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REVIEW 8 minor 97 references

Hard X-ray and gamma-ray detectors

T0 review · 0 major / 8 minor · reviewed 2026-08-12 · deepseek-v4-flash

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Pith's one-line read The chapter organizes hard X-ray and gamma-ray astronomy around one principle: photon energy decides which interaction with matter dominates, and that decides the telescope design.

desk verdict A competent, clearly written review chapter that breaks no new ground but is a sound reference for students and mission planners; worth refereeing as a handbook chapter, not as a research paper. read the letter →

arxiv 2411.11987 v1 pith:JM7X3KQ7 submitted 2024-11-18 astro-ph.IM astro-ph.HE

Vincent Tatischeff , Philippe Laurent This is my paper · ORCID
classification astro-ph.IMastro-ph.HE
keywords X-rayastronomyGamma-rayCodedmaskComptontelescopePaircreationtelescopesSolid-statedetectorsScintillatorsGas
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The chapter organizes the field of space-based hard X-ray and gamma-ray astronomy around a single physical principle: the photon energy decides which interaction with matter dominates, and that decision dictates the telescope architecture. Photoelectric absorption rules the hard X-ray band, Compton scattering dominates near 1 MeV, and electron-positron pair production takes over above about 10 MeV. Each regime maps onto a distinct instrument family, from focusing optics and coded masks through Compton telescopes to pair-production trackers with calorimeters. If this classification is right, it explains the design of every major mission from NuSTAR to Fermi/LAT and points to where the unresolved 'MeV gap' comes from.

What carries the argument

The load-bearing object is the set of mass attenuation coefficients for photoelectric absorption, Compton scattering, and pair production as functions of photon energy and atomic number, shown in Figure 1 for Si, Ge, and Xe. These curves define the crossover energies where one process outcompetes the others, and those crossovers determine the detector material and telescope geometry: thin pixelated semiconductors for photoelectric-dominated focusing and coded-mask instruments, low-atomic-number scatterers paired with high-atomic-number calorimeters for Compton telescopes, and converter/tracker/calorimeter stacks for pair-production telescopes. The mechanism is that the dominant interaction process sets what quantity the instrument must measure—energy deposition position, scattered-photon direction, or electron-positron tracks—and therefore which detector technology is viable.

What would settle it

Measure the mass attenuation coefficients of a representative detector material such as CdTe or GAGG(Ce) from 10 keV to 100 MeV and compare them with the tabulated values used in the chapter; a deviation large enough to shift the photoelectric-to-Compton or Compton-to-pair boundary by a factor of two would invalidate the classification. Alternatively, a space telescope that achieves high sensitivity in the 200 keV to 50 MeV band using an architecture the chapter assigns to a different energy regime would falsify the mapping.

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Extended reading notes

Core claim

The central claim, stated in the chapter's own words, is that the operating principle of hard X-ray and gamma-ray detectors depends above all on the energy of the photons to be detected, through the three main processes by which photons above 10 keV interact with matter. Using mass attenuation coefficients for silicon, germanium, and xenon, the authors show that photoelectric absorption is the main process up to about 57 keV in Si, 150 keV in Ge, and 300 keV in Xe, while pair production overtakes Compton scattering above roughly 15 MeV, 9 MeV, and 6 MeV respectively. They then survey the detector families—semiconductor imagers, scintillators, and gas or liquid detectors—and map them onto the telescope types assigned to these energy bands. The review's demonstration is that a single energy-domain classification coherently accounts for the past, present, and proposed space telescopes across seven orders of magnitude in photon energy.

Load-bearing premise

The classification assumes the tabulated photon cross-section data used in Figure 1 are accurate for silicon, germanium, and xenon and remain representative when applied to other detector materials such as CdTe and scintillators; if those attenuation coefficients were materially wrong, the energy boundaries that assign telescope types would mislead.

Editorial extensions

If this is right

  • A designer can pick detector material and thickness directly from the crossover energies for that material's atomic number.
  • The persistent 'MeV gap' between roughly 200 keV and 50 MeV is a direct consequence of the classification, since neither photoelectric-focused optics nor pair trackers work well in that band.
  • Modern Compton-telescope proposals such as COSI can use one detector type for both scattering and absorption because the Compton regime permits it.
  • The review implies that the path to better MeV sensitivity is improved angular resolution and background rejection within each regime, not a single detector that works at all energies.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The classification could be used predictively: novel high-atomic-number materials might push photoelectric-dominated focusing to higher energies than current CdTe/CZT systems, a direction the chapter does not explore.
  • A quantitative comparison of effective area and sensitivity as a function of energy across past and proposed missions would test the reality of the 'MeV gap' more rigorously than the chapter's qualitative discussion.
  • The three-regime scheme might transfer to detector design outside astronomy, such as Compton cameras for medical imaging or nuclear security, where the same interaction physics governs performance.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

0 major / 8 minor

Summary. This review chapter, intended for a handbook on X-ray and gamma-ray astrophysics, surveys detector technologies for space-based hard X-ray and gamma-ray astronomy. It is organized around the energy-dependent dominance of the three principal photon interaction processes—photoelectric absorption, Compton scattering, and pair production—and uses this scheme to classify telescope concepts (focusing optics, coded-mask, Compton, pair-production) and to motivate the choice of detector materials and geometries. The chapter reviews semiconductor detectors (Si, Ge, CdTe/CZT), scintillators (inorganic, organic), gas and liquid detectors (proportional counters, time projection chambers), photodetectors, readout electronics, in-orbit backgrounds, and simulation tools, closing with an outlook on future missions and technologies.

Significance. The chapter provides a comprehensive and accurate overview of the field, grounded in the standard NIST XCOM cross-section data for Si, Ge, and Xe, and it correctly maps these physics foundations to the design of past, current, and proposed missions (NuSTAR, INTEGRAL, Fermi/LAT, COSI, e-ASTROGAM, AMEGO-X, etc.). Its strength is its clear pedagogical organization: the energy-based classification is a well-established organizing principle, and the specific threshold values quoted (e.g., photoelectric/Compton equality at 57 keV in Si, 150 keV in Ge, 300 keV in Xe; Compton/pair equality at 15, 9, and 6 MeV, respectively) are quantitatively consistent with authoritative cross-section data. As a literature review, it makes no new empirical claims and fits no parameters; the authors' self-citations to their own mission-concept papers are used descriptively and are appropriate. The chapter is a reliable reference for newcomers and a useful synthesis for practitioners, though it contains a number of typographical and terminological errors that should be corrected.

minor comments (8)
  1. [Detectors for Compton telescopes] The phrase 'Using quantum optics in a Compton telescope' is a misnomer: the imaging technique relies on Compton scattering kinematics and coincidence measurement, not on quantum optics. Please replace with 'Compton imaging' or 'Compton kinematics'.
  2. [Silicon detectors] In the paragraph on charge-coupled devices, 'CDDs' is a typo for 'CCDs' (e.g., 'the readout time of CDDs is necessarily long').
  3. [Principle of detection / Pixelated detectors] The term 'solid-sate' appears twice (e.g., 'Finely-pixelated solid-sate detectors') and should be 'solid-state'.
  4. [CdTe and Cd(Zn)Te detectors] The spelling 'Shottky' is used inconsistently with 'Schottky' elsewhere in the chapter; the correct spelling is 'Schottky'.
  5. [Germanium detectors] The sentence 'Germanium detectors excellent energy resolution degrade when the detectors are exposed to particles irradiation' is grammatically garbled; it should read 'Germanium detectors' excellent energy resolution degrades when the detectors are exposed to particle irradiation.'
  6. [Scintillation detectors] There is a grammar error: 'Scintillators can been manufactured' should be 'Scintillators can be manufactured'.
  7. [Gas and liquid detectors] The phrase 'as one increase the bias' should be 'as one increases the bias'.
  8. [References] The editor's name 'Sangangelo' is misspelled; it should be 'Santangelo' (e.g., 'Bambi and Sangangelo, 2022' in the Introduction and the reference entries for Bambi and Sangangelo).

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the chapter is a descriptive review with no fitted parameters, derivations, or self-citation used to close an argument.

full rationale

This manuscript is a review chapter on hard X-ray and gamma-ray detectors. It presents a standard energy-based classification of interaction processes (photoelectric, Compton, pair production) with mass attenuation coefficients taken from the NIST XCOM database, and then describes detector technologies, missions, and proposals. There is no derivation chain in which a claim is reduced to its own input: the chapter fits no parameters, predicts no new observable, and invokes no uniqueness theorem. The authors cite their own prior work (e.g., Tatischeff et al. 2016 for e-ASTROGAM, Cumani et al. 2019 for background simulations, Tatischeff et al. 2022 for orbits) but these citations are used descriptively as examples of proposed instruments or supporting background calculations, not as load-bearing evidence to forbid alternatives or to define the classification. The central organizing principle—that the dominant photon interaction depends on photon energy and material—is independently supported by tabulated cross-section data and by the external, machine-independent success of the cited missions (Fermi/LAT, INTEGRAL, NuSTAR). Even the numerical thresholds (e.g., photoelectric/Compton equality at 57 keV in Si, 150 keV in Ge, 300 keV in Xe) are simply read from standard XCOM data, not derived from the chapter's own conclusions. No step in the text reduces by construction to its own assumption. Accordingly, no circularity is present, and the appropriate score is 0.

Assumptions & free parameters 0 free parameters · 4 assumptions · 0 invented entities

The central claim is a review summary; it rests on standard physics and on the accuracy of the cited sources, rather than on new free parameters, invented entities, or novel derivations.

assumptions (4)
  • domain assumption The mass attenuation coefficients for photoelectric absorption, Compton scattering, and pair production in Si, Ge, and Xe, as sourced from the NIST XCOM database, are accurate and representative for the chapter's energy-domain classification.
    Invoked in the 'Principle of detection' section and Figure 1 to set the energy ranges at which different telescope types apply.
  • domain assumption The detector performance numbers in Tables 1-3 and in the text (e.g., light yields, decay times, FWHM at 662 keV) are correctly transcribed from the cited references.
    Tables 2 and 3 cite the LBNL scintillator library and Knoll (2010); the review's reliability as a reference depends on these transcriptions.
  • standard math The Shockley-Ramo theorem correctly predicts the signal induced by moving charge carriers in biased semiconductor detectors.
    Used in the 'Semiconductor detectors' section to explain electrode charge induction; treated as textbook background.
  • domain assumption The stated mission statuses and launch dates (e.g., COSI planned for launch in 2027, SVOM launched in June 2024) were correct at the time of submission.
    Sections on Compton telescopes, CdTe detectors, and the outlook report mission timelines that can become outdated.

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Cite this review

Pith. "Pith review of Hard X-ray and gamma-ray detectors." pith.science (2026). https://pith.science/paper/JM7X3KQ7

@misc{pith2026241111987,
  author       = {Pith},
  title        = {Pith review of: Hard X-ray and gamma-ray detectors},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/JM7X3KQ7}},
  note         = {Machine review of arXiv:2411.11987}
}
read the original abstract

Space-based astronomy of hard X-rays and gamma rays covers more than seven orders of magnitude in photon energy, from 10 keV to several hundred GeV. Detecting cosmic photons in this energy range is a challenge, due to the relatively low probability of interaction of high-energy photons with matter and the high background noise generated in space detectors by environmental charged particles and radiation. However, the development of new detection technologies is constantly improving the performance of space-based X- and gamma-ray telescopes. This chapter presents the different detectors used in this field of astronomy, their configuration within space telescopes and some proposals for new instruments.

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Works this paper leans on

97 extracted references · 41 canonical work pages

  1. [1]

    260(2):53, doi:10.3847/1538-4365/ac6751, 2201.11184

    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-Bl \'a zquez J, Crnogorcevic M, Cutini S, D'Ammando F, De Gaetan...

    arXiv 2022

  2. [2]

    928(2):141, doi:10.3847/1538-4357/ac5626

    Aboudan A, Bulgarelli A, Fioretti V, Giuliani A, Tavani M, Debei S (2022) A Multimission Method for the Reconstruction of Gamma-ray Events on Silicon Tracker Pair Telescopes . 928(2):141, doi:10.3847/1538-4357/ac5626

    work page doi:10.3847/1538-4357/ac5626 2022

  3. [3]

    Nuclear Instruments and Methods in Physics Research A 835:186--225, doi:10.1016/j.nima.2016.06.125

    Allison J, Amako K, Apostolakis J, Arce P, Asai M, Aso T, Bagli E, Bagulya A, Banerjee S, Barrand G, Beck BR, Bogdanov AG, Brandt D, Brown JMC, Burkhardt H, Canal P, Cano-Ott D, Chauvie S, Cho K, Cirrone GAP, Cooperman G, Cort \'e s-Giraldo MA, Cosmo G, Cuttone G, Depaola G, Desorgher L, Dong X, Dotti A, Elvira VD, Folger G, Francis Z, Galoyan A, Garnier ...

    2016

  4. [4]

    697(2):1071--1102, doi:10.1088/0004-637X/697/2/1071, 0902.1089

    Atwood WB, Abdo AA, Ackermann M, Althouse W, Anderson B, Axelsson M, Baldini L, Ballet J, Band DL, Barbiellini G, Bartelt J, Bastieri D, Baughman BM, Bechtol K, B \'e d \'e r \`e de D, Bellardi F, Bellazzini R, Berenji B, Bignami GF, Bisello D, Bissaldi E, Blandford RD, Bloom ED, Bogart JR, Bonamente E, Bonnell J, Borgland AW, Bouvier A, Bregeon J, Brez A...

    arXiv 2009

  5. [5]

    Astroparticle Physics 133:102628, doi:10.1016/j.astropartphys.2021.102628, 2107.05496

    Baldini L, Barbanera M, Bellazzini R, Bonino R, Borotto F, Brez A, Caporale C, Cardelli C, Castellano S, Ceccanti M, Citraro S, Di Lalla N, Latronico L, Lucchesi L, Magazz \`u C, Magazz \`u G, Maldera S, Manfreda A, Marengo M, Marrocchesi A, Mereu P, Minuti M, Mosti F, Nasimi H, Nuti A, Oppedisano C, Orsini L, Pesce-Rollins M, Pinchera M, Profeti A, Sgr \...

    arXiv 2021

  6. [6]

    Springer

    Bambi C, Sangangelo A (2022) Handbook of X-ray and Gamma-ray Astrophysics . Springer

    2022

  7. [7]

    120(3-4):143--164, doi:10.1007/s11214-005-5096-3, astro-ph/0507410

    Barthelmy SD, Barbier LM, Cummings JR, Fenimore EE, Gehrels N, Hullinger D, Krimm HA, Markwardt CB, Palmer DM, Parsons A, Sato G, Suzuki M, Takahashi T, Tashiro M, Tueller J (2005) The Burst Alert Telescope (BAT) on the SWIFT Midex Mission . 120(3-4):143--164, doi:10.1007/s11214-005-5096-3, astro-ph/0507410

    arXiv 2005

  8. [8]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 101, doi:10.1007/978-981-16-4544-0_50-1

    Bernard D, Hunter SD, Tanimori T (2022) Time Projection Chambers for Gamma-Ray Astronomy . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 101, doi:10.1007/978-981-16-4544-0_50-1

    work page doi:10.1007/978-981-16-4544-0_50-1 2022

Show all 97 references
  1. [9]

    Journal of Astrophysics and Astronomy 38(2):31, doi:10.1007/s12036-017-9447-8, 1608.03408

    Bhalerao V, Bhattacharya D, Vibhute A, Pawar P, Rao AR, Hingar MK, Khanna R, Kutty APK, Malkar JP, Patil MH, Arora YK, Sinha S, Priya P, Samuel E, Sreekumar S, Vinod P, Mithun NPS, Vadawale SV, Vagshette N, Navalgund KH, Sarma KS, Pandiyan R, Seetha S, Subbarao K (2017) The Ca...

    2017 arXiv

  2. [10]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 55, doi:10.1007/978-981-16-4544-0_49-1

    Bissaldi E, Fiorini C, Uliyanov A (2022) Photodetectors for Gamma-Ray Astronomy . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 55, doi:10.1007/978-981-16-4544-0_49-1

    2022 doi

  3. [11]

    Bloser PF, Sharma T, Legere JS, Bancroft CM, McConnell ML, Ryan JM, Wright AM (2018) The Advanced Scintillator Compton Telescope (ASCOT) balloon payload . In: den Herder JWA, Nikzad S, Nakazawa K (eds) Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, Societ...

    2018 doi

  4. [12]

    50(7-8):604--607, doi:10.1016/j.newar.2006.06.076, astro-ph/0608532

    Boggs SE (2006) The Advanced Compton Telescope mission . 50(7-8):604--607, doi:10.1016/j.newar.2006.06.076, astro-ph/0608532

    2006 arXiv

  5. [13]

    Briel UG, Aschenbach B, Balasini M, Braeuninger HW, Burkert W, Dennerl K, Ehle M, Haberl F, Hartmann R, Hartner GD, Holl P, Massa P, Meidinger N, Kemmer J, Kendziorra E, Kirsch M, Krause N, Kuster M, Lumb DH, Pfeffermann E, Pal J, Pietsch W, Popp M, Read A, Reppin C, Soltau H,...

    2000

  6. [14]

    Journal of Astronomical Telescopes, Instruments, and Systems 8:044003, doi:10.1117/1.JATIS.8.4.044003, 2208.04990

    Caputo R, Ajello M, Kierans CA, Perkins JS, Racusin JL, Baldini L, Baring MG, Bissaldi E, Burns E, Cannady N, Charles E, da Silva RMC, Fang K, Fleischhack H, Fryer C, Fukazawa Y, Grove JE, Hartmann D, Howell EJ, Jadhav M, Karwin CM, Kocevski D, Kurahashi N, Latronico L, Lewis ...

    2022 arXiv

  7. [15]

    Experimental Astronomy 47(3):273--302, doi:10.1007/s10686-019-09624-0, 1902.06944

    Cumani P, Hernanz M, Kiener J, Tatischeff V, Zoglauer A (2019) Background for a gamma-ray satellite on a low-Earth orbit . Experimental Astronomy 47(3):273--302, doi:10.1007/s10686-019-09624-0, 1902.06944

    2019 arXiv

  8. [16]

    Exploring the extreme Universe with gamma rays in the MeV - GeV range

    De Angelis A, Tatischeff V, Tavani M, Oberlack U, Grenier I, Hanlon L, Walter R, Argan A, von Ballmoos P, Bulgarelli A, Donnarumma I, Hernanz M, Kuvvetli I, Pearce M, Zdziarski A, Aboudan A, Ajello M, Ambrosi G, Bernard D, Bernardini E, Bonvicini V, Brogna A, Branchesi M, Budt...

    2017 arXiv

  9. [17]

    411:L189--L195, doi:10.1051/0004-6361:20031346, astro-ph/0309224

    Di Cocco G, Caroli E, Celesti E, Foschini L, Gianotti F, Labanti C, Malaguti G, Mauri A, Rossi E, Schiavone F, Spizzichino A, Stephen JB, Traci A, Trifoglio M (2003) IBIS/PICsIT in-flight performances . 411:L189--L195, doi:10.1051/0004-6361:20031346, astro-ph/0309224

    2003 arXiv

  10. [18]

    Fiore F, Burderi L, Lavagna M, Bertacin R, Evangelista Y, Campana R, Fuschino F, Lunghi P, Monge A, Negri B, Pirrotta S, Puccetti S, Sanna A, Amarilli F, Ambrosino F, Amelino-Camelia G, Anitra A, Auricchio N, Barbera M, Bechini M, Bellutti P, Bertuccio G, Cao J, Ceraudo F, Che...

    2020 arXiv

  11. [19]

    IEEE Transactions on Nuclear Science 60(4):2923--2933, doi:10.1109/TNS.2013.2273418

    Fiorini C, Bombelli L, Busca P, Marone A, Peloso R, Quaglia R, Bellutti P, Boscardin M, Ficorella F, Giacomini G, Picciotto A, Piemonte C, Zorzi N, Nelms N, Shortt B (2013) Silicon Drift Detectors for Readout of Scintillators in Gamma-Ray Spectroscopy . IEEE Transactions on Nu...

    2013

  12. [20]

    In: 37th International Cosmic Ray Conference, p 649, doi:10.22323/1.395.0649, 2108.02860

    Fleischhack H (2022) AMEGO-X: MeV gamma-ray Astronomy in the Multi-messenger Era . In: 37th International Cosmic Ray Conference, p 649, doi:10.22323/1.395.0649, 2108.02860

    2022 arXiv

  13. [21]

    Garmire GP, Bautz MW, Ford PG, Nousek JA, Ricker J George R (2003) Advanced CCD imaging spectrometer (ACIS) instrument on the Chandra X-ray Observatory . In: Truemper JE, Tananbaum HD (eds) X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy., Society of Photo-Optical...

    2003 doi

  14. [22]

    Nuclear Instruments and Methods in Physics Research 225(3):608--614, doi:10.1016/0167-5087(84)90113-3

    Gatti E, Rehak P (1984) Semiconductor drift chamber An application of a novel charge transport scheme . Nuclear Instruments and Methods in Physics Research 225(3):608--614, doi:10.1016/0167-5087(84)90113-3

    1984 doi

  15. [23]

    Gendreau KC, Arzoumanian Z, Adkins PW, Albert CL, Anders JF, Aylward AT, Baker CL, Balsamo ER, Bamford WA, Benegalrao SS, Berry DL, Bhalwani S, Black JK, Blaurock C, Bronke GM, Brown GL, Budinoff JG, Cantwell JD, Cazeau T, Chen PT, Clement TG, Colangelo AT, Coleman JS, Coopers...

    2016

  16. [24]

    Journal of Astronomical Instrumentation 10(2):2150009-163, doi:10.1142/S2251171721500094, 2102.01992

    Gevin O, Limousin O, Lugiez F, Michalowska A, Meuris A, Baudin D, Delagnes E, Lemaire O, Pinsard F (2021) IDeF-X HD: A CMOS ASIC for the Readout of Cd(Zn)Te Detectors for Space-Borne Applications . Journal of Astronomical Instrumentation 10(2):2150009-163, doi:10.1142/S2251171...

    2021 arXiv

  17. [25]

    Astroparticle Physics 97:10--18, doi:10.1016/j.astropartphys.2017.10.008, 1706.06483

    Gros P, Amano S, Atti \'e D, Baron P, Baudin D, Bernard D, Bruel P, Calvet D, Colas P, Dat \'e S, Delbart A, Frotin M, Geerebaert Y, Giebels B, G \"o tz D, Hashimoto S, Horan D, Kotaka T, Louzir M, Magniette F, Minamiyama Y, Miyamoto S, Ohkuma H, Poilleux P, Semeniouk I, Sizun...

    2018 arXiv

  18. [26]

    770(2):103, doi:10.1088/0004-637X/770/2/103, 1301.7307

    Harrison FA, Craig WW, Christensen FE, Hailey CJ, Zhang WW, Boggs SE, Stern D, Cook WR, Forster K, Giommi P, Grefenstette BW, Kim Y, Kitaguchi T, Koglin JE, Madsen KK, Mao PH, Miyasaka H, Mori K, Perri M, Pivovaroff MJ, Puccetti S, Rana VR, Westergaard NJ, Willis J, Zoglauer A...

    2013 arXiv

  19. [27]

    Hayashida K, Tomida H, Mori K, Nakajima H, Tanaka T, Uchida H, Tsuru TG, Murakami H, Okajima T, Kohmura T, Hagino K, Kobayashi SB, Ishida M, Maeda Y, Uchiyama H, Yamaoka K, Matsumoto H, Nobukawa M, Nobukawa KK, Hiraga JS, Yamauchi M, Hatsukade I, Soong Y, Mori H, Hayashi T, Ts...

    2018

  20. [28]

    Astroparticle Physics 59:18--28, doi:10.1016/j.astropartphys.2014.04.002, 1311.2059

    Hunter SD, Bloser PF, Depaola GO, Dion MP, DeNolfo GA, Hanu A, Iparraguirre M, Legere J, Longo F, McConnell ML, Nowicki SF, Ryan JM, Son S, Stecker FW (2014) A pair production telescope for medium-energy gamma-ray polarimetry . Astroparticle Physics 59:18--28, doi:10.1016/j.as...

    2014 arXiv

  21. [29]

    Hurley K (1978) Phosphorescence in CS iCrystals . 69:313

    1978

  22. [30]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 66, doi:10.1007/978-981-16-4544-0_48-1

    Iyudin AF, Labanti C, Roberts OJ (2022) Scintillation Detectors in Gamma-Ray Astronomy . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 66, doi:10.1007/978-981-16-4544-0_48-1

    2022 doi

  23. [31]

    163(2):401--423, doi:10.1086/500659, astro-ph/0511531

    Jahoda K, Markwardt CB, Radeva Y, Rots AH, Stark MJ, Swank JH, Strohmayer TE, Zhang W (2006) Calibration of the Rossi X-Ray Timing Explorer Proportional Counter Array . 163(2):401--423, doi:10.1086/500659, astro-ph/0511531

    2006 arXiv

  24. [32]

    Journal of Crystal Growth 352(1):88--90, doi:10.1016/j.jcrysgro.2011.11.085

    Kamada K, Yanagida T, Endo T, Tsutumi K, Usuki Y, Nikl M, Fujimoto Y, Fukabori A, Yoshikawa A (2012) 2 inch diameter single crystal growth and scintillation properties of Ce:Gd _ 3 Al _ 2 Ga _ 3 O _ 12 . Journal of Crystal Growth 352(1):88--90, doi:10.1016/j.jcrysgro.2011.11.085

    2012 doi

  25. [33]

    Nuclear Instruments and Methods in Physics Research A 541(1-2):310--322, doi:10.1016/j.nima.2005.01.071

    Kanbach G, Andritschke R, Zoglauer A, Ajello M, McConnell ML, Macri JR, Ryan JM, Bloser P, Hunter S, Di Cocco G, Kurfess J, Reglero V (2005) Development and calibration of the tracking Compton/Pair telescope MEGA . Nuclear Instruments and Methods in Physics Research A 541(1-2)...

    2005 doi

  26. [34]

    Nuclear Instruments and Methods in Physics Research A 835:74--85, doi:10.1016/j.nima.2016.08.009

    Khalil M, Laurent P, Lebrun F, Tatischeff V, Dolgorouky Y, Bertoli W, Breelle E (2016) Thick silicon microstrip detectors simulation for PACT: Pair and Compton Telescope . Nuclear Instruments and Methods in Physics Research A 835:74--85, doi:10.1016/j.nima.2016.08.009

    2016 doi

  27. [35]

    arXiv e-prints arXiv:2407.18737, doi:10.48550/arXiv.2407.18737, 2407.18737

    Kirschner N, Kierans C, Wasti S, Schoenwald AJ, Caputo R, Griffin S, Liceaga-Indart I, Parker L, Perkins JS, Zajczyk A (2024) The Double-Sided Silicon Strip Detector Tracker onboard the ComPair Balloon Flight . arXiv e-prints arXiv:2407.18737, doi:10.48550/arXiv.2407.18737, 2407.18737

    2024 doi arXiv

  28. [36]

    John Wiley and Sons

    Knoll GF (2010) Radiation detection and measurement, 4th Edition . John Wiley and Sons

    2010

  29. [37]

    209(1):14, doi:10.1088/0067-0049/209/1/14, 1309.0755

    Krimm HA, Holland ST, Corbet RHD, Pearlman AB, Romano P, Kennea JA, Bloom JS, Barthelmy SD, Baumgartner WH, Cummings JR, Gehrels N, Lien AY, Markwardt CB, Palmer DM, Sakamoto T, Stamatikos M, Ukwatta TN (2013) The Swift/BAT Hard X-Ray Transient Monitor . 209(1):14, doi:10.1088...

    2013 arXiv

  30. [38]

    510(4):4796--4807, doi:10.1093/mnras/stab3751, 2111.02996

    Krivonos RA, Sazonov SY, Kuznetsova EA, Lutovinov AA, Mereminskiy IA, Tsygankov SS (2022) INTEGRAL/IBIS 17-yr hard X-ray all-sky survey . 510(4):4796--4807, doi:10.1093/mnras/stab3751, 2111.02996

    2022 arXiv

  31. [39]

    Journal of Instrumentation 16(8):P08038, doi:10.1088/1748-0221/16/08/P08038, 2107.09281

    Kushwah R, Stana TA, Pearce M (2021) The design and performance of CUBES - a CubeSat X-ray detector . Journal of Instrumentation 16(8):P08038, doi:10.1088/1748-0221/16/08/P08038, 2107.09281

    2021 arXiv

  32. [40]

    Labanti C, Amati L, Frontera F, Mereghetti S, Gasent-Blesa JL, Tenzer C, Orleanski P, Kuvvetli I, Campana R, Fuschino F, Terenzi L, Virgilli E, Morgante G, Orlandini M, Butler RC, Stephen JB, Auricchio N, De Rosa A, Da Ronco V, Evangelisti F, Melchiorri M, Squerzanti S, Fiorin...

    2020

  33. [41]

    Astroparticle Physics 103:131--141, doi:10.1016/j.astropartphys.2018.08.002

    Lacombe K, Dezalay JP, Houret B, Amoros C, Atteia JL, Bouchet L, Cordier B, Gevin O, Godet O, Gonzalez F, Guillemot P, Limousin O, Pons R, Ramon P, Waegebaert V (2018) Spectral performance of ECLAIRs flight detectors on SVOM mission . Astroparticle Physics 103:131--141, doi:10...

    2018 doi

  34. [42]

    411:L141--L148, doi:10.1051/0004-6361:20031367, astro-ph/0310362

    Lebrun F, Leray JP, Lavocat P, Cr \'e tolle J, Arqu \`e s M, Blondel C, Bonnin C, Bou \`e re A, Cara C, Chaleil T, Daly F, Desages F, Dzitko H, Horeau B, Laurent P, Limousin O, Mathy F, Mauguen V, Meignier F, Molini \'e F, Poindron E, Rouger M, Sauvageon A, Tourrette T (2003) ...

    2003 arXiv

  35. [43]

    210(1):3--32, doi:10.1023/A:1022428818870

    Lin RP, Dennis BR, Hurford GJ, Smith DM, Zehnder A, Harvey PR, Curtis DW, Pankow D, Turin P, Bester M, Csillaghy A, Lewis M, Madden N, van Beek HF, Appleby M, Raudorf T, McTiernan J, Ramaty R, Schmahl E, Schwartz R, Krucker S, Abiad R, Quinn T, Berg P, Hashii M, Sterling R, Ja...

    2002

  36. [44]

    a m \"a r \

    Lund N, Budtz-J rgensen C, Westergaard NJ, Brandt S, Rasmussen IL, Hornstrup A, Oxborrow CA, Chenevez J, Jensen PA, Laursen S, Andersen KH, Mogensen PB, Rasmussen I, Om K, Pedersen SM, Polny J, Andersson H, Andersson T, K \"a m \"a r \"a inen V, Vilhu O, Huovelin J, Maisala S,...

    2003

  37. [45]

    Springer, doi:10.1007/978-3-540-71679-2

    Lutz G (2007) Semiconductor Radiation Detectors . Springer, doi:10.1007/978-3-540-71679-2

    2007 doi

  38. [46]

    Nuclear Instruments and Methods 178:363--381, doi:10.1016/0029-554X(80)90815-0

    Mahoney WA, Ling JC, Jacobson AS, Tapphorn RM (1980) The HEAO 3 gamma-ray spectrometer. Nuclear Instruments and Methods 178:363--381, doi:10.1016/0029-554X(80)90815-0

    1980 doi

  39. [47]

    Nuclear Instruments and Methods in Physics Research A 912:199--204, doi:10.1016/j.nima.2017.11.035

    Maier D, Horeau B, Laurent P, Limousin O, Renaud D, Kawaharada M, Kokubun M, Sato G, Takahashi T, Watanabe S, Nakazawa K, Boatella Polo C (2018) Long-term test of a stacked CdTe mini-HXI setup . Nuclear Instruments and Methods in Physics Research A 912:199--204, doi:10.1016/j....

    2018 doi

  40. [48]

    Nuclear Instruments and Methods in Physics Research A 1049:168080, doi:10.1016/j.nima.2023.168080

    Maldera S, Fermi-LAT Collaboration (2023) Performance of the Fermi-LAT silicon strip tracker after 14 years of operation . Nuclear Instruments and Methods in Physics Research A 1049:168080, doi:10.1016/j.nima.2023.168080

    2023

  41. [49]

    122:341--356, doi:10.1051/aas:1997139

    Manzo G, Giarrusso S, Santangelo A, Ciralli F, Fazio G, Piraino S, Segreto A (1997) The high pressure gas scintillation proportional counter on-board the BeppoSAX X-ray astronomy satellite . 122:341--356, doi:10.1051/aas:1997139

    1997 doi

  42. [50]

    Review of Scientific Instruments 19(11):744--770, doi:10.1063/1.1741156

    Marshall FH, Coltman JW, Bennett AI (1948) The Photo-Multiplier Radiation Detector . Review of Scientific Instruments 19(11):744--770, doi:10.1063/1.1741156

    1948 doi

  43. [51]

    Nuclear Instruments and Methods in Physics Research A 676:135--139, doi:10.1016/j.nima.2011.11.076

    Matei C, Hambsch FJ, Oberstedt S (2012) Proton light output function and neutron efficiency of a p-terphenyl detector using a ^ 252 Cf source . Nuclear Instruments and Methods in Physics Research A 676:135--139, doi:10.1016/j.nima.2011.11.076

    2012 doi

  44. [52]

    In: Journal of Physics Conference Series, Journal of Physics Conference Series, vol 763, p 012008, doi:10.1088/1742-6596/763/1/012008

    McConnell ML, Bloser PF, Legere J, Ryan JM (2016) Applications for New Scintillator Technologies in Gamma Ray Astronomy . In: Journal of Physics Conference Series, Journal of Physics Conference Series, vol 763, p 012008, doi:10.1088/1742-6596/763/1/012008

    2016 doi

  45. [53]

    Nuclear Instruments and Methods in Physics Research A 695:288--292, doi:10.1016/j.nima.2011.11.016

    Meuris A, Hurford G, Bednarzik M, Limousin O, Gevin O, Le Mer I, Martignac J, Horeau B, Grimm O, Resanovic R, Krucker S, Orlea \'n ski P (2012) Caliste-SO X-ray micro-camera for the STIX instrument on-board Solar Orbiter space mission . Nuclear Instruments and Methods in Physi...

    2012 doi

  46. [54]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 10, doi:10.1007/978-981-16-4544-0_161-1

    Meuris A, Nagazawa K, Kuvvetli I, Caroli E (2022) Cd(Zn)Te Detectors for Hard X-Ray and Gamma-Ray Astronomy . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 10, doi:10.1007/978-981-16-4544-0_161-1

    2022 doi

  47. [55]

    Nuclear Instruments and Methods in Physics Research A 988:164798, doi:10.1016/j.nima.2020.164798, 2003.08213

    Mitchell L, Phlips B, Johnson WN, Johnson-Rambert M, Kansky AN, Woolf R (2021) Radiation damage assessment of SensL SiPMs . Nuclear Instruments and Methods in Physics Research A 988:164798, doi:10.1016/j.nima.2020.164798, 2003.08213

    2021

  48. [56]

    Mitchell LJ, Phlips BF, Woolf RS, Finne TT, Johnson WN (2019) Strontium iodide radiation instrumentation II (SIRI-2) . In: Siegmund OH (ed) UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXI, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Se...

    2019 doi

  49. [57]

    Astroparticle Physics 27(5):339--358, doi:10.1016/j.astropartphys.2006.12.003, astro-ph/0702581

    Moiseev AA, Hartman RC, Ormes JF, Thompson DJ, Amato MJ, Johnson TE, Segal KN, Sheppard DA (2007) The anti-coincidence detector for the GLAST large area telescope . Astroparticle Physics 27(5):339--358, doi:10.1016/j.astropartphys.2006.12.003, astro-ph/0702581

    2007 arXiv

  50. [58]

    Journal of Astronomical Telescopes, Instruments, and Systems 4:021410, doi:10.1117/1.JATIS.4.2.021410

    Nakazawa K, Sato G, Kokubun M, Enoto T, Fukazawa Y, Hagino K, Hayashi K, Kataoka J, Katsuta J, Kobayashi SB, Laurent P, Lebrun F, Limousin O, Maier D, Makishima K, Mizuno T, Mori K, Nakamori T, Nakano T, Noda H, Odaka H, Ohno M, Ohta M, Saito S, Sato R, Tajima H, Takahashi H, ...

    2018

  51. [59]

    235(1):4, doi:10.3847/1538-4365/aaa7fd, 1801.01882

    Oh K, Koss M, Markwardt CB, Schawinski K, Baumgartner WH, Barthelmy SD, Cenko SB, Gehrels N, Mushotzky R, Petulante A, Ricci C, Lien A, Trakhtenbrot B (2018) The 105-Month Swift-BAT All-sky Hard X-Ray Survey . 235(1):4, doi:10.3847/1538-4365/aaa7fd, 1801.01882

    2018 arXiv

  52. [60]

    Nuclear Instruments and Methods in Physics Research A 556(1):228--236, doi:10.1016/j.nima.2005.10.016

    Perotti F, Fiorini M, Incorvaia S, Mattaini E, Sant'Ambrogio E (2006) The AGILE anticoincidence detector . Nuclear Instruments and Methods in Physics Research A 556(1):228--236, doi:10.1016/j.nima.2005.10.016

    2006 doi

  53. [61]

    IRE Transactions on Nuclear Science 8(4):21--29, doi:10.1109/TNS2.1961.4315853

    Peterson LE, Howard RL (1961) Gamma-ray astronomy in space in the 50-kev to 3-mev region. IRE Transactions on Nuclear Science 8(4):21--29, doi:10.1109/TNS2.1961.4315853

    1961

  54. [62]

    Nuclear Instruments and Methods in Physics Research A 926:2--15, doi:10.1016/j.nima.2018.11.119

    Piemonte C, Gola A (2019) Overview on the main parameters and technology of modern Silicon Photomultipliers . Nuclear Instruments and Methods in Physics Research A 926:2--15, doi:10.1016/j.nima.2018.11.119

    2019 doi

  55. [63]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 97, doi:10.1007/978-981-16-4544-0_163-1

    Roques JP, Teegarden BJ, Lawrence DJ, Jourdain E (2022) The Use of Germanium Detectors in Space . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 97, doi:10.1007/978-981-16-4544-0_163-1

    2022 doi

  56. [64]

    In: Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 154, doi:10.1007/978-981-16-4544-0_34-1

    Santangelo A, Zhang SN, Feroci M, Hernanz M, Lu F, Xu Y (2023) The Enhanced X-Ray Timing and Polarimetry Mission: eXTP . In: Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 154, doi:10.1007/978-981-16-4544-0_34-1

    2023 doi

  57. [65]

    86:657, doi:10.1086/191794

    Schoenfelder V, Aarts H, Bennett K, de Boer H, Clear J, Collmar W, Connors A, Deerenberg A, Diehl R, von Dordrecht A, den Herder JW, Hermsen W, Kippen M, Kuiper L, Lichti G, Lockwood J, Macri J, McConnell M, Morris D, Much R, Ryan J, Simpson G, Snelling M, Stacy G, Steinle H, ...

    1993 doi

  58. [66]

    411:L215--L222, doi:10.1051/0004-6361:20031436

    Segreto A, Labanti C, Bazzano A, Bird AJ, Celesti E, Marisaldi M (2003) Cosmic rays tracks on the PICsIT detector . 411:L215--L222, doi:10.1051/0004-6361:20031436

    2003 doi

  59. [67]

    Journal of Applied Physics 9(10):635--636, doi:10.1063/1.1710367

    Shockley W (1938) Currents to Conductors Induced by a Moving Point Charge . Journal of Applied Physics 9(10):635--636, doi:10.1063/1.1710367

    1938 doi

  60. [68]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 80, doi:10.1007/978-981-16-4544-0_43-1

    Siegert T, Horan D, Kanbach G (2022) Telescope Concepts in Gamma-Ray Astronomy . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 80, doi:10.1007/978-981-16-4544-0_43-1

    2022 doi

  61. [69]

    Journal of Astrophysics and Astronomy 38(2):29, doi:10.1007/s12036-017-9448-7

    Singh KP, Stewart GC, Westergaard NJ, Bhattacharayya S, Chandra S, Chitnis VR, Dewangan GC, Kothare AT, Mirza IM, Mukerjee K, Navalkar V, Shah H, Abbey AF, Beardmore AP, Kotak S, Kamble N, Vishwakarama S, Pathare DP, Risbud VM, Koyande JP, Stevenson T, Bicknell C, Crawford T, ...

    2017

  62. [70]

    Soffitta P, Baldini L, Baumgartner W, Bellazzini R, Bongiorno SD, Bucciantini N, Costa E, Dov c iak M, Ehlert S, Kaaret PE, Kolodziejczak JJ, Latronico L, Marin F, Marscher AP, Marshall HL, Matt G, Muleri F, O'Dell SL, Poutanen J, Ramsey B, Romani RW, Slane P, Tennant AF, Turo...

    2023

  63. [71]

    arXiv e-prints arXiv:2407.05947, doi:10.48550/arXiv.2407.05947, 2407.05947

    Steinhebel AL, Ott J, Kroger O, Caputo R, Fadeyev V, Affolder A, Affolder K, Deshmukh A, Striebig N, Jadhav M, Suda Y, Fukazawa Y, Metcalfe J, Leys R, Peric I, Taylor , Shin , Violette D (2024) The path toward 500 m depletion of AstroPix, a pixelated silicon HVCMOS sensor for ...

    2024 doi arXiv

  64. [72]

    Nuclear Instruments and Methods in Physics Research A 1068:169762, doi:10.1016/j.nima.2024.169762, 2408.12891

    Suda Y, Caputo R, Steinhebel AL, Striebig N, Jadhav M, Fukazawa Y, Hashizume M, Kierans C, Leys R, Metcalfe J, Negro M, Peri \'c I, Perkins JS, Shin T, Tajima H, Violette D, Nakano N (2024) Performance evaluation of the high-voltage CMOS active pixel sensor AstroPix for gamma-...

    2024

  65. [73]

    930(1):6, doi:10.3847/1538-4357/ac6103, 2107.00180

    Takada A, Takemura T, Yoshikawa K, Mizumura Y, Ikeda T, Nakamura Y, Onozaka K, Abe M, Hamaguchi K, Kubo H, Kurosawa S, Miuchi K, Saito K, Sawano T, Tanimori T (2022) First Observation of the MeV Gamma-Ray Universe with Bijective Imaging Spectroscopy Using the Electron-tracking...

    2022 arXiv

  66. [74]

    Journal of Astronomical Telescopes, Instruments, and Systems 4:021402, doi:10.1117/1.JATIS.4.2.021402

    Takahashi T, Kokubun M, Mitsuda K, Kelley RL, Ohashi T, Aharonian F, Akamatsu H, Akimoto F, Allen SW, Anabuki N, Angelini L, Arnaud K, Asai M, Audard M, Awaki H, Axelsson M, Azzarello P, Baluta C, Bamba A, Bando N, Bautz MW, Bialas T, Blandford R, Boyce K, Brenneman LW, Brown ...

    2018

  67. [75]

    In: Ruffino R, Vereshchagin G (eds) The Sixteenth Marcel Grossmann Meeting

    Tashiro MS (2023) XRISM: X-ray imaging and spectroscopy mission . In: Ruffino R, Vereshchagin G (eds) The Sixteenth Marcel Grossmann Meeting. On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories, pp 95--103, d...

    2023 doi

  68. [76]

    Tatischeff V, Tavani M, von Ballmoos P, Hanlon L, Oberlack U, Aboudan A, Argan A, Bernard D, Brogna A, Bulgarelli A, Bykov A, Campana R, Caraveo P, Cardillo M, Coppi P, De Angelis A, Diehl R, Donnarumma I, Fioretti V, Giuliani A, Grenier I, Grove JE, Hamadache C, Hartmann D, H...

    2016 arXiv

  69. [77]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 53, doi:10.1007/978-981-16-4544-0_47-1

    Tatischeff V, Ubertini P, Mizuno T, Natalucci L (2022) Orbits and Background of Gamma-Ray Space Instruments . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 53, doi:10.1007/978-981-16-4544-0_47-1

    2022 doi

  70. [78]

    502(3):995--1013, doi:10.1051/0004-6361/200810527, 0807.4254

    Tavani M, Barbiellini G, Argan A, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Costa E, D'Ammando F, Del Monte E, de Paris G, Di Cocco G, di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Fornari F, Fuschino F, Froysland T, Frutti...

    2009 arXiv

  71. [79]

    In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 54, doi:10.1007/978-981-16-4544-0_159-1

    Thompson DJ, Moiseev AA (2022) Pair Production Detectors for Gamma-Ray Astrophysics . In: Bambi C, Sangangelo A (eds) Handbook of X-ray and Gamma-ray Astrophysics, Springer, p 54, doi:10.1007/978-981-16-4544-0_159-1

    2022 doi

  72. [80]

    86:629, doi:10.1086/191793

    Thompson DJ, Bertsch DL, Fichtel CE, Hartman RC, Hofstadter R, Hughes EB, Hunter SD, Hughlock BW, Kanbach G, Kniffen DA, Lin YC, Mattox JR, Mayer-Hasselwander HA, von Montigny C, Nolan PL, Nel HI, Pinkau K, Rothermel H, Schneid EJ, Sommer M, Sreekumar P, Tieger D, Walker AH (1...

    1993 doi

  73. [81]

    arXiv e-prints arXiv:2308.12362, doi:10.48550/arXiv.2308.12362, 2308.12362

    Tomsick JA, Boggs SE, Zoglauer A, Hartmann D, Ajello M, Burns E, Fryer C, Karwin C, Kierans C, Lowell A, Malzac J, Roberts J, Saint-Hilaire P, Shih A, Siegert T, Sleator C, Takahashi T, Tavecchio F, Wulf E, Beechert J, Gulick H, Joens A, Lazar H, Neights E, Martinez Oliveros J...

    2023 doi arXiv

  74. [82]

    411:L131--L139, doi:10.1051/0004-6361:20031224

    Ubertini P, Lebrun F, Di Cocco G, Bazzano A, Bird AJ, Broenstad K, Goldwurm A, La Rosa G, Labanti C, Laurent P, Mirabel IF, Quadrini EM, Ramsey B, Reglero V, Sabau L, Sacco B, Staubert R, Vigroux L, Weisskopf MC, Zdziarski AA (2003) IBIS: The Imager on-board INTEGRAL . 411:L13...

    2003 doi

  75. [83]

    IEEE Transactions on Nuclear Science 59(3):656--664, doi:10.1109/TNS.2012.2193597

    van Dam HT, Seifert S, Drozdowski W, Dorenbos P, Schaart DR (2012) Optical Absorption Length, Scattering Length, and Refractive Index of LaBr _ 3 :Ce ^ 3+ . IEEE Transactions on Nuclear Science 59(3):656--664, doi:10.1109/TNS.2012.2193597

    2012

  76. [84]

    o nfelder V, Mandrou P, Lichti GG, von Kienlin A, Cordier B, Schanne S, Kn \

    Vedrenne G, Roques JP, Sch \"o nfelder V, Mandrou P, Lichti GG, von Kienlin A, Cordier B, Schanne S, Kn \"o dlseder J, Skinner G, Jean P, Sanchez F, Caraveo P, Teegarden B, von Ballmoos P, Bouchet L, Paul P, Matteson J, Boggs S, Wunderer C, Leleux P, Weidenspointner G, Durouch...

    2003 doi

  77. [85]

    Virgilli E, Frontera F, Ferro L, Moita MF, Cavazzini L, Rosati P, Guidorzi C, Orlandini M, Labanti C, Caroli E, Auricchio N, Stephen JB, del Sordo S, Amati L (2022) ASTENA: an innovative mission concept for broadband high-energy astrophysics . In: den Herder JWA, Nikzad S, Nak...

    2022 doi

  78. [86]

    893(1):46, doi:10.3847/1538-4357/ab7a18, 2002.11460

    von Kienlin A, Meegan CA, Paciesas WS, Bhat PN, Bissaldi E, Briggs MS, Burns E, Cleveland WH, Gibby MH, Giles MM, Goldstein A, Hamburg R, Hui CM, Kocevski D, Mailyan B, Malacaria C, Poolakkil S, Preece RD, Roberts OJ, Veres P, Wilson-Hodge CA (2020) The Fourth Fermi-GBM Gamma-...

    2020 arXiv

  79. [87]

    Nuclear Instruments and Methods in Physics Research A 765:192--201, doi:10.1016/j.nima.2014.05.127, 1509.00588

    Watanabe S, Tajima H, Fukazawa Y, Ichinohe Y, Takeda S, Enoto T, Fukuyama T, Furui S, Genba K, Hagino K, Harayama A, Kuroda Y, Matsuura D, Nakamura R, Nakazawa K, Noda H, Odaka H, Ohta M, Onishi M, Saito S, Sato G, Sato T, Takahashi T, Tanaka T, Togo A, Tomizuka S (2014) The S...

    2014 arXiv

  80. [88]

    156(1):69--91, doi:10.1086/425577, astro-ph/0408399

    Weidenspointner G, Harris MJ, Sturner S, Teegarden BJ, Ferguson C (2005) MGGPOD: a Monte Carlo Suite for Modeling Instrumental Line and Continuum Backgrounds in Gamma-Ray Astronomy . 156(1):69--91, doi:10.1086/425577, astro-ph/0408399

    2005 arXiv

  81. [89]

    Weisskopf MC, Tananbaum HD, Van Speybroeck LP, O'Dell SL (2000) Chandra X-ray Observatory (CXO): overview . In: Truemper JE, Aschenbach B (eds) X-Ray Optics, Instruments, and Missions III, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, vol 4012, p...

    2000 arXiv

  82. [90]

    Experimental Astronomy 48(1):77--95, doi:10.1007/s10686-019-09636-w, 1907.06842

    Wen J, Long X, Zheng X, An Y, Cai Z, Cang J, Che Y, Chen C, Chen L, Chen Q, Chen Z, Cheng Y, Deng L, Deng W, Ding W, Du H, Duan L, Gan Q, Gao T, Gao Z, Han W, Han Y, He X, He X, Hou L, Hu F, Hu J, Huang B, Huang D, Huang X, Jia S, Jiang Y, Jin Y, Li K, Li S, Li Y, Liang J, Lia...

    2019 arXiv

  83. [91]

    Journal of Instrumentation 13(2):P02023, doi:10.1088/1748-0221/13/02/P02023

    Yoneyama M, Kataoka J, Arimoto M, Masuda T, Yoshino M, Kamada K, Yoshikawa A, Sato H, Usuki Y (2018) Evaluation of GAGG:Ce scintillators for future space applications . Journal of Instrumentation 13(2):P02023, doi:10.1088/1748-0221/13/02/P02023

    2018 doi

  84. [92]

    Nuclear Instruments and Methods in Physics Research A 1044:167510, doi:10.1016/j.nima.2022.167510, 2205.10506

    Zheng X, Gao H, Wen J, Zeng M, Pan X, Xu D, Liu Y, Zhang Y, Peng H, Jiang Y, Long X, Lu D, Yang D, Feng H, Zeng Z, Cang J, Tian Y, GRID Collaboration (2022) In-orbit radiation damage characterization of SiPMs in the GRID-02 CubeSat detector . Nuclear Instruments and Methods in...

    2022

  85. [93]

    50(7-8):629--632, doi:10.1016/j.newar.2006.06.049

    Zoglauer A, Andritschke R, Schopper F (2006) MEGAlib The Medium Energy Gamma-ray Astronomy Library . 50(7-8):629--632, doi:10.1016/j.newar.2006.06.049

    2006 doi

  86. [94]

    , " * write output.state after.block = add.period write newline

    ENTRY address archive author booktitle chapter doi edition editor eid eprint howpublished institution journal key month note number organization pages publisher school series title type url volume year label extra.label sort.label short.list INTEGERS output.state before.all mi...

  87. [95]

    write newline

    " write newline "" before.all 'output.state := FUNCTION add.period duplicate empty 'skip "." * add.blank if FUNCTION if.digit duplicate "0" = swap duplicate "1" = swap duplicate "2" = swap duplicate "3" = swap duplicate "4" = swap duplicate "5" = swap duplicate "6" = swap dupl...

  88. [96]

    , " * write output.state after.block = add.period write newline

    ENTRY address author booktitle chapter doi edition editor eid howpublished institution journal key month note number organization pages publisher school series title type url volume year label INTEGERS output.state before.all mid.sentence after.sentence after.block FUNCTION in...

  89. [97]

    write newline

    " write newline "" before.all 'output.state := FUNCTION if.digit duplicate "0" = swap duplicate "1" = swap duplicate "2" = swap duplicate "3" = swap duplicate "4" = swap duplicate "5" = swap duplicate "6" = swap duplicate "7" = swap duplicate "8" = swap "9" = or or or or or or...

Pith tools

Reviewed August 12, 2026 · model on record in the stance chip above.