well as outlook for future testing and application, will be presented.

    DOI: 10.1117/12.2630405

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  30. The Small-Sized Telescope of CTAO Reviewed

    Tagliaferri, G; Antonelli, A; Arnesen, T; Aschersleben, J; Attinà, P; Balbo, M; Bang, S; Barcelo, M; Baryshev, A; Bellassai, G; Berge, D; Bicknell, C; Bigongiari, C; Bonnoli, G; Bouley, F; Brown, A; Bulgarelli, A; Cappi, M; Caraveo, P; Caschera, S; Chadwick, P; Conte, F; Cotter, G; Cristofari, P; De Frondat, F; Dal Pino, ED; De Simone, N; Depaoli, D; Dournaux, JL; Duffy, C; Einecke, S; Fermino, C; Funk, S; Gargano, C; Giavitto, G; Giuliani, A; Greenshaw, T; Hinton, J; Huet, JM; Iovenitti, S; La Palombara, N; Lapington, J; Laporte, P; Leach, S; Lessio, L; Leto, G; Lloyd, S; Lucarelli, F; Lombardi, S; Macchi, A; Martinetti, E; Miccichè, A; Millul, R; Mineo, T; Mitsunari, T; Nayak, A; Nicotra, G; Okumura, A; Pareschi, G; Penno, M; Prokoph, H; Rebert, E; Righi, C; Rulten, C; Russo, F; Sanchez, RZ; Saturni, FG; Schaefer, J; Schwab, B; Scuderi, S; Sironi, G; Sliusar, V; Sol, H; Spencer, S; Stamerra, A; Tajima, H; Tavecchio, F; Tosti, G; Trois, A; Vecchi, M; Vercellone, S; Vink, J; Walter, R; Watson, J; White, R; Zanin, R; Zampieri, L; Zech, A; Zink, A

    GROUND-BASED AND AIRBORNE TELESCOPES IX   Vol. 12182   2022

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    DOI: 10.1117/12.2627956

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  31. SOlar Neutron and Gamma-ray Spectroscopy Mission (SONGS) Reviewed

    Yamaoka, K; Tajima, H; Miyata, K; Usami, M; Watabe, T; Matsushita, K; Ito, K; Nakazawa, K; Masuda, S; Tani, K; Arai, M; Hatori, S; Kume, K; Mizushima, S; Takahashi, H; Watanabe, K

    SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY   Vol. 12181   2022

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    The SOlar Neutron and Gamma-ray Spectroscopy (SONGS) mission is a 3U cubesat dedicated for detecting neutrons and gamma-rays associated with intense solar flares. Solar neutron observations have not been in progress because ground-based observations are affected by attenuation in the Earth atmosphere, and there is no dedicated mission in space at present. Hence, we are now developing in collaboration between science and engineering people at universities, and preparing for launch around 2024 during the next solar maximum. The SONGS carries a novel radiation detector which consists of multi-layered plastic scintillator bars and GAGG(Ce) scintillator array so that it can determine energies for both neutrons and gamma-rays. In total 704 signals from Silicon photo-multipliers (SiPMs) are processed by 45 ASICs with very low power consumption, and realized within limited resources. In this presentation, we will describe scientific motivation, mission and instrument overview, and results from the bread-board model (BBM).

    DOI: 10.1117/12.2629131

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  32. High-energy gamma-rays and neutrons observed in very impulsive solar flare on 2012 June 3 Reviewed

    Kamiya, K; Koga, K; Masuda, S; Matsumoto, H; Muraki, Y; Okudaira, O; Shibata, S; Tajima, H; Tanaka, Y; Yamamoto, T; Watanabe, K

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 73 ( 6 ) page: 1443 - 1469   2021.12

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    An impulsive solar flare was observed on 2012 June 3 by the Geostationary Operational Environment Satellite. In this flare, a salient feature was recognized whereby high-energy ions were accelerated to a few GeV within one minute. Associated with this flare, high-energy gamma-rays as well as high-energy neutrons were detected by the Space Environment Data Acquisition equipment onboard the International Space Station. A remarkable feature found of this event was an exceedingly high n/γ-ratio observed between the intensities of high-energy neutrons and gamma-rays. To understand a high n/γ-ratio of about 600, the interaction processes between the accelerated ions and ambient solar atmosphere were simulated for various test cases, taking into account the magnetic field of the photosphere. The simulation was extended by using the GEANT4 code and it was shown that the observed results could be reproduced under certain conditions selected for the actual interaction process. The results suggest that helium and C, N, and O ions were predominantly accelerated in this flare, and that high-energy gamma-rays and neutrons were produced by interactions between the accelerated ions and the ambient gas. As a result, a high n/γ-ratio was produced.

    DOI: 10.1093/pasj/psab089

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  33. Catalog of Long-term Transient Sources in the First 10 yr of Fermi-LAT Data Reviewed

    Baldini, L; Ballet, J; Bastieri, D; Gonzalez, JB; Bellazzini, R; Berretta, A; Bissaldi, E; Blandford, RD; Bloom, ED; Bonino, R; Bottacini, E; Bruel, P; Buson, S; Cameron, RA; Caraveo, PA; Cavazzuti, E; Chen, S; Chiaro, G; Ciangottini, D; Cibario, N; Ciprini, S; Orestano, PC; Crnogorcevic, M; Cutini, S; D'Ammando, F; Luque, PD; de Palma, F; Digel, SW; Di Lalla, N; Dirirsa, F; Di Venere, L; Domínguez, A; Fiori, A; Fleischhack, H; Franckowiak, A; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gasparrini, D; Germani, S; Giglietto, N; Giordano, F; Giroletti, M; Green, D; Grenier, IA; Griffin, S; Guiriec, S; Gustafsson, M; Hewitt, JW; Horan, D; Imazawa, R; Jóhannesson, G; Kerr, M; Kocevski, D; Kuss, M; Larsson, S; Latronico, L; Li, J; Liodakis, I; Longo, F; Loparco, F; Lovellette, MN; Lubrano, P; Maldera, S; Manfreda, A; Martí-Devesa, G; Matake, H; Mazziotta, MN; Mereu, I; Meyer, M; Mirabal, N; Mitthumsiri, W; Mizuno, T; Monzani, ME; Morselli, A; Moskalenko, IV; Nagasawa, S; Negro, M; Ojha, R; Orienti, M; Orlando, E; Palatiello, M; Paliya, V; Paneque, D; Pei, Z; Persic, M; Pesce-Rollins, M; Petrosian, V; Poon, H; Porter, TA; Principe, G; Racusin, JL; Rainò, S; Rando, R; Rani, B; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Parkinson, PMS; Scotton, L; Serini, D; Sgrò, C; Siskind, EJ; Spandre, G; Spinelli, P; Suson, DJ; Tajima, H; Tak, D; Torres, DF; Tosti, G; Troja, E; Wood, K; Yassine, M; Zaharijas, G

    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   Vol. 256 ( 1 )   2021.9

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    DOI: 10.3847/1538-4365/ac072a

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  34. Fermi Large Area Telescope Performance after 10 Years of Operation Reviewed International coauthorship

    Ajello, M; Atwood, WB; Axelsson, M; Bagagli, R; Bagni, M; Baldini, L; Bastieri, D; Bellardi, F; Bellazzini, R; Bissaldi, E; Bloom, ED; Bonino, R; Bregeon, J; Brez, A; Bruel, P; Buehler, R; Buson, S; Cameron, RA; Caraveo, PA; Cavazzuti, E; Ceccanti, M; Chen, S; Cheung, CC; Ciprini, S; Cognard, I; Cohen-Tanugi, J; Cutini, S; D'Ammando, F; Luque, PD; de Palma, F; Digel, SW; Dirirsa, F; Di Lalla, N; Di Venere, L; Domínguez, A; Fabiani, D; Ferrara, EC; Fiori, A; Foglia, G; Fukazawa, Y; Fusco, P; Gargano, F; Gasparrini, D; Giroletti, M; Glanzman, T; Green, D; Griffin, S; Grondin, MH; Grove, JE; Guillemot, L; Guiriec, S; Gustafsson, M; Hays, E; Horan, D; Jóhannesson, G; Johnson, TJ; Kamae, T; Kerr, M; Kuss, M; Larsson, S; Latronico, L; Lemoine-Goumard, M; Li, J; Liodakis, I; Longo, F; Loparco, F; Lovellette, MN; Lubrano, P; Maldera, S; Manfreda, A; Martí-Devesa, G; Mazziotta, MN; Menon, N; Mereu, I; Meyer, M; Michelson, PF; Minuti, M; Mitthumsiri, W; Mizuno, T; Mongelli, M; Monzani, ME; Moskalenko, IV; Negro, M; Nuss, E; Ojha, R; Orienti, M; Orlando, E; Paccagnella, A; Paliya, VS; Paneque, D; Pei, Z; Perkins, JS; Pesce-Rollins, M; Pinchera, M; Piron, F; Poon, H; Porter, TA; Primavera, R; Principe, G; Racusin, JL; Rainò, S; Rando, R; Rani, B; Rapposelli, E; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Russell, JJ; Saggini, N; Parkinson, PMS; Scolieri, N; Serini, D; Sgrò, C; Siskind, EJ; Smith, DA; Spandre, G; Spinelli, P; Suson, DJ; Tajima, H; Thayer, JG; Thompson, DJ; Tibaldo, L; Torres, DF; Tosti, G; Valverde, J; Vigiani, L; Zaharijas, G

    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   Vol. 256 ( 1 )   2021.9

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    DOI: 10.3847/1538-4365/ac0ceb

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  35. High-energy emission from a magnetar giant flare in the Sculptor galaxy Reviewed

    Ajello, M; Atwood, WB; Axelsson, M; Baldini, L; Barbiellini, G; Baring, MG; Bastieri, D; Bellazzini, R; Berretta, A; Bissaldi, E; Blandford, RD; Bonino, R; Bregeon, J; Bruel, P; Buehler, R; Burns, E; Buson, S; Cameron, RA; Caraveo, PA; Cavazzuti, E; Chen, S; Cheung, CC; Chiaro, G; Ciprini, S; Costantin, D; Crnogorcevic, M; Cutini, S; D'Ammando, F; Luque, PD; de Palma, F; Digel, SW; Di Lalla, N; Di Venere, L; Dirirsa, FF; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Giglietto, N; Gill, R; Giordano, F; Giroletti, M; Granot, J; Green, D; Grenier, IA; Griffin, S; Guiriec, S; Hays, E; Horan, D; Jóhannesson, G; Kerr, M; Kovacevic, M; Kuss, M; Larsson, S; Latronico, L; Li, J; Longo, F; Loparco, F; Lovellette, MN; Lubrano, P; Maldera, S; Manfreda, A; Martí-Devesa, G; Mazziotta, MN; McEnery, JE; Mereu, I; Michelson, PF; Mizuno, T; Monzani, ME; Morselli, A; Moskalenko, IV; Negro, M; Omodei, N; Orienti, M; Orlando, E; Paliya, VS; Paneque, D; Pei, Z; Pesce-Rollins, M; Piron, F; Poon, H; Porter, TA; Principe, G; Racusin, JL; Rainò, S; Rando, R; Rani, B; Razzaque, S; Reimer, A; Reimer, O; Parkinson, PMS; Scargle, JD; Scotton, L; Serini, D; Sgrò, C; Siskind, EJ; Spandre, G; Spinelli, P; Tajima, H; Takahashi, MN; Tak, D; Torres, DF; Tosti, G; Troja, E; Wadiasingh, Z; Wood, K; Yassine, M; Yusafzai, A; Zaharijas, G

    NATURE ASTRONOMY   Vol. 5 ( 4 ) page: 385 - +   2021.4

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    Magnetars are the most highly magnetized neutron stars in the cosmos (with magnetic field 1013–1015 G). Giant flares from magnetars are rare, short-duration (about 0.1 s) bursts of hard X-rays and soft γ rays1,2. Owing to the limited sensitivity and energy coverage of previous telescopes, no magnetar giant flare has been detected at gigaelectronvolt (GeV) energies. Here, we report the discovery of GeV emission from a magnetar giant flare on 15 April 2020 (refs. 3,4 and A. J. Castro-Tirado et al., manuscript in preparation). The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope detected GeV γ rays from 19 s until 284 s after the initial detection of a signal in the megaelectronvolt (MeV) band. Our analysis shows that these γ rays are spatially associated with the nearby (3.5 megaparsecs) Sculptor galaxy and are unlikely to originate from a cosmological γ-ray burst. Thus, we infer that the γ rays originated with the magnetar giant flare in Sculptor. We suggest that the GeV signal is generated by an ultra-relativistic outflow that first radiates the prompt MeV-band photons, and then deposits its energy far from the stellar magnetosphere. After a propagation delay, the outflow interacts with environmental gas and produces shock waves that accelerate electrons to very high energies; these electrons then emit GeV γ rays as optically thin synchrotron radiation. This observation implies that a relativistic outflow is associated with the magnetar giant flare, and suggests the possibility that magnetars can power some short γ-ray bursts.

    DOI: 10.1038/s41550-020-01287-8

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  36. Detection of the Crab Nebula with the 9.7 m prototype Schwarzschild-Couder telescope Reviewed

    Adams, CB; Alfaro, R; Ambrosi, G; Ambrosio, M; Aramo, C; Arlen, T; Batista, PI; Benbow, W; Bertucci, B; Bissaldi, E; Biteau, J; Bitossi, M; Boiano, A; Bonavolontà, C; Bose, R; Bouvier, A; Brill, A; Brown, AM; Buckley, JH; Byrum, K; Cameron, RA; Canestrari, R; Capasso, M; Caprai, M; Covault, CE; Depaoli, D; Errando, M; Fegan, S; Feng, Q; Fiandrini, E; Foote, G; Fortin, P; Funk, S; Furniss, A; Garfias, F; Gent, A; Giglietto, N; Giordano, F; Giro, E; González, MM; Guarino, V; Halliday, R; Hervet, O; Holder, J; Hughes, G; Humensky, TB; Ionica, M; Iriarte, A; Jin, W; Johnson, CA; Kaaret, P; Kieda, D; Kim, B; Kuznetsov, A; Lapington, JS; Licciulli, F; Loporchio, S; Masone, V; Meagher, K; Meures, T; Mode, BAW; Mognet, SAI; Mukherjee, R; Nguyen, T; Nieto, D; Okumura, A; Otte, N; La Palombara, N; Pantaleo, FR; Paoletti, R; Pareschi, G; Petrashyk, A; Di Pierro, F; Pueschel, E; Reynolds, PT; Ribeiro, D; Richards, G; Roache, E; Ross, D; Rousselle, J; Rugliancich, A; Ruíz-Díaz-Soto, J; Santander, M; Schlenstedt, S; Schneider, M; Scuderi, S; Shang, R; Sironi, G; Stevenson, B; Stiaccini, L; Tajima, H; Taylor, LP; Thornhill, J; Tosti, L; Tovmassian, G; Vagelli, V; Valentinoa, M; Vandenbroucke, J; Vassiliev, VV; Di Venere, L; Wakely, SP; Watson, JJ; White, R; Wilcoxa, P; Williams, DA; Wood, M; Yu, P; Zink, A

    ASTROPARTICLE PHYSICS   Vol. 128   2021.3

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    The Schwarzschild-Couder Telescope (SCT) is a telescope concept proposed for the Cherenkov Telescope Array. It employs a dual-mirror optical design to remove comatic aberrations over an 8∘ field of view, and a high-density silicon photomultiplier camera (with a pixel resolution of 4 arcmin) to record Cherenkov emission from cosmic ray and gamma-ray initiated particle cascades in the atmosphere. The prototype SCT (pSCT), comprising a 9.7 m diameter primary mirror and a partially instrumented camera with 1536 pixels, has been constructed at the Fred Lawrence Whipple Observatory. The telescope was inaugurated in January 2019, with commissioning continuing throughout 2019. We describe the first campaign of observations with the pSCT, conducted in January and February of 2020, and demonstrate the detection of gamma-ray emission from the Crab Nebula with a statistical significance of 8.6σ.

    DOI: 10.1016/j.astropartphys.2021.102562

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  37. Silicon photomultiplier (Si-PM) comparisons for low-energy gamma ray readouts with BGO and CsI (Tl) scintillators Reviewed

    Takahashi, H; Hirade, N; Uchida, N; Hirose, K; Mizuno, T; Fukazawa, Y; Yamaoka, K; Tajima, H; Ohno, M

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 989   2021.2

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    DOI: 10.1016/j.nima.2020.164945

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  38. Performance evaluation of GAGG(Ce)/LFS scintillator plus MPPC array readout with ASIC Reviewed

    Nobashi, D; Yamaoka, K; Tajima, H; Ito, K

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 986   2021.1

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    DOI: 10.1016/j.nima.2020.164811

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  39. Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA Reviewed International coauthorship International journal

    Adams, CB; Ambrosi, G; Ambrosio, M; Aramo, C; Batista, PI; Benbow, W; Bertucci, B; Bissaldi, E; Bitossi, M; Boiano, A; Bonavolontà, C; Bose, R; Brill, A; Brown, AM; Buckley, JH; Canestrari, R; Capasso, M; Caprai, M; Covault, CE; De Paoli, D; Di Venere, L; Errando, M; Fegan, S; Feng, Q; Fiandrini, E; Furniss, A; Gent, A; Giglietto, N; Giordano, F; Giro, E; Halliday, R; Hervet, O; Holder, J; Humensky, TB; Incardona, S; Ionica, M; Jin, W; Kieda, DB; Licciulli, F; Loporchio, S; Marsella, G; Masone, V; Meagher, K; Meures, T; Mode, BAW; Mognet, SAI; Mukherjee, R; Nieto, D; Okumura, A; Otte, N; Pantaleo, FR; Paoletti, R; Pareschi, G; Di Pierro, F; Pueschel, E; Ribeiro, D; Riitano, L; Roache, E; Ross, D; Rousselle, J; Rugliancich, A; Santander, M; Shang, R; Stiaccini, L; Tajima, H; Taylor, LP; Tosti, L; Tovmassian, G; Tripodo, G; Vagelli, V; Valentino, M; Vanderbrouke, JJ; Vassiliev, VV; Watson, JJ; White, R; Williams, DA; Yu, P; Zink, A

    ASTRONOMICAL OPTICS: DESIGN, MANUFACTURE, AND TEST OF SPACE AND GROUND SYSTEMS III   Vol. 11820   2021

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    DOI: 10.1117/12.2594580

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  40. Origin of the in-orbit instrumental background of the Hard X-ray Imager onboard Hitomi Reviewed

    Hagino, K; Odaka, H; Sato, G; Sato, T; Suzuki, H; Mizuno, T; Kawaharada, M; Ohno, M; Nakazawa, K; Kobayashi, SB; Murakami, H; Miyake, K; Asai, M; Koi, T; Madejski, G; Saito, S; Wright, DH; Enoto, T; Fukazawa, Y; Hayashi, K; Kataoka, J; Katsuta, J; Kokubun, M; Laurent, P; Lebrun, F; Limousin, O; Maier, D; Makishima, K; Mori, K; Nakamori, T; Nakano, T; Noda, H; Ohta, M; Sato, R; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Tanaka, T; Terada, Y; Uchiyama, H; Uchiyama, Y; Watanabe, S; Yamaoka, K; Yatsu, Y; Yuasa, T

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 6 ( 4 )   2020.10

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    DOI: 10.1117/1.JATIS.6.4.046003

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  41. <i>Fermi</i> Large Area Telescope Fourth Source Catalog Reviewed

    Abdollahi, S; Acero, F; Ackermann, M; Ajello, M; Atwood, WB; Axelsson, M; Baldini, L; Ballet, J; Barbiellini, G; Bastieri, D; Gonzalez, JB; Bellazzini, R; Berretta, A; Bissaldi, E; Blandford, RD; Bloom, ED; Bonino, R; Bottacini, E; Brandt, TJ; Bregeon, J; Bruel, P; Buehler, R; Burnett, TH; Buson, S; Cameron, RA; Caputo, R; Caraveo, PA; Casandjian, JM; Castro, D; Cavazzuti, E; Charles, E; Chaty, S; Chen, S; Cheung, CC; Chiaro, G; Ciprini, S; Cohen-Tanugi, J; Cominsky, LR; Coronado-Blázquez, J; Costantin, D; Cuoco, A; Cutini, S; D'Ammando, F; DeKlotz, M; Luque, PD; de Palma, F; Desai, A; Digel, SW; Di Lalla, N; Di Mauro, M; Di Venere, L; Domínguez, A; Dumora, D; Dirirsa, FF; Fegan, SJ; Ferrara, EC; Franckowiak, A; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gaspanini, D; Giglietto, N; Giommi, P; Giordano, F; Giroletti, M; Glanzman, T; Green, D; Grenier, IA; Griffin, S; Grondin, MH; Grove, JE; Guiriec, S; Harding, AK; Hayashi, K; Hays, E; Hewitt, JW; Horan, D; Jóhannesson, G; Johnson, TJ; Kamae, T; Kerr, M; Kocevski, D; Kovac'evic, M; Kuss, M; Landriu, D; Larsson, S; Latronico, L; Lemoine-Goumard, M; Li, J; Liodakis, I; Longo, F; Loparco, F; Lott, B; Lovellette, MN; Lubrano, P; Madejski, GM; Maldera, S; Malyshev, D; Manfreda, A; Marchesini, J; Marcotulli, L; Martí-Devesa, G; Martin, P; Massaro, F; Mazziotta, MN; McEnery, JE; Mereu, I; Meyer, M; Michelson, PF; Mirabal, N; Mizuno, T; Monzani, ME; Morselli, A; Moskalenko, IV; Negro, M; Nuss, E; Ojha, R; Omodei, N; Orienti, M; Orlando, E; Ormes, JF; Palatiello, M; Paliya, VS; Paneque, D; Pei, Z; Peña-Herazo, H; Perkins, JS; Persic, M; Pesce-Rollms, M; Petrosian, V; Petrov, L; Piron, F; Poon, H; Porter, TA; Principe, G; Rainò, S; Rando, R; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Remy, Q; Reposeur, T; Romani, RW; Parkinson, PMS; Schinzel, FK; Serini, D; Sgrò, C; Siskind, EJ; Smith, DA; Spandre, G; Spinelli, P; Strong, AW; Suson, DJ; Tajima, H; Takahashi, MN; Tak, D; Thayer, JB; Thompson, DJ; Tibaldo, L; Torres, DF; Torresi, E; Valverde, J; Van Klaveren, B; van Zyl, P; Wood, K; Yassine, M; Zaharijas, G

    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   Vol. 247 ( 1 )   2020.3

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  42. Study of the Cosmic Rays and Interstellar Medium in Local HI Clouds Using <i>Fermi</i>-LAT Gamma-Ray Observations Reviewed

    Mizuno, T; Abdollahi, S; Fukui, Y; Hayashi, K; Koyama, T; Okumura, A; Tajima, H; Yamamoto, H

    ASTROPHYSICAL JOURNAL   Vol. 890 ( 2 )   2020.2

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    DOI: 10.3847/1538-4357/ab6a99

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  43. <i>Fermi</i> and <i>Swift</i> Observations of GRB 190114C: Tracing the Evolution of High-energy Emission from Prompt to Afterglow Reviewed

    Ajello, M; Arimoto, M; Axelsson, M; Baldini, L; Barbiellini, G; Bastieri, D; Bellazzini, R; Berretta, A; Bissaldi, E; Blandford, RD; Bonino, R; Bottacini, E; Bregeon, J; Bruel, P; Buehler, R; Burns, E; Buson, S; Cameron, RA; Caputo, R; Caraveo, PA; Cavazzuti, E; Chen, S; Chiaro, G; Ciprini, S; Cohen-Tanugi, J; Costantin, D; Cutini, S; D'Ammando, F; DeKlotz, M; Luque, PDLT; de Palma, F; Desai, A; Di Lalla, N; Di Venere, L; Dirirsa, FF; Fegan, SJ; Franckowiak, A; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gasparrini, D; Giglietto, N; Gill, R; Giordano, F; Giroletti, M; Granot, J; Green, D; Grenier, IA; Grondin, MH; Guiriec, S; Hays, E; Horan, D; Jóhannesson, G; Kocevski, D; Kovac'evic', M; Kuss, M; Larsson, S; Latronico, L; Lemoine-Goumard, M; Li, J; Liodakis, I; Longo, F; Loparco, F; Lovellette, MN; Lubrano, P; Maldera, S; Malyshev, D; Manfreda, A; Martí-Devesa, G; Mazziotta, MN; McEnery, JE; Mereu, I; Meyer, M; Michelson, PF; Mitthumsiri, W; Mizuno, T; Monzani, ME; Moretti, E; Morselli, A; Moskalenko, IV; Negro, M; Nuss, E; Omodei, N; Orienti, M; Orlando, E; Palatiello, M; Paliya, VS; Paneque, D; Pei, Z; Persic, M; Pesce-Rollins, M; Petrosian, V; Piron, F; Poon, H; Porter, TA; Principe, G; Racusin, JL; Rainò, S; Rando, R; Rani, B; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Ryde, F; Parkinson, PMS; Serini, D; Sgrò, C; Siskind, EJ; Spandre, G; Spinelli, P; Tajima, H; Takagi, K; Takahashi, MN; Tak, D; Thayer, JB; Thompson, DJ; Torres, DF; Troja, E; Valverde, J; Van Klaveren, B; Wood, K; Yassine, M; Zaharijas, G; Mailyan, B; Bhat, PN; Briggs, MS; Cleveland, W; Giles, M; Goldstein, A; Hui, M; Malacaria, C; Preece, R; Roberts, OJ; Veres, P; Wilson-Hodge, C; von Kienlin, A; Cenko, SB; O'Brien, P; Beardmore, AP; Lien, A; Osborne, JP; Tohuvavohu, A; D'Elia, V; D'Aì, A; Perri, M; Gropp, J; Klingler, N; Capalbi, M; Tagliaferri, G; Stamatikos, M; De Pasquale, M

    ASTROPHYSICAL JOURNAL   Vol. 890 ( 1 )   2020.2

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  44. Front-end electronics of the Compact High Energy Camera Reviewed

    Leach, SA; Lapington, JS; Ross, D; Thornhill, J; Duffy, C; Funk, S; Zink, A; Jankowsky, D; White, R; Zorn, J; Tibaldo, L; Varner, G; Okumura, A; Tajima, H; Watson, J

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 952   2020.2

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    DOI: 10.1016/j.nima.2018.12.061

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  45. Bright Gamma-Ray Flares Observed in GRB 131108A Reviewed

    Ajello, M; Arimoto, M; Asano, K; Axelsson, M; Baldini, L; Barbiellini, G; Bastieri, D; Bellazzini, R; Berretta, A; Bissaldi, E; Blandford, RD; Bonino, R; Bottacini, E; Bregeon, J; Bruel, P; Buehler, R; Buson, S; Cameron, RA; Caputo, R; Caraveo, PA; Cavazzuti, E; Chen, S; Chiaro, G; Ciprini, S; Costantin, D; Cutini, S; D'Ammando, F; Luque, PD; de Palma, F; Di Lalla, N; Di Venere, L; Dirirsa, FF; Fegan, SJ; Franckowiak, A; Fukazawa, Y; Fusco, P; Gargano, F; Gasparrini, D; Giglietto, N; Giordano, F; Giroletti, M; Green, D; Grenier, IA; Grondin, MH; Guiriec, S; Hays, E; Horan, D; Jóhannesson, G; Kocevski, D; Kovac'evic, M; Kuss, M; Larsson, S; Latronico, L; Li, J; Liodakis, I; Longo, F; Loparco, F; Lovellette, MN; Lubrano, P; Maldera, S; Manfreda, A; Martí-Devesa, G; Mazziotta, MN; McEnery, JE; Mereu, I; Michelson, PF; Mizuno, T; Monzani, ME; Moretti, E; Morselli, A; Moskalenko, IV; Negro, M; Nuss, E; Ohno, M; Omodei, N; Orienti, M; Orlando, E; Palatiello, M; Paliya, VS; Paneque, D; Pei, Z; Persic, M; Pesce-Rollins, M; Petrosian, V; Piron, F; Poon, H; Porter, TA; Principe, G; Racusin, JL; Rainò, S; Rando, R; Rani, B; Razzano, M; Reimer, A; Reimer, O; Serini, D; Sgrò, C; Siskind, EJ; Spandre, G; Spinelli, P; Tajima, H; Takagi, K; Tak, D; Torres, DF; Valverde, J; Wood, K; Yamazaki, R; Yassine, M; Zhu, S; Uhm, ZL; Zhang, B

    ASTROPHYSICAL JOURNAL LETTERS   Vol. 886 ( 2 )   2019.12

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    DOI: 10.3847/2041-8213/ab564f

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  46. <i>Fermi</i>-LAT γ-Ray Study of the Interstellar Medium and Cosmic Rays in the Chamaeleon Molecular Cloud Complex: A Look at the Dark Gas as Optically Thick HI Reviewed

    Hayashi, K; Mizuno, T; Fukui, Y; Okamoto, R; Yamamoto, H; Hidaka, N; Okumura, A; Tajima, H; Sano, H

    ASTROPHYSICAL JOURNAL   Vol. 884 ( 2 )   2019.10

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    DOI: 10.3847/1538-4357/ab4351

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  47. A Search for Cosmic-Ray Proton Anisotropy with the Fermi Large Area Telescope Reviewed

    Ajello M., Baldini L., Barbiellini G., Bastieri D., Bechtol K., Bellazzini R., Bissaldi E., Blandford R. D., Bonino R., Bottacini E., Brandt T. J., Bruel P., Buson S., Cameron R. A., Caputo R., Cavazzuti E., Chen S., Chiaro G., Ciprini S., Cohen-Tanugi J., Costantin D., Cuoco A., Cutini S., D'Ammando F., Luque P. de la Torre, de Palma F., Desai A., Digel S. W., Di Lalla N., Di Venere L., Dominguez A., Fegan S. J., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guiriec S., Hayashi K., Hays E., Hewitt J. W., Horan D., Johannesson G., Kuss M., Latronico L., Li J., Liodakis I, Longo F., Loparco F., Lubrano P., Maldera S., Manfreda A., Marti-Devesa G., Mazziotta M. N., Meehan M., Mereu I, Meyer M., Michelson P. F., Mirabal N., Mitthumsiri W., Mizuno T., Morselli A., Negro M., Nuss E., Omodei N., Orienti M., Orlando E., Paliya V. S., Paneque D., Persic M., Pesce-Rollins M., Piron F., Porter T. A., Principe G., Raino S., Rando R., Razzano M., Razzaque S., Reimer A., Reimer O., Serini D., Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Thayer J. B., Torres D. F., Troja E., Vandenbroucke J., Yassine M., Zimmer S.

    ASTROPHYSICAL JOURNAL   Vol. 883 ( 1 )   2019.9

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    DOI: 10.3847/1538-4357/ab3a2e

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  48. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout Reviewed

    Acharyya A., Agudo I, Anguner E. O., Alfaro R., Alfaro J., Alispach C., Aloisio R., Alves Batista R., Amans J-P, Amati L., Amato E., Ambrosi G., Antonelli L. A., Aramo C., Armstrong T., Arqueros F., Arrabito L., Asano K., Ashkar H., Balazs C., Balbo M., Balmaverde B., Barai P., Barbano A., Barkov M., Barres de Almeida U., Barrio J. A., Bastieri D., Becerra Gonzalez J., Tjus J. Becker, Bellizzi L., Benbow W., Bernardini E., Bernardos M. I, Bernloehr K., Berti A., Berton M., Bertucci B., Beshley V, Biasuzzi B., Bigongiari C., Bird R., Bissaldi E., Biteau J., Blanch O., Blazek J., Boisson C., Bonanno G., Bonardi A., Bonavolonta C., Bonnoli G., Bordas P., Bottcher M., Bregeon J., Brill A., Brown A. M., Bruegge K., Brun P., Bruno P., Bulgarelli A., Bulik T., Burton M., Burtovoi A., Busetto G., Cameron R., Canestrari R., Capalbi M., Caproni A., Capuzzo-Dolcetta R., Caraveo P., Caroff S., Carosi R., Casanova S., Cascone E., Cassol F., Catalani F., Catalano O., Cauz D., Cerruti M., Chaty S., Chen A., Chernyakova M., Chiaro G., Cieslar M., Colak S. M., Conforti V, Congiu E., Contreras J. L., Cortina J., Costa A., Costantini H., Cotter G., Cristofari P., Cumani P., Cusumano G., D'Ai A., D'Ammando F., Dangeon L., Da Vela P., Dazzi F., De Angelis A., De Caprio V, de Cassia dos Anjos R., De Frondat F., de Gouveia Dal Pino E. M., De Lotto B., De Martino D., de Naurois M., Wilhelmi E. de Ona, de Palma F., de Souza V, Del Santo M., Delgado C., della Volpe D., Di Girolamo T., Di Pierro F., Di Venere L., Diaz C., Diebold S., Djannati-Atai A., Dmytriiev A., Prester D. Dominis, Donini A., Dorner D., Doro M., Dournaux J-L, Ebr J., Ekoume T. R. N., Elsaesser D., Emery G., Falceta-Goncalves D., Fedorova E., Fegan S., Feng Q., Ferrand G., Fiandrini E., Fiasson A., Filipovic M., Fioretti V, Fiori M., Flis S., Fonseca M. V, Fontaine G., Freixas Coromina L., Fukami S., Fukui Y., Funk S., Fuessling M., Gaggero D., Galanti G., Garcia Lopez R. J., Garczarczyk M., Gascon D., Gasparetto T., Gaug M., Ghalumyan A., Gianotti F., Giavitto G., Giglietto N., Giordano F., Giroletti M., Gironnet J., Glicenstein J-F, Gnatyk R., Goldoni P., Gonzalez J. M., Gonzalez M. M., Gourgouliatos K. N., Grabarczyk T., Granot J., Green D., Greenshaw T., Grondin M-H, Gueta O., Hadasch D., Hassan T., Hayashida M., Heller M., Hervet O., Hinton J., Hiroshima N., Hnatyk B., Hofmann W., Horvath P., Hrabovsky M., Hrupec D., Humensky T. B., Huetten M., Inada T., Iocco F., Ionica M., Iori M., Iwamura Y., Jamrozy M., Janecek P., Jankowsky D., Jean P., Jouvin L., Jurysek J., Kaaret P., Kadowaki L. H. S., Karkar S., Kerszberg D., Khelifi B., Kieda D., Kimeswenger S., Kluzniak W., Knapp J., Knodlseder J., Kobayashi Y., Koch B., Kocot J., Komin N., Kong A., Kowal G., Krause M., Kubo H., Kushida J., Kushwaha P., La Parola V, La Rosa G., Lallena Arquillo M., Lang R. G., Lapington J., Le Blanc O., Lefaucheur J., Leigui de Oliveira M. A., Lemoine-Goumard M., Lenain J-P, Leto G., Lico R., Lindfors E., Lohse T., Lombardi S., Longo F., Lopez A., Lopez M., Lopez-Oramas A., Lopez-Coto R., Loporchio S., Luque-Escamilla P. L., Lyard E., Maccarone M. C., Mach E., Maggio C., Majumdar P., Malaguti G., Mallamaci M., Mandat D., Maneva G., Manganaro M., Mangano S., Marculewicz M., Mariotti M., Marti J., Martinez M., Martinez G., Martinez-Huerta H., Masuda S., Maxted N., Mazin D., Meunier J-L, Meyer M., Micanovic S., Millul R., Minaya I. A., Mitchell A., Mizuno T., Moderski R., Mohrmann L., Montaruli T., Moralejo A., Morcuende D., Morlino G., Morselli A., Moulin E., Mukherjee R., Munar P., Mundell C., Murach T., Nagai A., Nagayoshi T., Naito T., Nakamori T., Nemmen R., Niemiec J., Nieto D., Rosillo M. Nievas, Nikolajuk M., Ninci D., Nishijima K., Noda K., Nosek D., Noethe M., Nozaki S., Ohishi M., Ohtani Y., Okumura A., Ong R. A., Orienti M., Orito R., Ostrowski M., Otte N., Ou Z., Oya I, Pagliaro A., Palatiello M., Palatka M., Paoletti R., Paredes J. M., Pareschi G., Parmiggiani N., Parsons R. D., Patricelli B., Pe'er A., Pech M., Penil Del Campo P., Perez-Romero J., Perri M., Persic M., Petrucci P-O, Petruk O., Pfrang K., Piel Q., Pietropaolo E., Pohl M., Polo M., Poutanen J., Prandini E., Produit N., Prokoph H., Prouza M., Przybilski H., Puehlhofer G., Punch M., Queiroz F., Quirrenbach A., Raino S., Rando R., Razzaque S., Reimer O., Renault-Tinacci N., Renier Y., Ribeiro D., Ribo M., Rico J., Rieger F., Rizi V, Fernandez G. Rodriguez, Rodriguez-Ramirez J. C., Rodri-guez Vazquez J. J., Romano P., Romeo G., Roncadelli M., Rosado J., Rowell G., Rudak B., Rugliancich A., Rulten C., Sadeh I, Saha L., Saito T., Sakurai S., Greus F. Salesa, Sangiorgi P., Sano H., Santander M., Santangelo A., Santos-Lima R., Sanuy A., Satalecka K., Saturni F. G., Sawangwit U., Schlenstedt S., Schovanek P., Schussler F., Schwanke U., Sciacca E., Scuderi S., Sedlaczek K., Seglar-Arroyo M., Sergijenko O., Seweryn K., Shalchi A., Shellard R. C., Siejkowski H., Sillanpaa A., Sinha A., Sironi G., Sliusar V, Slowikowska A., Sol H., Specovius A., Spencer S., Spengler G., Stamerra A., Stanic S., Stawarz L., Stefanik S., Stolarczyk T., Straumann U., Suomijarvi T., Swierk P., Szepieniec T., Tagliaferri G., Tajima H., Tam T., Tavecchio F., Taylor L., Tejedor L. A., Temnikov P., Terzic T., Testa V, Tibaldo L., Todero Peixoto C. J., Tokanai F., Tomankova L., Tonev D., Torres D. F., Tosti G., Tosti L., Tothill N., Toussenel F., Tovmassian G., Travnicek P., Trichard C., Umana G., Vagelli V., Valentino M., Vallage B., Vallania P., Valore L., Vandenbroucke J., Varner G. S., Vasileiadis G., Vassiliev V., Vazquez Acosta M., Vecchi M., Vercellone S., Vergani S., Vettolani G. P., Viana A., Vigorito C. F., Vink J., Vitale V., Voelk H., Vollhardt A., Vorobiov S., Wagner S. J., Walter R., Werner F., White R., Wierzcholska A., Will M., Williams D. A., Wischnewski R., Yang L., Yoshida T., Yoshikoshi T., Zacharias M., Zampieri L., Zavrtanik M., Zavrtanik D., Zdziarski A. A., Zech A., Zechlin H., Zenin A., Zhdanov V. I, Zimmer S., Zorn J.

    ASTROPARTICLE PHYSICS   Vol. 111   page: 35 - 53   2019.9

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    DOI: 10.1016/j.astropartphys.2019.04.001

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  49. A Decade of Gamma-Ray Bursts Observed by Fermi-LAT: The Second GRB Catalog Reviewed

    Ajello M., Arimoto M., Axelsson M., Baldini L., Barbiellini G., Bastieri D., Bellazzini R., Bhat P. N., Bissaldi E., Blandford R. D., Bonino R., Bonnell J., Bottacini E., Bregeon J., Bruel P., Buehler R., Cameron R. A., Caputo R., Caraveo P. A., Cavazzuti E., Chen S., Cheung C. C., Chiaro G., Ciprini S., Costantin D., Crnogorcevic M., Cutini S., Dainotti M., D'Ammando F., Luque P. de la Torre, de Palma F., Desai A., Desiante R., Di Lalla N., Di Venere L., Dirirsa F. Fana, Fegan S. J., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Grove J. E., Guiriec S., Hays E., Hewitt J. W., Horan D., Johannesson G., Kocevski D., Kuss M., Latronico L., Li J., Longo F., Loparco F., Lovellette M. N., Lubrano P., Maldera S., Manfreda A., Marti-Devesa G., Mazziotta M. N., Mereu I, Meyer M., Michelson P. F., Mirabal N., Mitthumsiri W., Mizuno T., Monzani M. E., Moretti E., Morselli A., Moskalenko I. V, Negro M., Nuss E., Ohno M., Omodei N., Orienti M., Orlando E., Palatiello M., Paliya V. S., Paneque D., Persic M., Pesce-Rollins M., Petrosian V, Piron F., Poolakkil S., Poon H., Porter T. A., Principe G., Racusin J. L., Raino S., Rando R., Razzano M., Razzaque S., Reimer A., Reimer O., Reposeur T., Ryde F., Serini D., Sgro C., Siskind E. J., Sonbas E., Spandre G., Spinelli P., Suson D. J., Tajima H., Takahashi M., Tak D., Thayer J. B., Torres D. F., Troja E., Valverde J., Veres P., Vianello G., von Kienlin A., Wood K., Yassine M., Zhu S., Zimmer S.

    ASTROPHYSICAL JOURNAL   Vol. 878 ( 1 )   2019.6

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    DOI: 10.3847/1538-4357/ab1d4e

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  50. MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sources Reviewed

    Ahnen M. L, Ansoldi S, Antonelli L. A, Arcaro C, Baack D, Babic A, Banerjee B, Bangale P, Barres de Almeida U, Barrio J. A, Becerra Gonzalez J, Bednarek W, Bernardini E, Berse R. Ch, Berti A, Bhattacharyya W, Biland A, Blanch O, Bonnoli G, Carosi R, Carosi A, Ceribella G, Chatterjee A, Colak S. M, Colin P, Colombo E, Contreras J. L, Cortina J, Covino S, Cumani P, Da Vela P, Dazzi F, De Angelis A, De Lotto B, Delfino M, Delgado J, Di Pierro F, Dominguez A., P

    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY   Vol. 485 ( 1 ) page: 356 - 366   2019.5

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    DOI: 10.1093/mnras/stz089

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  51. Event-selection technique for the multi-layer Si-CdTe Compton camera onboard Hitomi Reviewed

    Ohno Masanori, Fukazawa Yasushi, Mizuno Tsunefumi, Takahashi Hiromitsu, Tanaka Yasuyuki, Katsuta Jun'ichiro, Kawano Takafumi, Habata Sho, Okada Chiho, Ohashi Norie, Teramae Takuto, Tanaka Koji, Takahashi Tadayuki, Kokubun Motohide, Watanabe Shin, Sato Goro, Sato Rie, Ohta Masayuki, Uchida Yusuke, Tamaru Ryota, Yoneda Hiroki, Nakazawa Kazuhiro, Murakami Hiroaki, Tajima Hiroyasu, Yamaoka Kazutaka, Kinoshita Masaomi, Hayashi Katsuhiro, Kitaguchi Takao, Odaka Hirokazu

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 924   page: 327 - 331   2019.4

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    DOI: 10.1016/j.nima.2018.09.114

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  52. Introduction to CTA Science Reviewed

    Acharya B. S., Agudo I., Al Samarai I., Alfaro R., Alfaro J., Alispach C., Batista R. Alves, Amans J. -P., Amato E., Ambrosi G., Antolini E., Antonelli L. A., Aramo C., Araya M., Armstrong T., Arqueros F., Arrabito L., Asano K., Ashley M., Backes M., Balazs C., Balbo M., Ballester O., Ballet J., Bamba A., Barkov M., Barres de Almeida U., Barrio J. A., Bastieri D., Becherini Y., Belfiore A., Benbow W., Berge D., Bernardini E., Bernardini M. G., Bernardos M., Bernloehr K., Bertucci B., Biasuzzi B., Bigongiari C., Biland A., Bissaldi E., Biteau J., Blanch O., Blazek J., Boisson C., Bolmont J., Bonanno G., Bonardi A., Bonavolonta C., Bonnoli G., Bosnjak Z., Bottcher M., Braiding C., Bregeon J., Brill A., Brown A. M., Brun P., Brunetti G., Buanes T., Buckley J., Bugaev V., Buehler R., Bulgarelli A., Bulik T., Burton M., Burtovoi A., Busetto G., Canestrari R., Capalbi M., Capitanio F., Caproni A., Caraveo P., Cardenas V., Carlile C., Carosi R., Carquin E., Carr J., Casanova S., Cascone E., Catalani F., Catalano O., Cauz D., Cerruti M., Chadwick P., Chaty S., Chaves R. C. G., Chen A., Chen X., Chernyakova M., Chikawa M., Christov A., Chudoba J., Cieslar M., Coco V., Colafrancesco S., Colin P., Conforti V., Connaughton V., Conrad J., Contreras J. L., Cortina J., Costa A., Costantini H., Cotter G., Covino S., Crocker R., Cuadra J., Cuevas O., Cumani P., D'Ai A., D'Ammando F., D'Avanzo P., D'Urso D., Daniel M., Davids I., Dawson B., Dazzi F., De Angelis A., de Cassia dos Anjos R., De Cesare G., De Franco A., De Gouveia Dal Pino E. M., de la Calle I., Lopez R. de los Reyes, De Lotto B., De Luca A., De Lucia M., de Naurois M., de Ona Wilhelmi E., De Palma F., De Persio F., de Souza V., Deil C., Del Santo M., Delgado C., della Volpe D., Di Girolamo T., Di Pierro F., Di Venere L., Diaz C., Dib C., Diebold S., Djannati-Atai A., Dominguez A., Prester D. Dominis, Dorner D., Doro M., Drass H., Dravins D., Dubus G., Dwarkadas V. V., Ebr J., Eckner C., Egberts K., Einecke S., Ekoume T. R. N., Elsaesser D., Ernenwein J. -P., Espinoza C., Evoli C., Fairbairn M., Falceta-Goncalves D., Falcone A., Farnier C., Fasola G., Fedorova E., Fegan S., Fernandez-Alonso M., Fernandez-Barral A., Ferrand G., Fesquet M., Filipovic M., Fioretti V., Fontaine G., Fornasa M., Fortson L., Freixas Coromina L., Fruck C., Fujita Y., Fukazawa Y., Funk S., Fuessling M., Gabici S., Gadola A., Gallant Y., Garcia B., Garcia Lopez R., Garczarczyk M., Gaskins J., Gasparetto T., Gaug M., Gerard L., Giavitto G., Giglietto N., Giommi P., Giordano F., Giro E., Giroletti M., Giuliani A., Glicenstein J. -F., Gnatyk R., Godinovic N., Goldoni P., Gomez-Vargas G., Gonzalez M. M., Gonzalez J. M., Gotz D., Graham J., Grandi P., Granot J., Green A. J., Greenshaw T., Griffiths S., Gunji S., Hadasch D., Hara S., Hardcastle M. J., Hassan T., Hayashi K., Hayashida M., Heller M., Helo J. C., Hermann G., Hinton J., Hnatyk B., Hofmann W., Holder J., Horan D., Horandel J., Horns D., Horvath P., Hovatta T., Hrabovsky M., Hrupec D., Humensky T. B., Huetten M., Iarlori M., Inada T., Inome Y., Inoue S., Inoue T., Inoue Y., Iocco F., Ioka K., Iori M., Ishio K., Iwamura Y., Jamrozy M., Janecek P., Jankowsky D., Jean P., Jung-Richardt I., Jurysek J., Kaaret P., Karkar S., Katagiri H., Katz U., Kawanaka N., Kazanas D., Khelifi B., Kieda D. B., Kimeswenger S., Kimura S., Kisaka S., Knapp J., Knodlseder J., Koch B., Kohri K., Komin N., Kosack K., Kraus M., Krause M., Krauss F., Kubo H., Mezek G. Kukec, Kuroda H., Kushida J., La Palombara N., Lamanna G., Lang R. G., Lapington J., Le Blanc O., Leach S., Lees J. -P., Lefaucheur J., Leigui de Oliveira M. A., Lenain J. -P., Lico R., Limon M., Lindfors E., Lohse T., Lombardi S., Longo F., Lopez M., Lopez-Coto R., Lu C. -C., Lucarelli F., Luque-Escamilla P. L., Lyard E., Maccarone M. C., Maier G., Majumdar P., Malaguti G., Mandat D., Maneva G., Manganaro M., Mangano S., Marcowith A., Marin J., Markoff S., Marti J., Martin P., Martinez M., Martinez G., Masetti N., Masuda S., Maurin G., Maxted N., Mazin D., Medina C., Melandri A., Mereghetti S., Meyer M., Minaya I. A., Mirabal N., Mirzoyan R., Mitchell A., Mizuno T., Moderski R., Mohammed M., Mohrmann L., Montaruli T., Moralejo A., Morcuende-Parrilla D., Mori K., Morlino G., Morris P., Morselli A., Moulin E., Mukherjee R., Mundell C., Murach T., Muraishi H., Murase K., Nagai A., Nagataki S., Nagayoshi T., Naito T., Nakamori T., Nakamura Y., Niemiec J., Nieto D., Nikolajuk M., Nishijima K., Noda K., Nosek D., Novosyadlyj B., Nozaki S., O'Brien P., Oakes L., Ohira Y., Ohishi M., Ohm S., Okazaki N., Okumura A., Ong R. A., Orienti M., Orito R., Osborne J. P., Ostrowski M., Otte N., Oya I., Padovani M., Paizis A., Palatiello M., Palatka M., Paoletti R., Paredes J. M., Pareschi G., Parsons R. D., Pe'er A., Pech M., Pedaletti G., Perri M., Persic M., Petrashyk A., Petrucci P., Petruk O., Peyaud B., Pfeifer M., Piano G., Pisarski A., Pita S., Pohl M., Polo M., Pozo D., Prandini E., Prast J., Principe G., Prokhorov D., Prokoph H., Prouza M., Puehlhofer G., Punch M., Puerckhauer S., Queiroz F., Quirrenbach A., Raino S., Razzaque S., Reimer O., Reimer A., Reisenegger A., Renaud M., Rezaeian A. H., Rhode W., Ribeiro D., Ribo M., Richtler T., Rico J., Rieger F., Riquelme M., Rivoire S., Rizi V., Rodriguez J., Fernandez G. Rodriguez, Rodriguez Vazquez J. J., Rojas G., Romano P., Romeo G., Rosado J., Rovero A. C., Rowell G., Rudak B., Rugliancich A., Rulten C., Sadeh I., Safi-Harb S., Saito T., Sakaki N., Sakurai S., Salina G., Sanchez-Conde M., Sandaker H., Sandoval A., Sangiorgi P., Sanguillon M., Sano H., Santander M., Sarkar S., Satalecka K., Saturni F. G., Schioppa E. J., Schlenstedt S., Schneider M., Schoorlemmer H., Schovanek P., Schulz A., Schussler F., Schwanke U., Sciacca E., Scuderi S., Seitenzahl I., Semikoz D., Sergijenko O., Servillat M., Shalchi A., Shellard R. C., Sidoli L., Siejkowski H., Sillanpaa A., Sironi G., Sitarek J., Sliusar V., Slowikowska A., Sol H., Stamerra A., Stanic S., Starling R., Stawarz L., Stefanik S., Stephan M., Stolarczyk T., Stratta G., Straumann U., Suomijarvi T., Supanitsky A. D., Tagliaferri G., Tajima H., Tavani M., Tavecchio F., Tavernet J. -P., Tayabaly K., Tejedor L. A., Temnikov P., Terada Y., Terrier R., Terzic T., Teshima M., Testa V., Thoudam S., Tian W., Tibaldo L., Tluczykont M., Todero Peixoto C. J., Tokanai F., Tomastik J., Tonev D., Tornikoski M., Torres D. F., Torresi E., Tosti G., Tothill N., Tovmassian G., Travnicek P., Trichard C., Trifoglio M., Pujadas I. Troyano, Tsujimoto S., Umana G., Vagelli V., Vagnetti F., Valentino M., Vallania P., Valore L., van Eldik C., Vandenbroucke J., Varner G. S., Vasileiadis G., Vassiliev V., Vazquez Acosta M., Vecchi M., Vega A., Vercellone S., Veres P., Vergani S., Verzi V., Vettolani G. P., Viana A., Vigorito C., Villanueva J., Voelk H., Vollhardt A., Vorobiov S., Vrastil M., Vuillaume T., Wagner S. J., Wagner R., Walter R., Ward J. E., Warren D., Watson J. J., Werner F., White M., White R., Wierzcholska A., Wilcox P., Will M., Williams D. A., Wischnewski R., Wood M., Yamamoto T., Yamazaki R., Yanagita S., Yang L., Yoshida T., Yoshiike S., Yoshikoshi T., Zacharias M., Zaharijas G., Zampieri L., Zandanel F., Zanin R., Zavrtanik M., Zavrtanik D., Zdziarski A. A., Zech A., Zechlin H., Zhdanov V. I., Ziegler A., Zorn J.

    SCIENCE WITH THE CHERENKOV TELESCOPE ARRAY     page: 1-+   2019

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  53. SENSE - Ultimate Low Light-Level Sensor Development Reviewed

    Bonanna G., Haungs A., Henjes-Kunst K., Huber T., Link K., Nagai A., Mirzoyan R., Montaruli T., Romeo G., Strom D., Tajima H.

    26TH EXTENDED EUROPEAN COSMIC RAY SYMPOSIUM   Vol. 1181   2019

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    DOI: 10.1088/1742-6596/1181/1/012082

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  54. Introduction to CTA Science Reviewed

    Acharya B. S, Agudo I, Al Samarai I, Alfaro R, Alfaro J, Alispach C, Batista R. Alves, Amans J. -P, Amato E, Ambrosi G, Antolini E, Antonelli L. A, Aramo C, Araya M, Armstrong T, Arqueros F, Arrabito L, Asano K, Ashley M, Backes M, Balazs C, Balbo M, Ballester O, Ballet J, Bamba A, Barkov M, Barres de Almeida U, Barrio J. A, Bastieri D, Becherini Y, Belfiore A, Benbow W, Berge D, Bernardini E, Bernardini M. G, Bernardos M, Bernloehr K, Bertucci B, Biasuzzi B

    SCIENCE WITH THE CHERENKOV TELESCOPE ARRAY     page: 1-+   2019

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  55. Evaluation of silicon photomultipliers for dual-mirror Small-Sized Telescopes of Cherenkov Telescope Array Reviewed International coauthorship

    Asano A., Berge D., Bonanno G., Bryan M., Gebhardt B., Grillo A., Hidaka N., Kachru P., Lapington J., Leach S., Nakamura Y., Okumura A., Romeo G., Ross D., Stephan M., Tajima H., Timpanaro M. C., White R., Yamane N., Zink A.

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 912   page: 177 - 181   2018.12

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    DOI: 10.1016/j.nima.2017.11.017

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  56. SENSE: A comparison of photon detection efficiency and optical crosstalk of various SiPM devices Reviewed

    Nagai A., Alispach C., Berghoefer T., Bonanno G., Coco V., della Volpe D., Haungs A., Heller M., Henjes-Kunst K., Mirzoyan R., Montaruli T., Romeo G., Renier Y., Schultz-Coulon H. C., Shen W., Strom D., Tajima H., Troyano-Pujadas I.

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 912   page: 182 - 185   2018.12

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    DOI: 10.1016/j.nima.2017.11.018

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  57. Unresolved Gamma-Ray Sky through its Angular Power Spectrum Reviewed

    Ackermann M., Ajello M., Baldini L., Ballet J., Barbiellini G., Bastieri D., Bellazzini R., Bissaldi E., Blandford R. D., Bonino R., Bottacini E., Bregeon J., Bruel P., Buehler R., Burns E., Buson S., Cameron R. A., Caputo R., Caraveo P. A., Cavazzuti E., Chen S., Chiaro G., Ciprini S., Costantin D., Cuoco A., Cutini S., D'Ammando F., Luque P. de la Torre, de Palma F., Desai A., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Dirirsa F. Fana, Favuzzi C., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guillemot L., Guiriec S., Horan D., Johannesson G., Kuss M., Larsson S., Latronico L., Li J., Liodakis I., Longo F., Loparco F., Lubrano P., Magill J. D., Maldera S., Malyshev D., Manfreda A., Mazziotta M. N., Mereu I., Michelson P. F., Mitthumsiri W., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Orienti M., Orlando E., Palatiello M., Paliya V. S., Paneque D., Persic M., Pesce-Rollins M., Petrosian V., Piron F., Porter T. A., Principe G., Raino S., Rando R., Razzano M., Razzaque S., Reimer A., Reimer O., Serini D., Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Takahashi M., Thayer J. B., Tibaldo L., Torres D. F., Troja E., Venters T. M., Vianello G., Wood K., Yassine M., Zaharijas G., Ammazzalorso S., Fornengo N., Regis M.

    PHYSICAL REVIEW LETTERS   Vol. 121 ( 24 )   2018.12

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    DOI: 10.1103/PhysRevLett.121.241101

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  58. Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector Reviewed International coauthorship

    Aharonian Felix, Akamatsu Hiroki, Akimoto Fumie, Allen Steven W., Angelini Lorella, Audard Marc, Awaki Hisamitsu, Axelsson Magnus, Bamba Aya, Bautz Marshall W., Blandford Roger, Brenneman Laura W., Brown Gregory V., Bulbul Esra, Cackett Edward M., Chernyakova Maria, Chiao Meng P., Coppi Paolo S., Costantini Elisa, de Plaa Jelle, de Vries Cor P., den Herder Jan-Willem, Done Chris, Dotani Tadayasu, Ebisawa Ken, Eckart Megan E., Enoto Teruaki, Ezoe Yuichiro, Fabian Andrew C., Ferrigno Carlo, Foster Adam R., Fujimoto Ryuichi, Fukazawa Yasushi, Furuzawa Akihiro, Galeazzi Massimiliano, Gallo Luigi C., Gandhi Poshak, Giustini Margherita, Goldwurm Andrea, Gu Liyi, Guainazzi Matteo, Haba Yoshito, Hagino Kouichi, Hamaguchi Kenji, Harrus Ilana M., Hatsukade Isamu, Hayashi Katsuhiro, Hayashi Takayuki, Hayashida Kiyoshi, Hiraga Junko S., Hornschemeier Ann, Hoshino Akio, Hughes John P., Ichinohe Yuto, Iizuka Ryo, Inoue Hajime, Inoue Yoshiyuki, Ishida Manabu, Ishikawa Kumi, Ishisaki Yoshitaka, Iwai Masachika, Kaastra Jelle, Kallman Tim, Kamae Tsuneyoshi, Kataoka Jun, Katsuda Satoru, Kawai Nobuyuki, Kelley Richard L., Kilbourne Caroline A., Kitaguchi Takao, Kitamoto Shunji, Kitayama Tetsu, Kohmura Takayoshi, Kokubun Motohide, Koyama Katsuji, Koyama Shu, Kretschmar Peter, Krimm Hans A., Kubota Aya, Kunieda Hideyo, Laurent Philippe, Lee Shiu-Hang, Leutenegger Maurice A., Limousin Olivier, Loewenstein Michael, Long Knox S., Lumb David, Madejski Greg, Maeda Yoshitomo, Maier Daniel, Makishima Kazuo, Markevitch Maxim, Matsumoto Hironori, Matsushita Kyoko, McCammon Dan, McNamara Brian R., Mehdipour Missagh, Miller Eric D., Miller Jon M., Mineshige Shin, Mitsuda Kazuhisa, Mitsuishi Ikuyuki, Miyazawa Takuya, Mizuno Tsunefumi, Mori Hideyuki, Mori Koji, Mukai Koji, Murakami Hiroshi, Mushotzky Richard F., Nakagawa Takao, Nakajima Hiroshi, Nakamori Takeshi, Nakashima Shinya, Nakazawa Kazuhiro, Nobukawa Kumiko K., Nobukawa Masayoshi, Noda Hirofumi, Odaka Hirokazu, Ohashi Takaya, Ohno Masanori, Okajima Takashi, Ota Naomi, Ozaki Masanobu, Paerels Frits, Paltani Stephane, Petre Robert, Pinto Ciro, Porter Frederick S., Pottschmidt Katja, Reynolds Christopher S., Safi-Harb Samar, Saito Shinya, Sakai Kazuhiro, Sasaki Toru, Sato Goro, Sato Kosuke, Sato Rie, Sawada Makoto, Schartel Norbert, Serlemtsos Peter J., Seta Hiromi, Shidatsu Megumi, Simionescu Aurora, Smith Randall K., Soong Yang, Stawarz Lukasz, Sugawara Yasuharu, Sugita Satoshi, Szymkowiak Andrew, Tajima Hiroyasu, Takahashi Hiromitsu, Takahashi Tadayuki, Takeda Shin'ichiro, Takei Yoh, Tamagawa Toru, Tamura Takayuki, Tanaka Takaaki, Tanaka Yasuo, Tanaka Yasuyuki T., Tashiro Makoto S., Tawara Yuzuru, Terada Yukikatsu, Terashima Yuichi, Tombesi Francesco, Tomida Hiroshi, Tsuboi Yohko, Tsujimoto Masahiro, Tsunemi Hiroshi, Tsuru Takeshi Go, Uchida Hiroyuki, Uchiyama Hideki, Uchiyama Yasunobu, Ueda Shutaro, Ueda Yoshihiro, Uno Shin'ichiro, Urry C. Megan, Ursino Eugenio, Watanabe Shin, Werner Norbert, Wilkins Dan R., Williams Brian J., Yamada Shinya, Yamaguchi Hiroya, Yamaoka Kazutaka, Yamasaki Noriko Y., Yamauchi Makoto, Yamauchi Shigeo, Yaqoob Tahir, Yatsu Yoichi, Yonetoku Daisuke, Zhuravleva Irina, Zoghbi Abderahmen, Uchida Yuusuke

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 6 )   2018.12

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    DOI: 10.1093/pasj/psy118

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  59. A gamma-ray determination of the Universe's star formation history Reviewed

    Abdollahi S., Ackermann M., Ajello M., Atwood W. B., Baldini L., Ballet J., Barbiellini G., Bastieri D., Gonzalez J. Becerra, Bellazzini R., Bissaldi E., Blandford R. D., Bloom E. D., Bonino R., Bottacini E., Buson S., Bregeon J., Bruel P., Buehler R., Cameron R. A., Caputo R., Caraveo P. A., Cavazzuti E., Charles E., Chen S., Cheung C. C., Chiaro G., Ciprini S., Cohen-Tanugi J., Cominsky L. R., Conrad J., Costantin D., Cutini S., D'Ammando F., de Palma F., Desai A., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Dominguez A., Favuzzi C., Fegan S. J., Finke J., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Romero G. Gallardo, Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guillemot L., Guiriec S., Hartmann D. H., Hays E., Helgason K., Horan D., Johannesson G., Kocevski D., Kuss M., Larsson S., Latronico L., Li J., Longo F., Loparco F., Lott B., Lovellette M. N., Lubrano P., Madejski G. M., Magill J. D., Maldera S., Manfreda A., Marcotulli L., Mazziotta M. N., McEnery J. E., Meyer M., Michelson P. F., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Ojha R., Omodei N., Orienti M., Orlando E., Ormes J. F., Palatiello M., Paliya V. S., Paneque D., Perkins J. S., Persic M., Pesce-Rollins M., Petrosian V., Piron F., Porter T. A., Primack J. R., Principe G., Raino S., Rando R., Razzano M., Razzaque S., Reimer A., Reimer O., Parkinson P. M. Saz, Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Takahashi M., Thayer J. B., Tibaldo L., Torres D. F., Torresi E., Tosti G., Tramacere A., Troja E., Valverde J., Vianello G., Vogel M., Wood K., Zaharijas G.

    SCIENCE   Vol. 362 ( 6418 ) page: 1031 - +   2018.11

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    DOI: 10.1126/science.aat8123

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  60. VERITAS and Fermi-LAT Observations of TeV Gamma-Ray Sources Discovered by HAWC in the 2HWC Catalog Reviewed

    Abeysekara A. U., Archer A., Benbow W., Bird R., Brose R., Buchovecky M., Buckley J. H., Bugaev V., Chromey A. J., Connolly M. P., Cui W., Daniel M. K., Falcone A., Feng Q., Finley J. P., Fortson L., Furniss A., Huetten M., Hanna D., Hervet O., Holder J., Hughes G., Humensky T. B., Johnson C. A., Kaaret P., Kar P., Kertzman M., Kieda D., Krause M., Krennrich F., Kumar S., Lang M. J., Lin T. T. Y., McArthur S., Moriarty P., Mukherjee R., O'Brien S., Ong R. A., Otte A. N., Park N., Petrashyk A., Pohl M., Pueschel E., Quinn J., Ragan K., Reynolds P. T., Richards G. T., Roache E., Rulten C., Sadeh I., Santander M., Sembroski G. H., Shahinyan K., Sushch I., Tyler J., Wakely S. P., Weinstein A., Wells R. M., Wilcox P., Wilhelm A., Williams D. A., Williamson T. J., Zitzer B., Abdollahi S., Ajello M., Baldini L., Barbiellini G., Bastieri D., Bellazzini R., Berenji B., Bissaldi E., Blandford R. D., Bonino R., Bottacini E., Brandt T. J., Bruel P., Buehler R., Cameron R. A., Caputo R., Caraveo P. A., Castro D., Cavazzuti E., Charles E., Chiaro G., Ciprini S., Cohen-Tanugi J., Costantin D., Cutini S., D'Ammando F., de Palma F., Di Lalla N., Di Mauro M., Di Venere L., Dominguez A., Favuzzi C., Fegan S. J., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guillemot L., Guiriec S., Hays E., Hewitt J. W., Horan D., Johannesson G., Kensei S., Kuss M., Larsson S., Latronico L., Lemoine-Goumard M., Li J., Longo F., Loparco F., Lovellette M. N., Lubrano P., Magill J. D., Maldera S., Mazziotta M. N., McEnery J. E., Michelson P. F., Mitthumsiri W., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Ojha R., Omodei N., Orienti M., Orlando E., Palatiello M., Paliya V. S., Paneque D., Perkins J. S., Persic M., Pesce-Rollins M., Petrosian V., Piron F., Porter T. A., Principe G., Raino S., Rando R., Rani B., Razzano M., Razzaque S., Reimer A., Reimer O., Reposeur T., Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Thayer J. B., Thompson D. J., Torres D. F., Tosti G., Troja E., Valverde J., Vianello G., Vogel M., Wood K., Yassine M., Alfaro R., Alvarez C., Alvarez J. D., Arceo R., Arteaga-Velazquez J. C., Rojas D. Avila, Ayala Solares H. A., Becerril A., Belmont-Moreno E., BenZvi S. Y., Bernal A., Braun J., Brisbois C., Caballero-Mora K. S., Capistran T., Carraminana A., Casanova S., Castillo M., Cotti U., Cotzomi J., Coutino de Leon S., De Leon C., De la Fuente E., Dichiara S., Dingus B. L., DuVernois M. A., Diaz-Velez J. C., Engel K., Enriquez-Rivera O., Fiorino D. W., Fleischhack H., Fraija N., Garcia-Gonzalez J. A., Garfias F., Gonzalez Munoz A., Gonzalez M. M., Goodman J. A., Hampel-Arias Z., Harding J. P., Hernandez S., Hernandez-Almada A., Hona B., Hueyotl-Zahuantitla F., Hui C. M., Huntemeyer P., Iriarte A., Jardin-Blicq A., Joshi V., Kaufmann S., Lara A., Lauer R. J., Lee W. H., Lennarz D., Leon Vargas H., Linnemann J. T., Longinotti A. L., Luis-Raya G., Luna-Garcia R., Lopez-Coto R., Malone K., Marinelli S. S., Martinez O., Martinez-Castellanos I., Martinez-Castro J., Martinez-Huerta H., Matthews J. A., Miranda-Romagnoli P., Moreno E., Mostafa M., Nayerhoda A., Nellen L., Newbold M., Nisa M. U., Noriega-Papaqui R., Pelayo R., Pretz J., Perez-Perez E. G., Ren Z., Rho C. D., Riviere C., Rosa-Gonzalez D., Rosenberg M., Ruiz-Velasco E., Salazar H., Greus F. Salesa, Sandoval A., Schneider M., Arroyo M. Seglar, Sinnis G., Smith A. J., Springer R. W., Surajbali P., Taboada I., Tibolla O., Tollefson K., Torres I., Ukwatta T. N., Villasenor L., Weisgarber T., Westerhoff S., Wisher I. G., Wood J., Yapici T., Yodh G., Zepeda A., Zhou H.

    ASTROPHYSICAL JOURNAL   Vol. 866 ( 1 )   2018.10

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    DOI: 10.3847/1538-4357/aade4e

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  61. Characterisation and testing of CHEC-M-A camera prototype for the small-sized telescopes of the Cherenkov telescope array Reviewed

    Zorn J., White R., Watson J. J., Armstrong T. P., Balzer A., Barcelo M., Berge D., Bose R., Brown A. M., Bryan M., Chadwick P. M., Clark P., Costantini H., Cotter G., Dangeon L., Daniel M., De Franco A., Deiml P., Fasola G., Funk S., Gebyehu M., Gironnet J., Graham J. A., Greenshaw T., Hinton J. A., Kraus M., Lapington J. S., Laporte P., Leach S. A., Le Blanc O., Malouf A., Molyneux P., Moore P., Prokoph H., Okumura A., Ross D., Rowell G., Sapozhnikov L., Schoorlemmer H., Sol H., Stephan M., Tajima H., Tibaldo L., Varner G., Zink A.

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 904   page: 44 - 63   2018.10

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    DOI: 10.1016/j.nima.2018.06.078

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  62. Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry Reviewed

    Chauvin M., Floren H-G, Friis M., Jackson M., Kamae T., Kataoka J., Kawano T., Kiss M., Mikhalev V, Mizuno T., Ohashi N., Stana T., Tajima H., Takahashi H., Uchida N., Pearce M.

    NATURE ASTRONOMY   Vol. 2 ( 8 ) page: 652 - 655   2018.8

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    DOI: 10.1038/s41550-018-0489-x

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  63. The Search for Spatial Extension in High-latitude Sources Detected by the Fermi Large Area Telescope Reviewed

    Ackermann M., Ajello M., Baldini L., Ballet J., Barbiellini G., Bastieri D., Bellazzini R., Bissaldi E., Blandford R. D., Bloom E. D., Bonino R., Bottacini E., Brandt T. J., Bregeon J., Bruel P., Buehler R., Cameron R. A., Caputo R., Caraveo P. A., Castro D., Cavazzuti E., Charles E., Cheung C. C., Chiaro G., Ciprini S., Cohen-Tanugi J., Costantin D., Cutini S., D'Ammando F., de Palma F., Desai A., Di Lalla N., Di Mauro M., Di Venere L., Favuzzi C., Finke J., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guillemot L., Guiriec S., Hays E., Hewitt J. W., Horan D., Johannesson G., Kensei S., Kuss M., Larsson S., Latronico L., Lemoine-Goumard M., Li J., Longo F., Loparco F., Lovellette M. N., Lubrano P., Magill J. D., Maldera S., Manfreda A., Mazziotta M. N., McEnery J. E., Meyer M., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Omodei N., Orienti M., Orlando E., Ormes J. F., Palatiello M., Paliya V. S., Paneque D., Perkins J. S., Persic M., Pesce-Rollins M., Piron F., Porter T. A., Principe G., Raino S., Rando R., Rani B., Razzaque S., Reimer A., Reimer O., Reposeur T., Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Thayer J. B., Tibaldo L., Torres D. F., Tosti G., Valverde J., Venters T. M., Vogel M., Wood K., Wood M., Zaharijas G., Biteau J.

    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   Vol. 237 ( 2 )   2018.8

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    DOI: 10.3847/1538-4365/aacdf7

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  64. Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A Reviewed

    Aartsen M. G., Ackermann M., Adams J., Aguilar J. A., Ahlers M., Ahrens M., Al Samarai I., Altmann D., Andeen K., Anderson T., Ansseau I., Anton G., Arguelles C., Auffenberg J., Axani S., Bagherpour H., Bai X., Barron J. P., Barwick S. W., Baum V., Bay R., Beatty J. J., Tjus J. Becker, Becker K. -H., BenZvi S., Berley D., Bernardini E., Besson D. Z., Binder G., Bindig D., Blaufuss E., Blot S., Bohm C., Borner M., Bos F., Boser S., Botner O., Bourbeau E., Bourbeau J., Bradascio F., Braun J., Brenzke M., Bretz H. -P., Bron S., Brostean-Kaiser J., Burgman A., Busse R. S., Carver T., Cheung E., Chirkin D., Christov A., Clark K., Classen L., Coenders S., Collin G. H., Conrad J. M., Coppin P., Correa P., Cowen D. F., Cross R., Dave P., Day M., de Andre J. P. A. M., De Clercq C., DeLaunay J. J., Dembinski H., De Ridder S., Desiati P., de Vries K. D., de Wasseige G., de With M., DeYoung T., Diaz-Velez J. C., di Lorenzo V., Dujmovic H., Dumm J. P., Dunkman M., Dvorak E., Eberhardt B., Ehrhardt T., Eichmann B., Eller P., Evenson P. A., Fahey S., Fazely A. R., Felde J., Filimonov K., Finley C., Flis S., Franckowiak A., Friedman E., Fritz A., Gaisser T. K., Gallagher J., Gerhardt L., Ghorbani K., Glauch T., Glusenkamp T., Goldschmidt A., Gonzalez J. G., Grant D., Griffith Z., Haack C., Hallgren A., Halzen F., Hanson K., Hebecker D., Heereman D., Helbing K., Hellauer R., Hickford S., Hignight J., Hill G. C., Hoffman K. D., Hoffmann R., Hoinka T., Hokanson-Fasig B., Hoshina K., Huang F., Huber M., Hultqvist K., Hunnefeld M., Hussain R., In S., Iovine N., Ishihara A., Jacobi E., Japaridze G. S., Jeong M., Jero K., Jones B. J. P., Kalaczynski P., Kang W., Kappes A., Kappesser D., Karg T., Karle A., Katz U., Kauer M., Keivani A., Kelley J. L., Kheirandish A., Kim J., Kim M., Kintscher T., Kiryluk J., Kittler T., Klein S. R., Koirala R., Kolanoski H., Kopke L., Kopper C., Kopper S., Koschinsky J. P., Koskinen D. J., Kowalski M., Krings K., Kroll M., Kruckl G., Kunwar S., Kurahashi N., Kuwabara T., Kyriacou A., Labare M., Lanfranchi J. L., Larson M. J., Lauber F., Leonard K., Lesiak-Bzdak M., Leuermann M., Liu Q. R., Mariscal C. J. Lozano, Lu L., Lunemann J., Luszczak W., Madsen J., Maggi G., Mahn K. B. M., Mancina S., Maruyama R., Mase K., Maunu R., Meagher K., Medici M., Meier M., Menne T., Merino G., Meures T., Miarecki S., Micallef J., Momente G., Montaruli T., Moore R. W., Morse R., Moulai M., Nahnhauer R., Nakarmi P., Naumann U., Neer G., Niederhausen H., Nowicki S. C., Nygren D. R., Pollmann A. Obertacke, Olivas A., O'Murchadha A., O'Sullivan E., Palczewski T., Pandya H., Pankova D. V., Peiffer P., Pepper J. A., de los Heros C. Perez, Pieloth D., Pinat E., Plum M., Price P. B., Przybylski G. T., Raab C., Radel L., Rameez M., Rauch L., Rawlins K., Rea I. C., Reimann R., Relethford B., Relich M., Resconi E., Rhode W., Richman M., Robertson S., Rongen M., Rott C., Ruhe T., Ryckbosch D., Rysewyk D., Safa I., Salzer T., Herrera S. E. Sanchez, Sandrock A., Sandroos J., Santander M., Sarkar S., Sarkar S., Satalecka K., Schlunder P., Schmidt T., Schneider A., Schoenen S., Schoneberg S., Schumacher L., Sclafani S., Seckel D., Seunarine S., Soedingrekso J., Soldin D., Song M., Spiczak G. M., Spiering C., Stachurska J., Stamatikos M., Stanev T., Stasik A., Stein R., Stettner J., Steuer A., Stezelberger T., Stokstad R. G., Stossl A., Strotjohann N. L., Stuttard T., Sullivan G. W., Sutherland M., Taboada I., Tatar J., Tenholt F., Ter-Antonyan S., Terliuk A., Tilav S., Toale P. A., Tobin M. N., Toennis C., Toscano S., Tosi D., Tselengidou M., Tung C. F., Turcati A., Turley C. F., Ty B., Unger E., Usner M., Vandenbroucke J., Van Driessche W., van Eijk D., van Eijndhoven N., Vanheule S., van Santen J., Vogel E., Vraeghe M., Walck C., Wallace A., Mallraff M., Wandler F. D., Wandkowsky N., Waza A., Weaver C., Weiss M. J., Wendt C., Werthebach J., Westerhoff S., Whelan B. J., Whitehorn N., Whelan B. J., Whitehorn N., Wiebe K., Wiebusch C. H., Wille L., Williams D. R., Wills L., Wolf M., Wood J., Wood T. R., Woschnagg K., Xu D. L., Xu X. W., Xu Y., Yanez J. P., Yodh G., Yoshida S., Yuan T., Abdollahi S., Ajello M., Angioni R., Baldini L., Ballet J., Barbiellini G., Bastieri D., Bechtol K., Bellazzini R., Berenji B., Bissaldi E., Blandford R. D., Bonino R., Bottacini E., Bregeon J., Bruel P., Buehler R., Burnett T. H., Burns E., Buson S., Cameron R. A., Caputo R., Caraveo P. A., Cavazzuti E., Charles E., Chen S., Cheung C. C., Chiang J., Chiaro G., Ciprini S., Cohen-Tanugi J., Conrad J., Costantin D., Cutini S., D'Ammando F., de Palma F., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Dominguez A., Favuzzi C., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giomi M., Giommi P., Giordano F., Giroletti M., Glanzman T., Green D., Grenier I. A., Grondin M. -H., Guiriec S., Harding A. K., Hayashida M., Hays E., Hewitt J. W., Horan D., Johannesson G., Kadler M., Kensei S., Kocevski D., Krauss F., Kreter M., Kuss M., La Mura G., Larsson S., Latronico L., Lemoine-Goumard M., Li J., Longo F., Loparco F., Lovellette M. N., Lubrano P., Magill J. D., Maldera S., Malyshev D., Manfreda A., Mazziotta M. N., McEnery J. E., Meyer M., Michelson P. F., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Ojha R., Omodei N., Orienti M., Orlando E., Palatiello M., Paliya V. S., Perkins J. S., Persic M., Pesce-Rollins M., Piron F., Porter T. A., Principe G., Raino S., Rando R., Rani B., Razzano M., Razzaque S., Reimer A., Reimer O., Renault-Tinacci N., Ritz S., Rochester L. S., Parkinson P. M. Saz, Sgro C., Siskind E. J., Spandre G., Spinelli P., Suson D. J., Tajima H., Takahashi M., Tanaka Y., Thayer J. B., Thompson D. J., Tibaldo L., Torres D. F., Torresi E., Tosti G., Troja E., Valverde J., Vianello G., Vogel M., Wood K., Wood M., Zaharijas G., Ahnen M. L., Ansoldi S., Antonelli L. A., Arcaro C., Baack D., Babic A., Banerjee B., Bangale P., de Almeida U. Barres, Barrio J. A., Gonzalez J. Becerra, Bednarek W., Bernardini E., Berti A., Bhattacharyya W., Biland A., Blanch O., Bonnoli G., Carosi A., Carosi R., Ceribella G., Chatterjee A., Colak S. M., Colin P., Colombo E., Contreras J. L., Cortina J., Covino S., Cumani P., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Delfino M., Delgado J., Di Pierro F., Dominguez A., Prester D. . Dominis, Dorner D., Doro M., Einecke S., Elsaesser D., Ramazani V. Fallah, Fernandez-Barral A., Fidalgo D., Foffano L., Pfrang K., Fonseca M. V., Font L., Franceschini A., Fruck C., Galindo D., Gallozzi S., Lopez R. J. Garcia, Garczarczyk M., Gaug M., Giammaria P., Godinovic N., Gora D., Guberman D., Hadasch D., Hahn A., Hassan T., Hayashida M., Herrera J., Hose J., Hrupec D., Inoue S., Ishio K., Konno Y., Kubo H., Kushida J., Lelas D., Lindfors E., Lombardi S., Longo F., Lopez M., Maggio C., Majumdar P., Makariev M., Maneva G., Manganaro M., Mannheim K., Maraschi L., Mariotti M., Martinez M., Masuda S., Mazin D., Minev M., M J. M., Mirzoyan R., Moralejo A., Moreno V., Moretti E., Nagayoshi T., Neustroev V., Niedzwiecki A., Rosillo M. Nievas, Nigro C., Nilsson K., Ninci D., Nishijima K., Noda K., Nogues L., Paiano S., Palacio J., Paneque D., Paoletti R., Paredes J. M., Pedaletti G., Peresano M., Persic M., Moroni P. G. Prada, Prandini E., Puljak I., Garcia J. Rodriguez, Reichardt I., Rhode W., Ribo M., Rico J., Righi C., Rugliancich A., Saito T., Satalecka K., Schweizer T., Sitarek J., Snidaric I., Sobczynska D., Stamerra A., Strzys M., Suric T., Takahashi M., Tavecchio F., Temnikov P., Terzic T., Teshima M., Torres-Alba N., Treves A., Tsujimoto S., Vanzo G., Acosta M. Vazquez, Vovk I., Ward J. E., Will M., Zaric D., Lucarelli F., Tavani M., Piano G., Donnarumma I., Pittori C., Verrecchia F., Barbiellini G., Bulgarelli A., Caraveo P., Cattaneo P. W., Colafrancesco S., Costa E., Di Cocco G., Ferrari A., Gianotti F., Giuliani A., Lipari P., Mereghetti S., Morselli A., Pacciani L., Paoletti F., Parmiggiani N., Pellizzoni A., Picozza P., Pilia M., Rappoldi A., Trois A., Vercellone S., Vittorini V., Franckowiak A., Stanek K. Z., Kochanek C. S., Beacom J. F., Thompson T. A., Holoien W. -S., Dong S., Prieto J. L., Shappee B. J., Holmbo S., Abeysekara A. U., Albert A., Alfaro R., Alvarez C., Arceo R., Arteaga-Velazquez J. C., Rojas D. Avila, Solares H. A. Ayala, Becerril A., Belmont-Moreno E., Bernal A., Caballero-Mora K. S., Capistran T., Carraminana A., Casanova S., Castillo M., Cotti U., Cotzomi J., de Leon S. Coutino, De Leon C., De la Fuente E., Hernandez R. Diaz, Dichiara S., Dingus B. L., DuVernois M. A., Diaz-Velez J. C., Ellsworth R. W., Engel K., Fiorino D. W., Fleischhack H., Fraija N., Garcia-Gonzalez J. A., Garfias F., Munoz A. Gonzalez, Gonzalez M. M., Goodman J. A., Hampel-Arias Z., Harding J. P., Hernandez S., Hona B., Hueyotl-Zahuantitla F., Hui C. M., Huntemeyer P., Iriarte A., Jardin-Blicq A., Joshi V., Kaufmann S., Kunde G. J., Lara A., Lauer R. J., Lee W. H., Lennarz D., Vargas H. Leon, Linnemann J. T., Longinotti A. L., Luis-Raya G., Luna-Garcia R., Malone K., Marinelli S. S., Martinez O., Martinez-Castellanos I., Martinez-Castro J., Martinez-Huerta H., Matthews J. A., Miranda-Romagnoli P., Moreno E., Mostafa M., Nayerhoda A., Nellen L., Newbold M., Nisa M. U., Noriega-Papaqui R., Pelayo R., Pretz J., Perez-Perez E. G., Ren Z., Rho C. D., Riviere C., Rosa-Gonzalez D., Rosenberg M., Ruiz-Velasco E., Ruiz-Velasco E., Greus F. Salesa, Sandoval A., Schneider M., Schoorlemmer H., Sinnis G., Smith A. J., Springer R. W., Surajbali P., Tibolla O., Tollefson K., Torres I., Villasenor L., Weisgarber T., Werner F., Yapici T., Gaurang Y., Zepeda A., Zhou H., Alvarez J. D., Abdalla H., Anguner E. O., Armand C., Backes M., Becherini Y., Berge D., Bottcher M., Boisson C., Bolmont J., Bonnefoy S., Bordas P., Brun F., Buchele M., Bulik T., Caroff S., Carosi A., Casanova S., Cerruti M., Chakraborty N., Chandra S., Chen A., Colafrancesco S., Davids I. D., Deil C., Devin J., Djannati-Atai A., Egberts K., Emery G., Eschbach S., Fiasson A., Fontaine G., Funk S., Fussling M., Gallant Y. A., Gate F., Giavitto G., Glawion D., Glicenstein J. F., Gottschall D., Grondin M. -H., Haupt M., Henri G., Hinton J. A., Hoischen C., Holch T. L., Huber D., Jamrozy M., Jankowsky D., Jankowsky F., Jouvin L., Jung-Richardt I., Kerszberg D., Khelifi B., King J., Klepser S., Kluzniak W., Komin Nu., Kraus M., Lefaucheur J., Lemiere A., Lemoine-Goumard M., Lenain J. -P., Leser E., Lohse T., Lopez-Coto R., Lorentz M., Lypova I., Marandon V., Marti-Devesa G. Guillem, Maurin G., Mitchell A. M. W., Moderski R., Mohamed M., Mohrmann L., Moulin E., Murach T., de Naurois M., Niederwanger F., Niemiec J., Oakes L., O'Brien P., Ohm S., Ostrowski M., Oya I., Panter M., Parsons R. D., Perennes C., Piel Q., Pita S., Poireau V., Noel A. Priyana, Prokoph H., Puhlhofer G., Quirrenbach A., Raab S., Rauth R., Renaud M., Rieger F., Rinchiuso L., Romoli C., Rowell G., Rudak B., Sanchez D. A., Sasaki M., Schlickeiser R., Schussler F., Schulz A., Schwanke U., Seglar-Arroyo M., Shafi N., Simoni R., Sol H., Stegmann C., Steppa C., Tavernier T., Taylor A. M., Tiziani D., Trichard C., Tsirou M., van Eldik C., van Rensburg C., van Soelen B., Veh J., Vincent P., Voisin F., Wagner S. J., Wagner R. M., Wierzcholska A., Zanin R., Zdziarski A. A., Zech A., Ziegler A., Zorn J., Zywucka N., Savchenko V., Ferrigno C., Bazzano A., Diehl R., Kuulkers E., Laurent P., Mereghetti S., Natalucci L., Panessa F., Rodi J., Ubertini P., Morokuma T., Ohta K., Tanaka Y. T., Mori H., Yamanaka M., Kawabata K. S., Utsumi Y., Nakaoka T., Kawabata M., Nagashima H., Yoshida M., Matsuoka Y., Itoh R., Keel W., Copperwheat C., Steele I., Cenko S. B., Cowen D. F., DeLaunay J. J., Evans P. A., Fox D. B., Keivani A., Kennea J. A., Marshall F. E., Osborne J. P., Santander M., Tohuvavohu A., Turley C. F., Abeysekara A. U., Archer A., Benbow W., Bird R., Brill A., Brose R., Buchovecky M., Buckley J. H., Bugaev V., Christiansen J. L., Connolly M. P., Cui W., Daniel M. K., Errando M., Falcone A., Feng Q., Finley J. P., Fortson L., Furniss A., Gueta O., Hutten M., Hervet O., Hughes G., Humensky T. B., Johnson C. A., Kaaret P., Kar P., Kelley-Hoskins N., Kertzman M., Kieda D., Krause M., Krennrich F., Kumar S., Lang M. J., Lin T. T. Y., Maier G., McArthur S., Moriarty P., Mukherjee R., Nieto D., O'Brien S., Ong R. A., Otte A. N., Park N., Petrashyk A., Pohl M., Popkow A., Pueschel E., Quinn J., Ragan K., Reynolds P. T., Richards G. T., Roache E., Rulten C., Sadeh I., Santander M., Scott S. S., Sembroski G. H., Shahinyan K., Sushch I., Trepanier S., Tyler J., Vassiliev V. V., Wakely S. P., Weinstein A., Wells R. M., Wilcox P., Wilhelm A., Williams D. A., Zitzer B., Tetarenko A. J., Kimball A. E., Miller-Jones J. C. A., Sivakoff G. R.

    SCIENCE   Vol. 361 ( 6398 )   2018.7

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    DOI: 10.1126/science.aat1378

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  65. Fermi-LAT Observations of LIGO/Virgo Event GW170817 Reviewed

    Ajello M., Allafort A., Axelsson M., Baldini L., Barbiellini G., Baring M. G., Bastieri D., Bellazzini R., Berenji B., Bissaldi E., Blandford R. D., Bloom E. D., Bonino R., Bottacini E., Brandt T. J., Bregeon J., Bruel P., Buehler R., Burnett T. H., Buson S., Cameron R. A., Caputo R., Caraveo P. A., Casandjian J. M., Cavazzuti E., Chekhtman A., Cheung C. C., Chiang J., Chiaro G., Ciprini S., Cohen-Tanugi J., Cominsky L. R., Costantin D., Cuoco A., Cutini S., D'Ammando F., de Palma F., Di Lalla N., Di Mauro M., Di Venere L., Dubois R., Dumora D., Favuzzi C., Ferrara E. C., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Gill R., Giordano F., Giroletti M., Glanzman T., Granot J., Green D., Grenier I. A., Grondin M. -H., Guillemot L., Guiriec S., Harding A. K., Hays E., Horan D., Imazato F., Johannesson G., Kamae T., Kensei S., Kocevski D., Kuss M., La Mura G., Larsson S., Latronico L., Li J., Longo F., Loparco F., Lovellette M. N., Lubrano P., Magill J. D., Maldera S., Manfreda A., Mazziotta M. N., Michelson P. F., Mizuno T., Moiseev A. A., Monzani M. E., Moretti E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Ojha R., Omodei N., Orlando E., Ormes J. F., Palatiello M., Paliya V. S., Paneque D., Persic M., Pesce-Rollins M., Petrosian V., Piron F., Porter T. A., Principe G., Racusin J. L., Raino S., Rando R., Razzano M., Razzaque S., Reimer A., Reimer O., Ritz S., Rochester L. S., Ryde F., Parkinson P. M. Saz, Sgro C., Siskind E. J., Spada F., Spandre G., Spinelli P., Suson D. J., Tajima H., Takahashi M., Tak D., Thayer J. G., Thayer J. B., Torres D. F., Torresi E., Tosti G., Troja E., Valverde J., Venters T. M., Vianello G., Wood K., Yang C., Zaharijas G.

    ASTROPHYSICAL JOURNAL   Vol. 861 ( 2 )   2018.7

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    DOI: 10.3847/1538-4357/aac515

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  66. Search for Gamma-Ray Emission from the Coma Cluster with Six Years of Fermi-LAT Data (vol 819, 149, 2016) Reviewed

    Ackermann M., Ajello M., Albert A., Atwood W. B., Baldini L., Ballet J., Barbiellini G., Bastieri D., Bechtol K., Bellazzini R., Bissaldi E., Blandford R. D., Bloom E. D., Bonino R., Bottacini E., Bregeon J., Bruel P., Buehler R., Caliandro G. A., Cameron R. A., Caragiulo M., Caraveo P. A., Casandjian J. M., Cavazzuti E., Cecchi C., Charles E., Chekhtman A., Chiaro G., Ciprini S., Cohen-Tanugi J., Conrad J., Cutini S., D'Ammando F., de Angelis A., de Palma F., Desiante R., Digel S. W., Di Venere L., Drell P. S., Favuzzi C., Fegan S. J., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Godfrey G., Green D., Grenier I. A., Guiriec S., Hays E., Hewitt J. W., Horan D., Johannesson G., Kuss M., Larsson S., Latronico L., Li J., Li L., Longo F., Loparco F., Lovellette M. N., Lubrano P., Madejski G. M., Maldera S., Manfreda A., Mayer M., Mazziotta M. N., Michelson P. F., Mitthumsiri W., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Murgia S., Nuss E., Ohsugi T., Orienti M., Orlando E., Ormes J. F., Paneque D., Pesce-Rollins M., Petrosian V., Piron F., Pivato G., Porter T. A., Raino S., Rando R., Razzano M., Reimer A., Reimer O., Sanchez-Conde M., Sgro C., Siskind E. J., Spada F., Spandre G., Spinelli P., Tajima H., Takahashi H., Thayer J. B., Tibaldo L., Torres D. F., Tosti G., Troja E., Vianello G., Wood K. S., Zimmer S., Rephaeli Y.

    ASTROPHYSICAL JOURNAL   Vol. 860 ( 1 )   2018.6

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    DOI: 10.3847/1538-4357/aac7c3

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  67. The PoGO plus view on Crab off-pulse hard X-ray polarization Reviewed

    Chauvin M., Floren H. -G., Friis M., Jackson M., Kamae T., Kataoka J., Kawano T., Kiss M., Mikhalev V., Mizuno T., Tajima H., Takahashi H., Uchida N., Pearce M.

    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY   Vol. 477 ( 1 ) page: L45 - L49   2018.6

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    DOI: 10.1093/mnrasl/sly027

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  68. Hitomi X-ray observation of the pulsar wind nebula G21.5-0.9 Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, O; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Nobukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemtsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Uno, S; Ueda, Y; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A; Sato, T; Nakaniwa, N; Murakami, H; Guest, B

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 3 )   2018.6

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    DOI: 10.1093/pasj/psy027

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  69. Modeling of proton-induced radioactivation background in hard X-ray telescopes: Geant4-based simulation and its demonstration by Hitomi's measurement in a low Earth orbit Reviewed

    Odaka Hirokazu, Asai Makoto, Hagino Kouichi, Koi Tatsumi, Madejski Greg, Mizuno Tsunefumi, Ohno Masanori, Saito Shinya, Sato Tamotsu, Wright Dennis H., Enoto Teruaki, Fukazawa Yasushi, Hayashi Katsuhiro, Kataoka Jun, Katsuta Junichiro, Kawaharada Madoka, Kobayashi Shogo B., Kokubun Motohide, Laurent Philippe, Lebrun Francois, Limousin Olivier, Maier Daniel, Makishima Kazuo, Mimura Taketo, Miyake Katsuma, Mori Kunishiro, Murakami Hiroaki, Nakamori Takeshi, Nakano Toshio, Nakazawa Kazuhiro, Noda Hirofumi, Ohta Masayuki, Ozaki Masanobu, Sato Goro, Sato Rie, Tajima Hiroyasu, Takahashi Hiromitsu, Takahashi Tadayuki, Takeda Shin'ichiro, Tanaka Takaaki, Tanaka Yasuyuki, Terada Yukikatsu, Uchiyama Hideki, Uchiyama Yasunobu, Watanabe Shin, Yamaoka Kazutaka, Yasuda Tetsuya, Yatsu Yoichi, Yuasa Takayuki, Zoglauer Andreas

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 891   page: 92 - 105   2018.5

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    DOI: 10.1016/j.nima.2018.02.071

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  70. Shedding new light on the Crab with polarized X-rays (vol 7, 7816, 2017) Reviewed

    Chauvin M., Floren H. -G., Friis M., Jackson M., Kamae T., Kataoka J., Kawano T., Kiss M., Mikhalev V., Mizuno T., Ohashi N., Stana T., Tajima H., Takahashi H., Uchida N., Pearce M.

    SCIENTIFIC REPORTS   Vol. 8   2018.5

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    DOI: 10.1038/s41598-018-24853-7

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    PubMed

  71. Search for Gamma-Ray Emission from Local Primordial Black Holes with the Fermi Large Area Telescope Reviewed

    Ackermann M., Atwood W. B., Baldini L., Ballet J., Barbiellini G., Bastieri D., Bellazzini R., Berenji B., Bissaldi E., Blandford R. D., Bloom E. D., Bonino R., Bottacini E., Bregeon J., Bruel P., Buehler R., Cameron R. A., Caputo R., Caraveo P. A., Cavazzuti E., Charles E., Chekhtman A., Cheung C. C., Chiaro G., Ciprini S., Cohen-Tanugi J., Conrad J., Costantin D., D'Ammando F., de Palma F., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Favuzzi C., Fegan S. J., Focke W. B., Franckowiak A., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Grenier I. A., Guillemot L., Guiriec S., Horan D., Johannesson G., Johnson C., Kensei S., Kocevski D., Kuss M., Larsson S., Latronico L., Li J., Longo F., Loparco F., Lovellette M. N., Lubrano P., Magill J. D., Maldera S., Malyshev D., Manfreda A., Mazziotta M. N., McEnery J. E., Meyer M., Michelson P. F., Mitthumsiri W., Mizuno T., Monzani M. E., Moretti E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Ojha R., Omodei N., Orienti M., Orlando E., Ormes J. F., Palatiello M., Paliya V. S., Paneque D., Persic M., Pesce-Rollins M., Piron F., Principe G., Raino S., Rando R., Razzano M., Razzaque S., Reimer A., Reimer O., Ritz S., Sanchez-Conde M., Sgro C., Siskind E. J., Spada F., Spandre G., Spinelli P., Suson D. J., Tajima H., Thayer J. G., Thayer J. B., Torres D. F., Tosti G., Troja E., Valverde J., Vianello G., Wood K., Wood M., Zaharijas G.

    ASTROPHYSICAL JOURNAL   Vol. 857 ( 1 )   2018.4

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    DOI: 10.3847/1538-4357/aaac7b

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  72. Design and performance of Soft Gamma-ray Detector onboard the Hitomi (ASTRO-H) satellite Reviewed International coauthorship

    Tajima Hiroyasu, Watanabe Shin, Fukazawa Yasushi, Blandford Roger, Enoto Teruaki, Goldwurm Andrea, Hagino Kouichi, Hayashi Katsuhiro, Ichinohe Yuto, Kataoka Jun, Katsuta Jun'ichiro, Kitaguchi Takao, Kokubun Motohide, Laurent Philippe, Lebrun Francois, Limousin Olivier, Madejski Grzegorz M., Makishima Kazuo, Mizuno Tsunefumi, Mori Kunishiro, Nakamori Takeshi, Nakano Toshio, Nakazawa Kazuhiro, Noda Hirofumi, Odaka Hirokazu, Ohno Masanori, Ohta Masayuki, Saito Shinya, Sato Goro, Sato Rie, Takeda Shin'ichiro, Takahashi Hiromitsu, Takahashi Tadayuki, Tanaka Takaaki, Tanaka Yasuyuki, Terada Yukikatsu, Uchiyama Hideki, Uchiyama Yasunobu, Yamaoka Kazutaka, Yatsu Yoichi, Yonetoku Daisuke, Yuasao Takayuki

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 4 ( 2 )   2018.4

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    DOI: 10.1117/1.JATIS.4.2.021411

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  73. In-orbit performance and calibration of the Hard X-ray Imager onboard Hitomi (ASTRO-H) Reviewed

    Hagino Kouichi, Nakazawa Kazuhiro, Sato Goro, Kokubun Motohide, Enoto Teruaki, Fukazawa Yasushi, Hayashi Katsuhiro, Kataoka Jun, Katsuta Junichiro, Kobayashi Shogo B., Laurent Philippe, Lebrun Francois, Limousin Olivier, Maier Daniel, Makishima Kazuo, Mimura Taketo, Miyake Katsuma, Mizuno Tsunefumi, Mori Kunishiro, Murakami Hiroaki, Nakamori Takeshi, Nakano Toshio, Noda Hirofumi, Odaka Hirokazu, Ohno Masanori, Ohta Masayuki, Saito Shinya, Sato Rie, Tajima Hiroyasu, Takahashi Hiromitsu, Takahashi Tadayuki, Takeda Shin'ichiro, Tanaka Takaaki, Terada Yukikatsu, Uchiyama Hideki, Uchiyama Yasunobu, Watanabe Shin, Yamaoka Kazutaka, Yatsu Yoichi, Yuasa Takayuki

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 4 ( 2 )   2018.4

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    DOI: 10.1117/1.JATIS.4.2.021409

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  74. Hitomi (ASTRO-H) X-ray Astronomy Satellite Reviewed

    Takahashi Tadayuki, Kokubun Motohide, Mitsuda Kazuhisa, Kelley Richard L., Ohashi Takaya, Aharonian Felix, Akamatsu Hiroki, Akimoto Fumie, Allen Steven W., Anabuki Naohisa, Angelini Lorella, Arnaud Keith, Asai Makoto, Audard Marc, Awaki Hisamitsu, Axelsson Magnus, Azzarello Philipp, Baluta Chris, Bamba Aya, Bando Nobutaka, Bautz Marshall W., Bialas Thomas, Blandford Roger, Boyce Kevin, Brenneman Laura W., Brown Gregory V., Bulbul Esra, Cackett Edward M., Canavan Edgar, Chernyakova Maria, Chiao Meng P., Coppi Paolo S., Costantini Elisa, Dell Steve O', DiPirro Michael, Done Chris, Dotani Tadayasu, Doty John, Ebisawa Ken, Eckart Megan E., Enoto Teruaki, Ezoe Yuichiro, Fabian Andrew C., Ferrigno Carlo, Foster Adam R., Fujimoto Ryuichi, Fukazawa Yasushi, Funk Stefan, Furuzawa Akihiro, Galeazzi Massimiliano, Gallo Luigi C., Gandhi Poshak, Gilmore Kirk, Giustini Margherita, Goldwurm Andrea, Gu Liyi, Guainazzi Matteo, Haas Daniel, Haba Yoshito, Hagino Kouichi, Hamaguchi Kenji, Harrus Ilana M., Hatsukade Isamu, Hayashi Takayuki, Hayashi Katsuhiro, Hayashida Kiyoshi, den Herder Jan-Willem, Hiraga Junko S., Hirose Kazuyuki, Hornschemeier Ann, Hoshino Akio, Hughes John P., Ichinohe Yuto, Iizuka Ryo, Inoue Hajime, Inoue Yoshiyuki, Ishibashi Kazunori, Ishida Manabu, Ishikawa Kumi, Ishimura Kosei, Ishisaki Yoshitaka, Itoh Masayuki, Iwai Masachika, Iwata Naoko, Iyomoto Naoko, Jewell Chris, Kaastra Jelle, Kallman Tim, Kamae Tsuneyoshi, Kara Erin, Kataoka Jun, Katsuda Satoru, Katsuta Junichiro, Kawaharada Madoka, Kawai Nobuyuki, Kawano Taro, Kawasaki Shigeo, Khangulyan Dmitry, Kilbourne Caroline A., Kimball Mark, King Ashley, Kitaguchi Takao, Kitamoto Shunji, Kitayama Tetsu, Kohmura Takayoshi, Konami Saori, Kosaka Tatsuro, Koujelev Alex, Koyama Katsuji, Koyama Shu, Kretschmar Peter, Krimm Hans A., Kubota Aya, Kunieda Hideyo, Laurent Philippe, Lee Shiu-Hang, Leutenegger Maurice A., Limousin Olivier, Loewenstein Michael, Long Knox S., Lumb David, Madejski Greg, Maeda Yoshitomo, Maier Daniel, Makishima Kazuo, Markevitch Maxim, Masters Candace, Matsumoto Hironori, Matsushita Kyoko, McCammon Dan, Mcguinness Daniel, McNamar Brian R., Mehdipour Missagh, Miko Joseph, Miller Eric D., Miller Jon M., Mineshige Shin, Minesugi Kenji, Mitsuishi Ikuyuki, Miyazawa Takuya, Mizuno Tsunefumi, Mori Hideyuki, Mori Koji, Moroso Franco, Moseley Harvey, Muench Theodore, Mukai Koji, Murakami Hiroshi, Murakami Toshio, Mushotzky Richard F., Nagano Housei, Nagino Ryo, Nakagawa Takao, Nakajima Hiroshi, Nakamori Takeshi, Nakano Toshio, Nakashima Shinya, Nakazawa Kazuhiro, Namba Yoshiharu, Natsukari Chikara, Nishioka Yusuke, Nobukawa Kumiko K., Nobukawa Masayoshi, Noda Hirofumi, Nomachi Masaharu, Odaka Hirokazu, Ogawa Hiroyuki, Ogawa Mina, Ogi Keiji, Ohno Masanori, Ohta Masayuki, Okajima Takashi, Okamoto Atsushi, Okazaki Tsuyoshi, Ota Naomi, Ozaki Masanobu, Paerels Frits, Paltani Stephane, Parmar Arvind, Petre Robert, Pinto Ciro, de Plaa Jelle, Pohl Martin, Pontius James, Porter Frederick S., Pottschmidt Katja, Ramsey Brian, Reynolds Christopher, Russell Helen, Safi-Harb Samar, Saito Shinya, Sakai Kazuhiro, Sakai Shin-ichiro, Sameshima Hiroaki, Sasaki Toru, Sato Goro, Sato Kosuke, Sato Rie, Sato Yoichi, Sawada Makoto, Schartel Norbert, Serlemitsos Peter J., Seta Hiromi, Shibano Yasuko, Shida Maki, Shidatsu Megumi, Shimada Takanobu, Shinozaki Keisuke, Shirron Peter, Simionescu Aurora, Simmons Cynthia, Smith Randall K., Sneiderman Gary, Soong Yang, Stawarz Lukasz, Sugawara Yasuharu, Sugita Satoshi, Sugita Hiroyuki, Szymkowiak Andrew, Tajima Hiroyasu, Takahashi Hiromitsu, Takeda Shin'ichiro, Takei Yoh, Tamagawa Toru, Tamura Takayuki, Tamura Keisuke, Tanaka Takaaki, Tanaka Yasuo, Tanaka Yasuyuki T., Tashiro Makoto S., Tawara Yuzuru, Terada Yukikatsu, Terashima Yuichi, Tombesi Francesco, Tomida Hiroshi, Tsuboi Yohko, Tsujimoto Masahiro, Tsunemi Hiroshi, Tsuru Takeshi Go, Uchida Hiroyuki, Uchiyama Hideki, Uchiyama Yasunobu, Ueda Shutaro, Ueda Yoshihiro, Ueno Shiro, Uno Shin'ichiro, Urry C. Megan, Ursino Eugenio, de Vries Cor P., Wada Atsushi, Watanabe Shin, Watanabe Tomomi, Werner Norbert, Wik Daniel R., Wilkins Dan R., Williams Brian J., Yamada Shinya, Yamada Takahiro, Yamaguchi Hiroya, Yamaoka Kazutaka, Yamasaki Noriko Y., Yamauchi Makoto, Yamauchi Shigeo, Yaqoob Tahir, Yatsu Yoichi, Yonetoku Daisuke, Yoshida Atsumasa, Yuasa Takayuki, Zhuravleva Irina, Zoghbi Abderahmen

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 4 ( 2 )   2018.4

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    DOI: 10.1117/1.JATIS.4.2.021402

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  75. Hard x-ray imager onboard Hitomi (ASTRO-H) Reviewed

    Nakazawa Kazuhiro, Sato Goro, Kokubun Motohide, Enoto Teruaki, Fukazawa Yasushi, Hagino Kouichi, Hayashi Katsuhiro, Kataoka Jun, Katsuta Junichiro, Kobayashi Shogo B., Laurent Philippe, Lebrun Francois, Limousin Olivier, Maier Daniel, Makishima Kazuo, Mizuno Tsunefumi, Mori Kunishiro, Nakamori Takeshi, Nakano Toshio, Noda Hirofumi, Odaka Hirokazu, Ohno Masanori, Ohta Masayuki, Saito Shinya, Sato Rie, Tajima Hiroyasu, Takahashi Hiromitsu, Takahashi Tadayuki, Takeda Shin'ichiro, Tanaka Takaaki, Terada Yukikatsu, Uchiyama Hideki, Uchiyama Yasunobu, Watanabe Shin, Yamaoka Kazutaka, Yatsu Yoichi, Yuasa Takayuki

    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS   Vol. 4 ( 2 )   2018.4

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    DOI: 10.1117/1.JATIS.4.2.021410

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  76. Atmospheric gas dynamics in the Perseus cluster observed with Hitomi Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Canning, REA; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, S; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, O; Loewenstein, M; Long, KS; Lumr, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, K; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Wang, QHS; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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    DOI: 10.1093/pasj/psx138

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  77. Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, O; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sato, T; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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    DOI: 10.1093/pasj/psx151

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  78. Hitomi observation of radio galaxy NGC 1275: The first X-ray microcalorimeter spectroscopy of Fe-Kα line emission from an active galactic nucleus Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, OO; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A; Kawamuro, T

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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  79. Glimpse of the highly obscured HMXB IGR J16318-4848 with Hitomi Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, OO; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A; Nakaniwa, N

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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    DOI: 10.1093/pasj/psx154

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  80. Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hell, N; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, OO; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A; Raassen, AJJ

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    DOI: 10.1093/pasj/psx156

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  81. Hitomi X-ray studies of giant radio pulses from the Crab pulsar Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; De Plaa, J; De Vries, CP; Den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, OO; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Nobukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Oshimizu, K; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemtsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A; Terasawa, T; Sekido, M; Takefuji, K; Kawai, E; Misawa, H; Tsuchiya, F; Yamazaki, R; Kobayashi, E; Kisaka, S; Aoki, T

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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    DOI: 10.1093/pasj/psx083

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  82. Temperature structure in the Perseus cluster core observed with Hitomi Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furukawa, M; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Kato, Y; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, O; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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    DOI: 10.1093/pasj/psy004

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  83. Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguch, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, O; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Nobukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sato, T; Sawada, M; Schartel, N; Serlemtsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A; Tominaga, N; Moriya, TJ

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    DOI: 10.1093/pasj/psx072

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  84. Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS Reviewed

    Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H; Axelsson, M; Bamba, A; Bautz, MW; Blandford, R; Brenneman, LW; Brown, GV; Bulbul, E; Cackett, EM; Chernyakova, M; Chiao, MP; Coppi, PS; Costantini, E; de Plaa, J; de Vries, CP; den Herder, JW; Done, C; Dotani, T; Ebisawa, K; Eckart, ME; Enoto, T; Ezoe, Y; Fabian, AC; Ferrigno, C; Foster, AR; Fujimoto, R; Fukazawa, Y; Furukawa, M; Furuzawa, A; Galeazzi, M; Gallo, LC; Gandhi, P; Giustini, M; Goldwurm, A; Gu, LY; Guainazzi, M; Haba, Y; Hagino, K; Hamaguchi, K; Harrus, IM; Hatsukade, I; Hayashi, K; Hayashi, T; Hayashida, K; Hiraga, JS; Hornschemeier, A; Hoshino, A; Hughes, JP; Ichinohe, Y; Iizuka, R; Inoue, H; Inoue, Y; Ishida, M; Ishikawa, K; Ishisaki, Y; Iwai, M; Kaastra, J; Kallman, T; Kamae, T; Kataoka, J; Katsuda, S; Kawai, N; Kelley, RL; Kilbourne, CA; Kitaguchi, T; Kitamoto, S; Kitayama, T; Kohmura, T; Kokubun, M; Koyama, K; Koyama, S; Kretschmar, P; Krimm, HA; Kubota, A; Kunieda, H; Laurent, P; Lee, SH; Leutenegger, MA; Limousin, OO; Loewenstein, M; Long, KS; Lumb, D; Madejski, G; Maeda, Y; Maier, D; Makishima, K; Markevitch, M; Matsumoto, H; Matsushita, K; McCammon, D; McNamara, BR; Mehdipour, M; Miller, ED; Miller, JM; Mineshige, S; Mitsuda, K; Mitsuishi, I; Miyazawa, T; Mizuno, T; Mori, H; Mori, K; Mukai, K; Murakami, H; Mushotzky, RF; Nakagawa, T; Nakajima, H; Nakamori, T; Nakashima, S; Nakazawa, K; Norukawa, KK; Nobukawa, M; Noda, H; Odaka, H; Ogorzalek, A; Ohashi, T; Ohno, M; Okajima, T; Ota, N; Ozaki, M; Paerels, F; Paltani, S; Petre, R; Pinto, C; Porter, FS; Pottschmidt, K; Reynolds, CS; Safi-Harb, S; Saito, S; Sakai, K; Sasaki, T; Sato, G; Sato, K; Sato, R; Sawada, M; Schartel, N; Serlemitsos, PJ; Seta, H; Shidatsu, M; Simionescu, A; Smith, RK; Soong, Y; Stawarz, L; Sugawara, Y; Sugita, S; Szymkowiak, A; Tajima, H; Takahashi, H; Takahashi, T; Takeda, S; Takei, Y; Tamagawa, T; Tamura, T; Tanaka, T; Tanaka, Y; Tanaka, YT; Tashiro, MS; Tawara, Y; Terada, Y; Terashima, Y; Tombesi, F; Tomida, H; Tsuboi, Y; Tsujimoto, M; Tsunemi, H; Tsuru, TG; Uchida, H; Uchiyama, H; Uchiyama, Y; Ueda, S; Ueda, Y; Uno, S; Urry, CM; Ursino, E; Watanabe, S; Werner, N; Wilkins, DR; Williams, BJ; Yamada, S; Yamaguchi, H; Yamaoka, K; Yamasaki, NY; Yamauchi, M; Yamauchi, S; Yaqoob, T; Yatsu, Y; Yonetoku, D; Zhuravleva, I; Zoghbi, A

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   Vol. 70 ( 2 )   2018.3

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  85. Solar Neutron and Gamma-ray Spectrometer For a Small Satellite Reviewed

    Yamaoka Kazutaka, Tajima Hiroyasu, Itow Yoshitaka, Fujii Hirosame, Nakanishi Yuta, Kamei Yuhei, Yamakawa Takeharu, Niwa Takumi, Okui Itsuki, Miyata Kikuko, Inamori Takaya

    HARD X-RAY, GAMMA-RAY, AND NEUTRON DETECTOR PHYSICS XX   Vol. 10762   2018

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    DOI: 10.1117/12.2323451

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  86. Final characterisation and design of the Gamma-ray Cherenkov Telescope (GCT) for the Cherenkov Telescope Array Reviewed

    Le Blanc O., Fasola G., Huet J. M., White R., Dmytriiev A., Sol H., Zech A., Abchiche A., Amans J. P., Armstrong T. P., Barcelo M., Berge D., Brown A. M., Buchholtz G., Chadwick P. M., Clark P., Cotter G., Dangeon L., De Frondat F., Deiml P., Dournaux J. L., Duffy C., Einecke S., Flis S., Funk S., Giavitto G., Gironnet J., Graham J. A., Greenshaw T., Hinton J. A., Jegouzo I., Kraus M., Lapington J. S., Laporte P., Leach S. A., Lloyd S., Minaya I. A., Morier R., Okumura A., Prokoph H., Ross D., Rowell G., Rulten C. B., Schoorlemmer H., Schmoll J., Spencer S. T., Stephan M., Stuik R., Tajima H., Thornhill J., Tibaldo L., Vink J., Watson J. J., Williams J., Zink A., Zorn J.

    GROUND-BASED AND AIRBORNE TELESCOPES VII   Vol. 10700   2018

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    DOI: 10.1117/12.2313158

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  87. The GCT camera for the Cherenkov Telescope Array Reviewed

    CTA GCT Team

    Nuclear Instruments and Methods in Physics Research Section A   Vol. 876   page: 1 - 4   2017.12

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    DOI: 10.1016/j.nima.2016.12.010

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  88. Solar abundance ratios of the iron-peak elements in the Perseus cluster Reviewed

    Hitomi collaboration

    Nature   Vol. 551 ( 7681 ) page: 478 - +   2017.11

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    DOI: 10.1038/nature24301

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  89. Shedding new light on the Crab with polarized X-rays Reviewed

    Chauvin M., Floren H. -G., Friis M., Jackson M., Kamae T., Kataoka J., Kawano T., Kiss M., Mikhalev V., Mizuno T., Ohashi N., Stana T., Tajima H., Takahashi H., Uchida N., Pearce M.

    SCIENTIFIC REPORTS   Vol. 7   2017.8

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    DOI: 10.1038/s41598-017-07390-7

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  90. TARGET 5: A new multi-channel digitizer with triggering capabilities for gamma-ray atmospheric Cherenkov telescopes Reviewed International coauthorship

    Albert A., Funk S., Katagiri H., Kawashima T., Murphy M., Okumura A., Quagliani R., Sapozhnikov L., Shigenaka A., Tajima H., Tibaldo L., Vandenbroucke J., Varner G., Wu T.

    ASTROPARTICLE PHYSICS   Vol. 92   page: 49 - 61   2017.6

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    DOI: 10.1016/j.astropartphys.2017.05.003

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  91. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946 Reviewed

    Acero F., Aloisio R., Amans J., Amato E., Antonelli L. A., Aramo C., Armstrong T., Arqueros F., Asano K., Ashley M., Backes M., Balazs C., Balzer A., Bamba A., Barkov M., Barrio J. A., Benbow W., Bernloehr K., Beshley V., Bigongiari C., Biland A., Bilinsky A., Bissaldi E., Biteau J., Blanch O., Blasi P., Blazek J., Boisson C., Bonanno G., Bonardi A., Bonavolonta C., Bonnoli G., Braiding C., Brau-Nogue S., Bregeon J., Brown A. M., Bugaev V., Bulgarelli A., Bulik T., Burton M., Burtovoi A., Busetto G., Bottcher M., Cameron R., Capalbi M., Caproni A., Caraveo P., Carosi R., Cascone E., Cerruti M., Chaty S., Chen A., Chen X., Chernyakova M., Chikawa M., Chudoba J., Cohen-Tanugi J., Colafrancesco S., Conforti V., Contreras J. L., Costa A., Cotter G., Covino S., Covone G., Cumani P., Cusumano G., D'Ammando F., D'Urso D., Daniel M., Dazzi F., De Angelis A., De Cesare G., De Franco A., De Frondat F., Dal Pino E. M. de Gouveia, De Lisio C., Lopez R. de los Reyes, De Lotto B., de Naurois M., De Palma F., Del Santo M., Delgado C., della Volpe D., Di Girolamo T., Di Giulio C., Di Pierro F., Di Venere L., Doro M., Dournaux J., Dumas D., Dwarkadas V., Diaz C., Ebr J., Egberts K., Einecke S., Elsaesser D., Eschbach S., Falceta-Goncalves D., Fasola G., Fedorova E., Fernandez-Barral A., Ferrand G., Fesquet M., Fiandrini E., Fiasson A., Filipovic M. D., Fioretti V., Font L., Fontaine G., Franco F. J., Freixas Coromina L., Fujita Y., Fukui Y., Funk S., Forster A., Gadola A., Lopez R. Garcia, Garczarczyk M., Giglietto N., Giordano F., Giuliani A., Glicenstein J., Gnatyk R., Goldoni P., Grabarczyk T., Graciani R., Graham J., Grandi P., Granot J., Green A. J., Griffiths S., Gunji S., Hakobyan H., Hara S., Hassan T., Hayashida M., Heller M., Helo J. C., Hinton J., Hnatyk B., Huet J., Huetten M., Humensky T. B., Hussein M., Horandel J., Ikeno Y., Inada T., Inome Y., Inoue S., Inoue T., Inoue Y., Ioka K., Iori M., Jacquemier J., Janecek P., Jankowsky D., Jung I., Kaaret P., Katagiri H., Kimeswenger S., Kimura S., Knodlseder J., Koch B., Kocot J., Kohri K., Komin N., Konno Y., Kosack K., Koyama S., Kraus M., Kubo H., Mezek G. Kukec, Kushida J., La Palombara N., Lalik K., Lamanna G., Landt H., Lapington J., Laporte P., Lee S., Lees J., Lefaucheur J., Lenain J. -P., Leto G., Lindfors E., Lohse T., Lombardi S., Longo F., Lopez M., Lucarelli F., Luque-Escamilla P. L., Lopez-Coto R., Maccarone M. C., Maier G., Malaguti G., Mandat D., Maneva G., Mangano S., Marcowith A., Marti J., Martinez M., Martinez G., Masuda S., Maurin G., Maxted N., Melioli C., Mineo T., Mirabal N., Mizuno T., Moderski R., Mohammed M., Montaruli T., Moralejo A., Mori K., Morlino G., Morselli A., Moulin E., Mukherjee R., Mundell C., Muraishi H., Murase K., Nagataki S., Nagayoshi T., Naito T., Nakajima D., Nakamori T., Nemmen R., Niemiec J., Nieto D., Nievas-Rosillo M., Nikolajuk M., Nishijima K., Noda K., Nogues L., Nosek D., Novosyadlyj B., Nozaki S., Ohira Y., Ohishi M., Ohm S., Okumura A., Ong R. A., Orito R., Orlati A., Ostrowski M., Oya I., Padovani M., Palacio J., Palatka M., Paredes J. M., Pavy S., Pe'er A., Persic M., Petrucci P., Petruk O., Pisarski A., Pohl M., Porcelli A., Prandini E., Prast J., Principe G., Prouza M., Pueschel E., Puelhofer G., Quirrenbach A., Rameez M., Reimer O., Renaud M., Ribo M., Rico J., Rizi V., Rodriguez J., Fernandez G. Rodriguez, Rodriguez Vazquez J. J., Romano P., Romeo G., Rosado J., Rousselle J., Rowell G., Rudak B., Sadeh I., Safi-Harb S., Saito T., Sakaki N., Sanchez D., Sangiorgi P., Sano H., Santander M., Sarkar S., Sawada M., Schioppa E. J., Schoorlemmer H., Schovanek P., Schussler F., Sergijenko O., Servillat M., Shalchi A., Shellard R. C., Siejkowski H., Sillanpaa A., Simone D., Sliusar V., Sol H., Stanic S., Starling R., Stawarz L., Stefanik S., Stephan M., Stolarczyk T., Szanecki M., Szepieniec T., Tagliaferri G., Tajima H., Takahashi M., Takeda J., Tanaka M., Tanaka S., Tejedor L. A., Telezhinsky I., Temnikov P., Terada Y., Tescaro D., Teshima M., Testa V., Thoudam S., Tokanai F., Torres D. F., Torresi E., Tosti G., Townsley C., Travnicek P., Trichard C., Trifoglio M., Tsujimoto S., Vagelli V., Vallania P., Valore L., van Driel W., van Eldik C., Vandenbroucke J., Vassiliev V., Vecchi M., Vercellone S., Vergani S., Vigorito C., Vorobiov S., Vrastil M., Vazquez Acosta M. L., Wagner S. J., Wagner R., Wakely S. P., Walter R., Ward J. E., Watson J. J., Weinstein A., White M., White R., Wierzcholska A., Wilcox P., Williams D. A., Wischnewski R., Wojcik P., Yamamoto T., Yamamoto H., Yamazaki R., Yanagita S., Yang L., Yoshida T., Yoshida M., Yoshiike S., Yoshikoshi T., Zacharias M., Zampieri L., Zanin R., Zavrtanik M., Zavrtanik D., Zdziarski A., Zech A., Zechlin H., Zhdanov V., Ziegler A., Zorn J.

    ASTROPHYSICAL JOURNAL   Vol. 840 ( 2 )   2017.5

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  92. The Fermi Galactic Center GeV Excess and Implications for Dark Matter Reviewed

    Fermi LAT collaboration

    Astrophysical Journal   Vol. 840 ( 1 )   2017.5

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    DOI: 10.3847/1538-4357/aa6cab

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  93. Cosmic-ray electron-positron spectrum from 7 GeV to 2 TeV with the Fermi Large Area Telescope Reviewed

    Abdollahi S., Ackermann M., Ajello M., Atwood W. B., Baldini L., Barbiellini G., Bastieri D., Bellazzini R., Bloom E. D., Bonino R., Brandt T. J., Bregeon J., Bruel P., Buehler R., Cameron R. A., Caputo R., Caragiulo M., Castro D., Cavazzuti E., Cecchi C., Chekhtman A., Ciprini S., Cohen-Tanugi J., Costanza F., Cuoco A., Cutini S., D'Ammando F., de Palma F., Desiante R., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Drell P. S., Drlica-Wagner A., Favuzzi C., Focke W. B., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Guillemot L., Guiriec S., Harding A. K., Jogler T., Johannesson G., Kamae T., Kuss M., La Mura G., Latronico L., Longo F., Loparco F., Lubrano P., Maldera S., Malyshev D., Manfreda A., Mazziotta M. N., Michelson P. F., Mirabal N., Mitthumsiri W., Mizuno T., Moiseev A. A., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Orlando E., Paneque D., Perkins J. S., Pesce-Rollins M., Piron F., Pivato G., Porter T. A., Principe G., Raino S., Rando R., Razzano M., Reimer A., Reimer O., Sgro C., Simone D., Siskind E. J., Spada F., Spandre G., Spinelli P., Tajima H., Thayer J. B., Tibaldo L., Torres D. F., Troja E., Wood M., Worley A., Zaharijas G., Zimmer S.

    PHYSICAL REVIEW D   Vol. 95 ( 8 )   2017.4

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    DOI: 10.1103/PhysRevD.95.082007

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  94. Search for Cosmic-Ray Electron and Positron Anisotropies with Seven Years of Fermi Large Area Telescope Data Reviewed

    Abdollahi S., Ackermann M., Ajello M., Albert A., Atwood W. B., Baldini L., Barbiellini G., Bellazzini R., Bissaldi E., Bloom E. D., Bonino R., Bottacini E., Brandt T. J., Bruel P., Buson S., Caragiulo M., Cavazzuti E., Chekhtman A., Ciprini S., Costanza F., Cuoco A., Cutini S., D'Ammando F., de Palma F., Desiante R., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Donaggio B., Drell P. S., Favuzzi C., Focke W. B., Fukazawa Y., Funk S., Fusco P., Gargano F., Gasparrini D., Giglietto N., Giordano F., Giroletti M., Green D., Guiriec S., Harding A. K., Jogler T., Johannesson G., Kamae T., Kuss M., Larsson S., Latronico L., Li J., Longo F., Loparco F., Lubrano P., Magill J. D., Malyshev D., Manfreda A., Mazziotta M. N., Meehan M., Michelson P. F., Mitthumsiri W., Mizuno T., Moiseev A. A., Monzani M. E., Morselli A., Negro M., Nuss E., Ohsugi T., Omodei N., Paneque D., Perkins J. S., Pesce-Rollins M., Piron F., Pivato G., Principe G., Raino S., Rando R., Razzano M., Reimer A., Reimer O., Sgro C., Simone D., Siskind E. J., Spada F., Spandre G., Spinelli P., Strong A. W., Tajima H., Thayer J. B., Torres D. F., Troja E., Vandenbroucke J., Zaharijas G., Zimmer S.

    PHYSICAL REVIEW LETTERS   Vol. 118 ( 9 )   2017.3

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    DOI: 10.1103/PhysRevLett.118.091103

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  95. Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster Reviewed

    Aharonian F. A., Akamatsu H., Akimoto F., Allen S. W., Angelini L., Arnaud K. A., Audard M., Awaki H., Axelsson M., Bamba A., Bautz M. W., Blandford R. D., Bulbul E., Brenneman L. W., Brown G. V., Cackett E. M., Chernyakova M., Chiao M. P., Coppi P., Costantini E., de Plaa J., den Herder J. -W., Done C., Dotani T., Ebisawa K., Eckart M. E., Enoto T., Ezoe Y., Fabian A. C., Ferrigno C., Foster A. R., Fujimoto R., Fukazawa Y., Furuzawa A., Galeazzi M., Gallo L. C., Gandhi P., Giustini M., Goldwurm A., Gu L., Guainazzi M., Haba Y., Hagino K., Hamaguchi K., Harrus I., Hatsukade I., Hayashi K., Hayashi T., Hayashida K., Hiraga J., Hornschemeier A. E., Hoshino A., Hughes J. P., Ichinohe Y., Iizuka R., Inoue H., Inoue S., Inoue Y., Ishibashi K., Ishida M., Ishikawa K., Ishisaki Y., Itoh M., Iwai M., Iyomoto N., Kaastra J. S., Kallman T., Kamae T., Kara E., Kataoka J., Katsuda S., Katsuta J., Kawaharada M., Kawai N., Kelley R. L., Khangulyan D., Kilbourne C. A., King A. L., Kitaguchi T., Kitamoto S., Kitayama T., Kohmura T., Kokubun M., Koyama S., Koyama K., Kretschmar P., Krimm H. A., Kubota A., Kunieda H., Laurent P., Lebrun F., Lee S. -H., Leutenegger M. A., Limousin O., Loewenstein M., Long K. S., Lumb D. H., Madejski G. M., Maeda Y., Maier D., Makishima K., Markevitch M., Matsumoto H., Matsushita K., McCammon D., McNamara B. R., Mehdipour M., Miller E. D., Miller J. M., Mineshige S., Mitsuda K., Mitsuishi I., Miyazawa T., Mizuno T., Mori H., Mori K., Moseley H., Mukai K., Murakami H., Murakami T., Mushotzky R. F., Nakagawa T., Nakajima H., Nakamori T., Nakano T., Nakashima S., Nakazawa K., Nobukawa K., Nobukawa M., Noda H., Nomachi M., O'Dell S. L., Odaka H., Ohashi T., Ohno M., Okajima T., Ota N., Ozaki M., Paerels F., Paltani S., Parmar A., Petre R., Pinto C., Pohl M., Porter F. S., Pottschmidt K., Ramsey B. D., Reynolds C. S., Russell H. R., Safi-Harb S., Saito S., Sakai K., Sameshima H., Sasaki T., Sato G., Sato K., Sato R., Sawada M., Schartel N., Serlemitsos P. J., Seta H., Shidatsu M., Simionescu A., Smith R. K., Soong Y., Stawarz L., Sugawara Y., Sugita S., Szymkowiak A. E., Tajima H., Takahashi H., Takahashi T., Takeda S., Takei Y., Tamagawa T., Tamura K., Tamura T., Tanaka T., Tanaka Yasuo, Tanaka Yasuyuki, Tashiro M., Tawara Y., Terada Y., Terashima Y., Tombesi F., Tomida H., Tsuboi Y., Tsujimoto M., Tsunemi H., Tsuru T., Uchida H., Uchiyama H., Uchiyama Y., Ueda S., Ueda Y., Ueno S., Uno S., Urry C. M., Ursino E., de Vries C. P., Watanabe S., Werner N., Wik D. R., Wilkins D. R., Williams B. J., Yamada S., Yamaguchi H., Yamaoka K., Yamasaki N. Y., Yamauchi M., Yamauchi S., Yaqoob T., Yatsu Y., Yonetoku D., Yoshida A., Zhuravleva I., Zoghbi A.

    ASTROPHYSICAL JOURNAL LETTERS   Vol. 837 ( 1 )   2017.3

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    DOI: 10.3847/2041-8213/aa61fa

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  96. Operating performance of the gamma-ray Cherenkov telescope: An end-to-end Schwarzschild-Couder telescope prototype for the Cherenkov Telescope Array Reviewed

    Dournaux J. L., De Franco A., Laporte P., White R., Greenshaw T., Sol H., Abchiche A., Allan D., Amans J. P., Armstrong T. P., Balzer A., Berge D., Boisson C., Bousquet J. J., Brown A. M., Bryan M., Buchholtz G., Chadwick P. M., Costantini H., Cotter G., Daniel M., De Frondat F., Dumas D., Ernenwein J. P., Fasola G., Funk S., Gaudemard J., Graham J. A., Gironnet J., Hervet O., Hidaka N., Hinton J. A., Huet J. M., Jegouzo I., Jogler T., Kawashima T., Kraus M., Lapington J. S., Lefaucheur J., Markoff S., Melse T., Morhrmann L., Molnyeux P., Nolan S. J., Okumura A., Parsons R. D., Ross D., Rowell G., Sato Y., Sayede F., Schmoll J., Schoorlemmer H., Servillat M., Stamatescu V., Stephan M., Stuik R., Sykes J., Tajima H., Thornhill J., Tibaldo L., Trichard C., Vinkh J., Watson J., Yamane N., Zech A., Zink A.

    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT   Vol. 845   page: 355 - 358   2017.2

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    DOI: 10.1016/j.nima.2016.05.059

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  97. Fermi-LAT Observations of High-energy Behind-the-limb Solar Flares Reviewed

    Ackermann M., Allafort A., Baldini L., Barbiellini G., Bastieri D., Bellazzini R., Bissaldi E., Bonino R., Bottacini E., Bregeon J., Bruel P., Buehler R., Cameron R. A., Caragiulo M., Caraveo P. A., Cavazzuti E., Cecchi C., Charles E., Ciprini S., Costanza F., Cutini S., D'Ammando F., de Palma F., Desiante R., Digel S. W., Di Lalla N., Di Mauro M., Di Venere L., Drell P. S., Favuzzi C., Fukazawa Y., Fusco P., Gargano F., Giglietto N., Giordano F., Giroletti M., Grenier I. A., Guillemot L., Guiriec S., Jogler T., Johannesson G., Kashapova L., Krucker S., Kuss M., La Mura G., Larsson S., Latronico L., Li J., Liu W., Longo F., Loparco F., Lubrano P., Magill J. D., Maldera S., Manfreda A., Mazziotta M. N., Mitthumsiri W., Mizuno T., Monzani M. E., Morselli A., Moskalenko I. V., Negro M., Nuss E., Ohsugi T., Omodei N., Orlando E., Pal'shin V., Paneque D., Perkins J. S., Pesce-Rollins M., Petrosian V., piron F., Principe G., Raino S., Rando R., Razzano M., Reimer O., da Costa F. Rubio, Sgro C., Simone D., Sisikind E. J., Sapada F., Spandre G., Spinelli P., Tajima H., Thayer J. B., Torres D. F., Troja E., Vianello G.

    ASTROPHYSICAL JOURNAL   Vol. 835 ( 2 )   2017.2

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    DOI: 10.3847/1538-4357/835/2/219

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  98. Searching for the Gamma-ray Sky for Counterparts to Gravitational Wave Sources: Fermi Gamma-ray Burst Monitor and Large Area Telescope Observations of LVT151012 and GW151226 Reviewed

    Fermi GBM and LAT collaborations

    Astrophysical Journal   Vol. 835 ( 1 )   2017.1

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    DOI: 10.3847/1538-4357/835/1/82

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  99. TARGET: A Digitizing And Trigger ASIC For The Cherenkov Telescope Array Reviewed International coauthorship

    Funk S., Jankowsky D., Katagiri H., Kraus M., Okumura A., Schoorlemmer H., Shigenaka A., Tajima H., Tibaldo L., Varner G., Zink A., Zorn J.

    HIGH ENERGY GAMMA-RAY ASTRONOMY   Vol. 1792   2017

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    DOI: 10.1063/1.4969033

    Web of Science

  100. Inauguration and First Light of the GCT-M Prototype for the Cherenkov Telescope Array Reviewed

    Watson J. J., De Franco A., Abchiche A., Allan D., Amans J. -P., Armstrong T. P., Balzer A., Berge D., Boisson C., Bousquet J. -J., Brown A. M., Bryan M., Buchholtz G., Chadwick P. M., Costantini H., Cotter G., Daniel M. K., De Frondat F., Dournaux J. -L., Dumas D., Ernenwein J. -P., Fasola G., Funk S., Gironnet J., Graham J. A., Greenshaw T., Hervet O., Hidaka N., Hinton J. A., Huet J. -M., Jegouzo I., Jogler T., Kraus M., Lapington J. S., Laporte P., Lefaucheur J., Markoff S., Melse T., Mohrmann L., Molyneux P., Nolan S. J., Okumura A., Osborne J. P., Parsons R. D., Rosen S., Ross D., Rowell G., Rulten C. B., Sato Y., Sayede F., Schmoll J., Schoorlemmer H., Servillat M., Sol H., Stamatescu V., Stephan M., Stuik R., Sykes J., Tajima H., Thornhill J., Tibaldo L., Trichard C., Vink J., White R., Yamane N., Zech A., Zink A., Zorn J.

    HIGH ENERGY GAMMA-RAY ASTRONOMY   Vol. 1792   2017

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1063/1.4969027

    Web of Science

  101. The Gamma-ray Cherenkov Telescope for the Cherenkov Telescope Array Reviewed

    Tibaldo L., Abchiche A., Allan D., Amans J. -P., Armstrong T. P., Balzer A., Bergey D., Boisson C., Bousquet J. -J., Brown A. M., Bryan M., Buchholtz G., Chadwick P. M., Costantini H., Cotter G., Daniels M. K., De Franco A., De Frondat F., Dournaux J. -L., Dumas D., Ernenwein J. -P., Fasola G., Funk S., Gironnet J., Graham J. A., Greenshaws T., Hervet O., Hidaka N., Hintoni J. A., Huet J. -M., Jankowsky D., Jegouzo I., Jogler T., Kraus M., Lapington J. S., Laporte P., Lefaucheur J., Markoff S., Melse T., Mohrmann L., Molyneux P., Nolan S. J., Okumura A., Osborne J. P., Parsons R. D., Rosen S., Ross D., Rowell G., Rulten C. B., Sato Y., Sayede F., Schmoll J., Schoorlemmer H., Servillat M., Sol H., Stamatescu V., Stephan M., Stuik R., Sykes J., Tajima H., Thornhill J., Trichard C., Vink J., Watson J. J., White R., Yamane N., Zech A., Zink A., Zorn J.

    HIGH ENERGY GAMMA-RAY ASTRONOMY   Vol. 1792   2017

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1063/1.4969025

    Web of Science

  102. Study of the polarimetric performance of a Si/CdTe semiconductor Compton camera for the Hitomi satellite Reviewed

    J. Katsuta et al.

      Vol. 840   page: 51-58   2016.12

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1016/j.nima.2016.09.057

  103. The quiescent intracluster medium in the core of the Perseus cluster Reviewed

    Hitomi collaboration

    Nature   Vol. 535 ( 7610 ) page: 117-121   2016.7

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1038/nature18627

  104. The First Fermi LAT Supernova Remnant Catalog Reviewed

    Fermi LAT collaboration

    The Astrophysical Journal Supplement Series   Vol. 224 ( 1 ) page: article id. 8   2016.5

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/0067-0049/224/1/8

  105. Fermi-LAT Observations of High-Energy Gamma-Ray Emission toward the Galactic Center Reviewed

    Fermi LAT collaboration

      Vol. 819 ( 1 ) page: article id. 44   2016.3

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/0004-637X/819/1/44

  106. The first demonstration of the concept of "narrow-FOV Si/CdTe semiconductor Compton camera" Reviewed

    Y. Ichinohe, et al.

    Nuclear Inst. and Methods in Physics Research, A   Vol. 806   page: 5-13   2016.1

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1016/j.nima.2015.09.081

  107. Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data Reviewed

    Fermi LAT collaboration

    Physical Review Letters   Vol. 115   page: 231301   2015.11

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    Language:English   Publishing type:Research paper (scientific journal)  

    The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on gamma-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in gamma rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass <100 GeV annihilating via quark and tau-lepton channels.

    DOI: 10.1103/PhysRevLett.115.231301

  108. First Images from the Focusing Optics X-Ray Solar Imager Reviewed

    FOXSI collaboration

    The Astrophysical Journal Letters   Vol. 793   page: L32   2014.9

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    Language:English   Publishing type:Research paper (scientific journal)  

    The Focusing Optics X-ray Solar Imager (FOXSI) sounding rocket payload flew for the first time on 2012 November 2, producing the first focused images of the Sun above 5 keV. To enable hard X-ray (HXR) imaging spectroscopy via direct focusing, FOXSI makes use of grazing-incidence replicated optics combined with fine-pitch solid-state detectors. On its first flight, FOXSI observed several targets that included active regions, the quiet Sun, and a GOES-class B2.7 microflare. This Letter provides an introduction to the FOXSI instrument and presents its first solar image. These data demonstrate the superiority in sensitivity and dynamic range that is achievable with a direct HXR imager with respect to previous, indirect imaging methods, and illustrate the technological readiness for a spaceborne mission to observe HXRs from solar flares via direct focusing optics.

    DOI: 10.1088/2041-8205/793/2/L32

  109. Introducing the CTA concept Reviewed

    CTA consortium

    Astroparticle Physics   Vol. 43   page: 3-18   2013.3

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    Language:English   Publishing type:Research paper (scientific journal)  

    The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, to span about four decades of energy, from a few tens of GeV to above 100 TeV with enhanced angular and energy resolutions over existing VHE gamma-ray observatories. An international collaboration has formed with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America. In 2010 the CTA Consortium completed a Design Study and started a three-year Preparatory Phase which leads to production readiness of CTA in 2014. In this paper we introduce the science goals and the concept of CTA, and provide an overview of the project.

    DOI: 10.1016/j.astropartphys.2013.01.007

  110. Detection of the Characteristic Pion-Decay Signature in Supernova Remnants Reviewed

    Fermi LAT collaboration

    Science   Vol. 339   page: 807-811   2013.2

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    Language:English   Publishing type:Research paper (scientific journal)  

    Cosmic rays are particles (mostly protons) accelerated to relativistic speeds. Despite wide agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays, unequivocal evidence for the acceleration of protons in these objects is still lacking. When accelerated protons encounter interstellar material, they produce neutral pions, which in turn decay into gamma rays. This offers a compelling way to detect the acceleration sites of protons. The identification of pion-decay gamma rays has been difficult because high-energy electrons also produce gamma rays via bremsstrahlung and inverse Compton scattering. We detected the characteristic pion-decay feature in the gamma-ray spectra of two SNRs, IC 443 and W44, with the Fermi Large Area Telescope. This detection provides direct evidence that cosmic-ray protons are accelerated in SNRs.

    DOI: 10.1126/science.1231160

  111. TARGET: A multi-channel digitizer chip for very-high-energy gamma-ray telescopes Reviewed

    Bechtol, K.; Funk, S.; Okumura, A.; Ruckman, L. L.; Simons, A.; Tajima, H.; Vandenbroucke, J.; Varner, G. S.

    Astroparticle Physics   Vol. 36   page: 156-165   2012.8

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    Language:English   Publishing type:Research paper (scientific journal)  

    The next-generation very-high-energy (VHE) gamma-ray observatory, the Cherenkov Telescope Array, will feature dozens of imaging atmospheric Cherenkov telescopes (IACTs), each with thousands of pixels of photo-sensors. To be affordable and reliable, reading out such an array of up to a million channels requires event recording technology that is highly integrated and modular, with a low cost per channel. We present the design and performance of a chip targeted to this application: the TeV Array Readout with GSa/s sampling and Event Trigger (TARGET). This application-specific integrated circuit (ASIC) has 16 parallel input channels, a 4096-sample buffer for each channel, adjustable input termination, self-trigger functionality, and tight window-selected readout. We report the performance of the first-generation version of this chip (TARGET 1) in terms of sampling frequency, power consumption, dynamic range, current-mode gain, analog bandwidth, and cross talk. The large number of channels per chip allows a low cost per channel (10 to 20 including front-end and back-end electronics but not including photosensors) to be achieved with a TARGET-based IACT readout system. In addition to basic performance parameters of the TARGET 1 chip, we present a camera module prototype as well as a second-generation chip (TARGET 2), both of which have now been produced.

    DOI: 10.1016/j.astropartphys.2012.05.016

  112. Fermi Large Area Telescope Discovery of GeV Gamma-Ray Emission from the Vicinity of SNR W44 Reviewed

    Uchiyama, Yasunobu; Funk, Stefan; Katagiri, Hideaki; Katsuta, Junichiro; Lemoine-Goumard, Marianne; Tajima, Hiroyasu; Tanaka, Takaaki; Torres, Diego F.

    The Astrophysical Journal Letters   Vol. 749   page: L35   2012.4

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    Language:English   Publishing type:Research paper (scientific journal)  

    We report the detection of GeV gamma-ray emission from the molecular cloud complex that surrounds the supernova remnant (SNR) W44 using the Large Area Telescope on board Fermi. While the previously reported gamma-ray emission from SNR W44 is likely to arise from the dense radio-emitting filaments within the remnant, the gamma-ray emission that appears to come from the surrounding molecular cloud complex can be ascribed to the cosmic rays (CRs) that have escaped from W44. The non-detection of synchrotron radio emission associated with the molecular cloud complex suggests the decay of pi0 mesons produced in hadronic collisions as the gamma-ray emission mechanism. The total kinetic energy channeled into the escaping CRs is estimated to be Wesc ~ (0.3-3) x 10^50 erg, in broad agreement with the conjecture that SNRs are the main sources of Galactic CRs.

    DOI: 10.1088/2041-8205/749/2/L35

  113. Gamma-Ray Observations of the Supernova Remnant RX J0852.0-4622 with the Fermi Large Area Telescope Reviewed

    Tanaka, T.; Allafort, A.; Ballet, J.; Funk, S.; Giordano, F.; Hewitt, J.; Lemoine-Goumard, M.; Tajima, H.; Tibolla, O.; Uchiyama, Y.

    The Astrophysical Journal Letters   Vol. 740   page: L51   2011.10

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    Language:English   Publishing type:Research paper (scientific journal)  

    We report on gamma-ray observations of the supernova remnant (SNR) RX J0852.0-4622 with the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope. In the Fermi-LAT data, we find a spatially extended source at the location of the SNR. The extension is consistent with the SNR size seen in other wavelengths such as X-rays and TeV gamma rays, leading to the identification of the gamma-ray source with the SNR. The spectrum is well described as a power law with a photon index of 1.85±0.06 (stat)+0.18-0.19 (sys), which smoothly connects to the H.E.S.S. spectrum in the TeV energy band. We discuss the gamma-ray emission mechanism based on multiwavelength data. The broadband data can be fit well by a model in which the gamma rays are of hadronic origin. We also consider a scenario with inverse Compton scattering of electrons as the emission mechanism of the gamma rays. Although the leptonic model predicts a harder spectrum in the Fermi-LAT energy range, the model can fit the data considering the statistical and systematic errors.

    DOI: 10.1088/2041-8205/740/2/L51

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Presentations 17

  1. Suppressing Optical Cross Talk in Silicon Photomultipliers International conference

    H. Tajima, A. Okumura, N. Hidaka, Y. Nakamura, N. Yamane, A. Zenin

    International Conference on the Advancement of Silicon Photomultipliers 

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    Event date: 2018.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Schwetzingen, Germany   Country:Germany  

    Compared to conventional photomultiplier tubes (PMTs), silicon photomultipliers (SiPMs) based on multi-cell geiger-mode avalanche photodiodes (GAPDs) have advantages with regards to photon detection efficiency, compactness, robustness and tolerance of both magnetic fields and intense light sources. In addition, SiPMs can be cost effective for applications that require many channels with small unit area. Because of these advantages, SiPMs are starting to replace PMs in many applications.
    When used in the cameras of Imaging Atmospheric Cherenkov telescopes, the optical crosstalk of SiPMs needs to be reduced in order to suppress accidental triggers due to the high rate of night sky background caused by scattered starlight and moonlight, and the fluorescence of excited molecules in the atmosphere.
    In this contribution, the propagation properties of optical photons in SiPMs are investigated through systematic measurements of the optical crosstalk with varying SiPM pixel and GAPD cell sizes and with and without coatings on the SiPMs. It was observed that a significant portion of the optical crosstalk is mediated by the coating. The propagation of optical photons in the bulk silicon of the SiPM is also discussed.

  2. Indirect searches for dark matter with gamma rays and other messengers Invited

    Hiroyasu Tajima

    The first KMI School 

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    Event date: 2018.2 - 2018.3

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University   Country:Japan  

  3. Evaluation of Silicon Photomultipliers for Dual-Mirror Small-Sized Telescopes of CTA International conference

    Hiro Tajima for CTA ASTRI and GCT projects

    8th International Conference on New Development in Photodetection 

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    Event date: 2017.7

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Tours, France   Country:France  

    All camera designs for Small-Sized telescopes (SSTs) proposed for the Cherenkov Telescope Array (CTA) utilise silicon photomultipliers (SiPM) as their baseline photon sensor technology. The dual-mirror SST (SST-2M) has a smaller plate scale (i.e. image size) than the single-mirror SST, allowing it to employ 2,000 square SiPMs with pixel sizes of approximately 6 mm, close to the mainstream SiPM sizes.
    In CTA, the night sky background level of typically ~25 Mcount/s/pixel (> 100 Mcounts/s/pixel at maximum) places severe constraints on the trigger capability due to accidental coincidence on neighbouring pixels. In order to suppress such events, it is necessary to reduce optical crosstalk, a mechanism whereby a single optical photon can produce multiple avalanches in the SiPM, while keeping good photon detection efficiency. These are, in general, contradicting requirements.
    In this talk, we report on characterisation of a variety of SiPM technologies for SST-2M cameras and compare results obtained at different participating institutions. We assess the harmonisation of results and discuss the likely performance that will be achieved for the first production cameras.

  4. Search for PeVatrons with Imaging Cherenkov Telescopes Invited

    田島宏康

    CRC将来計画タウンミーティング 

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    Event date: 2017.3

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:東京大学   Country:Japan  

  5. Indirect Searches for WIMP Dark Matter Invited

    Hiroyasu Tajima

    Physics in LHC and the Early Universe 

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    Event date: 2017.1

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:University of Tokyo   Country:Japan  

    Indirect dark matter search by gamma-ray and cosmic anti-particle observations are reviewed.

  6. Quest for the Origin of Cosmic Rays with Gamma-Ray Observations Invited

    Hiroyasu Tajima

    The 3rd International Symposium on "Quest for the Origin of Particles and the Universe" 

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    Event date: 2017.1

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Nagoya University   Country:Japan  

    Cosmic rays are among long standing mysteries of the Universe since the origin and the acceleration mechanism of cosmic rays are not known well. Gamma-ray observations are expected to play a prominent role in probing into those questions since gamma rays are produced by interaction of cosmic rays. In fact, the Fermi Gamma-ray Space Telescope found the first undeniable evidence of cosmic ray acceleration in supernova remnants (SNRs) in 2013. However, it is not yet conclusive whether the SNRs is the sole origin of Galactic cosmic rays and we also have no credible clues on the extragalactic origins. In this talk, recent progresses and future prospects on uncovering the origins of Galactic and extragalatic cosmic rays are reviewed.

  7. Tracking with Fermi LAT International conference

    Hiroyasu Tajima

    23rd International Workshop on Vertex Detectors 

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    Event date: 2014.9

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:Czech Republic  

  8. Quest for Dark Matter with Cosmic Gamma-ray Observations International conference

    Hiroyasu Tajima

    KMI International Symposium 2013 on Quest for the Origin of Particles and the Universe" 

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    Event date: 2013.12

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:Japan  

  9. Particle Physics and Astrophysics by Cosmic Gamma-ray Observations International conference

    Hiroyasu Tajima

    KMI Inauguration Conference on "Quest for the Origin of Particles and the Universe" 

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    Event date: 2011.10

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:Japan  

  10. Soft gamma-ray detector for the ASTRO-H Mission International conference

    ASTRO-H SGD team

    SPIE Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray 

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    Event date: 2010.6 - 2010.7

    Language:English   Presentation type:Oral presentation (general)  

    Country:United States  

    ASTRO-H is the next generation JAXA X-ray satellite, intended to carry instruments with broad energy coverage and exquisite energy resolution. The Soft Gamma-ray Detector (SGD) is one of ASTRO-H instruments and will feature wide energy band (40-600 keV) at a background level 10 times better than the current instruments on orbit. SGD is complimentary to ASTRO-H's Hard X-ray Imager covering the energy range of 5-80 keV. The SGD achieves low background by combining a Compton camera scheme with a narrow field-of-view active shield where Compton kinematics is utilized to reject backgrounds. The Compton camera in the SGD is realized as a hybrid semiconductor detector system which consists of silicon and CdTe (cadmium telluride) sensors. Good energy resolution is afforded by semiconductor sensors, and it results in good background rejection capability due to better constraints on Compton kinematics. Utilization of Compton kinematics also makes the SGD sensitive to the gamma-ray polarization, opening up a new window to study properties of gamma-ray emission processes. The ASTRO-H mission is approved by ISAS/JAXA to proceed to a detailed design phase with an expected launch in 2014. In this paper, we present science drivers and concept of the SGD instrument followed by detailed description of the instrument and expected performance.

  11. Fermi Observations of High-energy Emission from Gamma-Ray Bursts International conference

    Hiroyasu Tajima

    TeV Particle Astrophysics 2009 

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    Event date: 2009.7

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:United States  

  12. Polarimetry with ASTRO-H Soft Gamma-ray Detector International conference

    Hiroyasu Tajima

    The coming of age of X-ray polarimetry 

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    Event date: 2009.4

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:Italy  

    ASTRO-H is a next generation JAXA X-ray satellite to be launched in 2014. Soft Gamma-ray Detector (SGD) onboard ASTRO-H is a semiconductor Compton camera with a narrow field-of-view (FOV) to achieve very low background. Although the SGD is primarily a spectrometer in the 40-600 keV energy band, it is also sensitive to polarization in the 50-200 keV energy band. This paper describes instrument design, expected performance, and experimental validation of polarimetric performance of the SGD.

  13. Compton Camera for Space and Security Applications International conference

    Hiroyasu Tajima

    IEEE Nuclear Science Symposium, Compton Camera Workshop 

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    Event date: 2008.10

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:Germany  

  14. Detectors for Cosmic Rays on Ground and in Space International conference

    Hiroyasu Tajima

    11th Vienna Conference on Instrumentation 

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    Event date: 2007.2

    Language:English   Presentation type:Oral presentation (invited, special)  

    Country:Austria  

    The origin of the cosmic rays has been a great mystery since it was discovered by Victor Hess in 1912.
    AGASA observation of ultra-high-energy cosmic-rays (UHECR) possibly beyond GZK (Greisen, Zatsepin and Kuzmin) cutoff stimulated the field in great deal.
    In addition, Kamiokande detection of neutrinos from SN1987A and H.E.S.S. detection of TeV gamma-rays from supernova remnants demonstrated viability of neutrino and TeV gamma-ray astronomy for cosmic-ray research.
    New generation of currently-operating or soon-to-be-operating detectors for charged particles, gamma-rays and neutrinos from cosmos will get us even closer to understanding the nature and origin of cosmic-rays.
    Detectors for UHECRs, gamma-rays and neutrinos are of particular importance in order to study the origins of cosmic-rays since these particles are free from the deflection due to magnetic fields.
    Detectors for antiparticles and gamma-rays would be useful to detect cosmic-rays originated from the decay of the dark matter in the Universe.
    I will review these cosmic-ray detectors with particular attention on the differences of ground-based, balloon-borne and satellite-borne detectors.

  15. Suppressing Optical Cross Talk in Silicon Photomultipliers

    H. Tajima, A. Okumura, N. Hidaka, Y. Nakamura, N. Yamane, A. Zenin

    International Conference on the Advancement of Silicon Photomultipliers  2018.6.11 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:Schwetzingen, Germany  

    Compared to conventional photomultiplier tubes (PMTs), silicon photomultipliers (SiPMs) based on multi-cell geiger-mode avalanche photodiodes (GAPDs) have advantages with regards to photon detection efficiency, compactness, robustness and tolerance of both magnetic fields and intense light sources. In addition, SiPMs can be cost effective for applications that require many channels with small unit area. Because of these advantages, SiPMs are starting to replace PMs in many applications.
    When used in the cameras of Imaging Atmospheric Cherenkov telescopes, the optical crosstalk of SiPMs needs to be reduced in order to suppress accidental triggers due to the high rate of night sky background caused by scattered starlight and moonlight, and the fluorescence of excited molecules in the atmosphere.
    In this contribution, the propagation properties of optical photons in SiPMs are investigated through systematic measurements of the optical crosstalk with varying SiPM pixel and GAPD cell sizes and with and without coatings on the SiPMs. It was observed that a significant portion of the optical crosstalk is mediated by the coating. The propagation of optical photons in the bulk silicon of the SiPM is also discussed.

  16. Indirect Searches for WIMP Dark Matter Invited International conference

    Hiroyasu Tajima

    Physics in LHC and the Early Universe  2017.1.9  Grant-in-Aid for Scientific Research on Innovative Areas "New expansion of particle physics of post-Higgs era by LHC revealing the vacuum and space-time structure"

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    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:University of Tokyo  

    Indirect dark matter search by gamma-ray and cosmic anti-particle observations are reviewed.

  17. Indirect searches for dark matter with gamma rays and other messengers Invited International conference

    Hiroyasu Tajima

    The first KMI School  2018.2.28 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University  

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Research Project for Joint Research, Competitive Funding, etc. 2

  1. Development of photon sensors for Cherenkov Telescope Array

    2015.10

    Cooperative Research within an Affiliated University or Institute 

  2. 革新的超広角高感度ガンマ線可視化装置の開発

    2012.5 - 2015.3

    研究成果展開事業 (先端計測分析技術・機器開発プログラム) 

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    Grant type:Competitive

KAKENHI (Grants-in-Aid for Scientific Research) 3

  1. Search for Dark Matter in Galactic Center with Cosmic Gamma-ray Observations

    Grant number:15H02086  2015.4 - 2019.3

    Tajima Hiroyasu

      More details

    Authorship:Principal investigator  Grant type:Competitive

    Grant amount:\39910000 ( Direct Cost: \30700000 、 Indirect Cost:\9210000 )

    Galactic diffuse gamma rays are the main background for the dark matter searches near the Galactic center. We have improved uncertainties of the galactic diffuse background by verifying the modeling the interstellar medium using dust radiance, opacity and temperature data and identifying several undetected gamma-ray objects by our image restoration software. In parallel, we have improved the crosstalk problem of the novel photon sensor for the next generation gamma-ray instrument, CTA. We found further improvement may be possible by reducing delayed crosstalk. We also successfully developed integrated circuits to provers signals from dense photon sensor and verified the performance by test observations using prototype telescope.

  2. Exploration of Energy Frontier in Cosmic Gamma-ray Observations

    Grant number:21H04468  2021.4 - 2026.3

    Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (A)

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    Authorship:Principal investigator  Grant type:Competitive

    Grant amount:\41340000 ( Direct Cost: \31800000 、 Indirect Cost:\9540000 )

  3. 大面積・半導体チェレンコフ・カメラの開発研究とその実証

    2011.4 - 2015.3

    科学研究費補助金  基盤研究(A)

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    Authorship:Principal investigator 

    本質的に量子効率の高い半導体光電子増倍素子を高密度に配列した開口率が高く大面積のモジュールを組み立てる技術を開発し、高密度読み出しを可能とする高速波形記録集積回路を組み合わせた大面積・半導体チェレンコフ・カメラを実用化する。

 

Social Contribution 29

  1. S-NETセミナー2021 in 愛知

    Role(s):Lecturer

    日本宇宙フォーラム  ~躍進する宇宙ビジネス産業の最前線~  2021.2

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    Audience: General

    Type:Seminar, workshop

  2. 東北大・宇宙航空研究連携拠点 第二回シンポジウム

    Role(s):Lecturer

    東北大学  〜大学ベースの宇宙航空研究教育:その現在と方向〜  2020.12

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    Audience: College students, Graduate students, Teachers, Researchesrs

    Type:Seminar, workshop

  3. 愛知県主催宇宙産業講演会

    Role(s):Lecturer

    愛知県 産業労働部 産業振興課  宇宙ビジネス促進セミナー  愛知県産業労働センター(ウインクあいち)  2019.2

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    Audience: Researchesrs, General, Company, Governmental agency, Media

    Type:Seminar, workshop

    愛知県 産業労働部 産業振興課が主催した宇宙ビジネス促進セミナーにおいて、超小型衛星による宇宙の民間利用について、名古屋大学における取り組みを紹介した。

  4. 第27回公開セミナー「天文学の最前線」

    Role(s):Lecturer

    名古屋大学理学研究科、名古屋市科学館  第27回公開セミナー「天文学の最前線」  2018.8

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    Audience: High school students, College students, Graduate students, General

    Type:Lecture

    「宇宙ガンマ線観測で解き明かす暗黒物質の正体」に関する講演をした。

  5. 図書館サイエンス夜話~シリーズ宇宙~

    Role(s):Lecturer

    鶴舞図書館・名古屋大学  超小型衛星で切り開く宇宙フロンティア  鶴舞図書館  2017.10

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    Audience: General

  6. 日米宇宙フォーラム

    Role(s):Lecturer, Organizing member

    モーリーン・アンド・マイク・マンスフィールド財団  「日米宇宙フォーラム」~安倍-トランプ時代の日米宇宙協力~  名古屋大学  2017.3

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    Audience: General, Company

    Type:Lecture

  7. 半田高校サイエンスコミュニケーション

    Role(s):Lecturer

    半田高校  半田高校サイエンスコミュニケーション  2016.6

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    Audience: High school students, General

    Type:Lecture

    「放射能除染に活かされる宇宙放射線観測技術」というタイトルで講演

  8. 系統別ガイダンス

    Role(s):Lecturer

    大学新聞社 名古屋支局  系統別ガイダンス  岐阜県立岐阜北高校  2016.6

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    Audience: High school students

    Type:Visiting lecture

    名古屋大学理学部の紹介および宇宙観測・実験分野の研究について出前授業を実施した。

  9. 社会人サポーター講演会

    2015.12

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    名古屋西高校において宇宙観測・実験分野の研究と社会貢献について講演した。

  10. 大学系統別出張講座

    2015.10

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    岐阜県立岐阜北高校にて、研究対象となる宇宙物理現象や、それを観測するための機器の名古屋大学における開発、その開発によって得られた技術を社会の発展に応用している事例を紹介した。

  11. 「関戸弥太郎と宇宙線望遠鏡」展・特別講演会

    2015.8

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    「チェレンコフ望遠鏡で探る宇宙線のふるさと」という題目で講演した。

  12. 笠松町歴史未来館開館記念講演会

    2015.6

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    「超小型衛星で広がる宇宙利用」という題目で講演した。

  13. 半田高校 SSHサイエンスコミュニケーション

    2014.12

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    「放射能除染に活かされる宇宙観測技術」というタイトルで講演

  14. 羽島郡立志塾

    2014.10

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    超小型衛星で夢を拓く

  15. 「宇宙科学の最前線:天体観測衛星がひらく未知の宇宙」

    2014.6

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    フェルミ衛星とAstro-H計画で迫る高エネルギー天体の謎

  16. 大空や宇宙へ羽ばたく夢の扉

    2013.10

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    中部発の人工衛星“金シャチ1号”

  17. 2013名古屋大学公開講座

    2013.10

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    放射能除染に活かされる宇宙放射線観測技術

  18. 先端イノベーション研修

    2013.9

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    先端技術で解き明かす高エネルギー宇宙

  19. 第22回公開セミナー「天文学の最前線」

    2013.8

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    ガンマ線で探る高エネルギーの宇宙

  20. 宇宙技術講演会・航空宇宙フェア特別講演会

    2013.6

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    名古屋市科学館で開催された宇宙技術講演会・航空宇宙フェア特別講演会において、「中部地区発人工衛星、ChubuSat-1の開発と将来の展望」と題する講演を行った。

  21. 時習館高校理科講演会

    2013.2

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    「中部発の人工衛星への挑戦」と題した講演を行った。

  22. 中部航空宇宙技術センター主催「超小型衛星が拓くニュービジネスセミナー」

    2013.1

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    中部航空宇宙技術センターが主催した「超小型衛星が拓くニュービジネスセミナー」で「中部発超小型衛星ChubuSat-1(金シャチ1号)の開発と将来のニュービジネスの可能性」と題する講演を行った。

  23. 2012年国際航空宇宙展

    2012.10

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    2012年国際航空宇宙展においてChubuSat-1のレプリカを展示した。

  24. 名大カフェ“Science, and Me”

    2012.10

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    名大カフェ“Science, and Me”第27回において「中部発人工衛星”金シャチ1
    号”の挑戦」と題する講演を行った。

  25. NPO法人「子供達と最先端科学技術の架け橋」主催「子どもの世界に先端技術を!」講演会

    2012.10

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    NPO法人「子供達と最先端科学技術の架け橋」主催の「子どもの世界に先端技術を!」講演会において「金シャチ1号にかける夢」に関して講演した。また、その後霧箱を用いた宇宙線の観測実験を実施した。

  26. 東海高校・中学校第20回サタデープログラム

    2012.2

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    東海高校・中学校第20回サタデープログラムにおいて「中部地方発50kg級小型人工衛星による科学観測への挑戦」に関する講演をした。

  27. 中部航空宇宙技術センター主催「超小型衛星利用に関するセミナー」

    2012.1

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    中部航空宇宙技術センター主催「超小型衛星利用に関するセミナー」において「航空宇宙産業の拠点である中部地区の衛星分野への取組み」に関する講演をした。

  28. NHK文化センター 23年度宇宙講座

    2011.9

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    NHK文化センター 23年度宇宙講座「先端宇宙2011」~最新研究で宇宙解明~ にて「高エネルギーの宇宙」に関する講演をした。

  29. クリスマスレクチャーズ2010

    2010.12

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    昭和女子大学オーロラホールで名大南半球宇宙観測研究センターが主催したクリスマスレクチャーズ2010において「ガンマ線でみた超新星爆発」に関する一般向け講演をした。

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