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Related papers: CZT in Space Based Hard-X-ray Astronomy

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The High Energy Cosmic-Radiation Detection (HERD) facility has been proposed as a leading experiment on China's Space Station (CSS). Scheduled for installation around 2027, HERD is expected to operate for at least a decade. The main…

High Energy Astrophysical Phenomena · Physics 2025-04-18 Keerthana Rajan Lathika

Cadmium zinc telluride (CdZnTe, CZT) radiation detectors are suitable for a variety of applications, due to their high spatial resolution and spectroscopic energy performance at room temperature. However, state-of-the-art detector systems…

Instrumentation and Detectors · Physics 2016-10-13 P. Födisch , M. Berthel , B. Lange , T. Kirschke , W. Enghardt , P. Kaever

We have modelled the hard X-ray background expected for a high-altitude balloon flight of the Energetic X-ray Telescope Experiment (EXITE2), an imaging phoswich detector/telescope for the 20--600 keV energy range. Photon and neutron-induced…

The CRESST experiment monitors 300g CaWO_4 crystals as targets for particle interactions in an ultra low background environment. In this paper, we analyze the background spectra that are recorded by three detectors over many weeks of data…

The Modified Horizontal Bridgman (MHB) process produces Cadmium Zinc Telluride (CZT) crystals with high yield and excellent homogeneity. Various groups,including our own, previously reported on the test of 2x2x0.5 cm3 MHB CZT detectors…

Rare event search experiments using germanium detectors are operated in underground laboratories to minimize the background induced by cosmic rays. However, the cosmogenic activation in germanium crystals on the ground during fabrication…

Instrumentation and Detectors · Physics 2024-03-08 Qiyuan Nie , Zhi Zeng , Hao Ma , Litao Yang , Qian Yue , Jianping Cheng

For several decades now, wide-field coded mask cameras have been used with success to localise Gamma-ray bursts (GRBs). In these instruments, the event count rate is dominated by the photon background due to their large field of view and…

Instrumentation and Methods for Astrophysics · Physics 2015-05-13 O. Godet , P. Sizun , D. Barret , P. Mandrou , B. Cordier , S. Schanne , N. Remoue

The hot and dense medium produced in relativistic heavy-ion collisions has been conjectured to be accompanied by an axial charge asymmetry that may lead to a separation of electric charges in the direction of the extremely strong magnetic…

Nuclear Experiment · Physics 2022-02-16 Yu Hu

The Soft Gamma-ray Detector (SGD) on board the NeXT (Japanese future high energy astrophysics mission) is a Compton telescope with narrow field of view (FOV), which utilizes Compton kinematics to enhance its background rejection…

Cosmic-ray background fluxes were modeled based on existing measurements and theories and are presented here. The model, originally developed for the Gamma-ray Large Area Space Telescope (GLAST) Balloon Experiment, covers the entire solid…

Astrophysics · Physics 2009-11-10 T. Mizuno , T. Kamae , G. Godfrey , T. Handa , D. J. Thompson , D. Lauben , Y. Fukazawa , M. Ozaki

We present new constraints on the cosmic ray electron boosted light dark matter (CReDM) using the 205.4 kg$\cdot$day data of the CDEX-10 experiment located at the China Jinping Underground Laboratory. The cosmic ray electron spectrum and…

The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. The large mass and proximity of the cryostat to the active…

Instrumentation and Detectors · Physics 2017-09-28 D. S. Akerib , C. W. Akerlof , D. Yu. Akimov , S. K. Alsum , H. M. Araújo , I. J. Arnquist , M. Arthurs , X. Bai , A. J. Bailey , J. Balajthy , S. Balashov , M. J. Barry , J. Belle , P. Beltrame , T. Benson , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , K. E. Boast , A. Bolozdynya , B. Boxer , R. Bramante , P. Brás , J. H. Buckley , V. V. Bugaev , R. Bunker , S. Burdin , J. K. Busenitz , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , C. Chan , J. J. Cherwinka , A. A. Chiller , C. Chiller , A. Cottle , R. Coughlen , W. W. Craddock , A. Currie , C. E. Dahl , T. J. R. Davison , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , T. K. Edberg , W. R. Edwards , W. T. Emmet , C. H. Faham , S. Fiorucci , T. Fruth , R. J. Gaitskell , N. J. Gantos , V. M. Gehman , R. M. Gerhard , C. Ghag , M. G. D. Gilchriese , B. Gomber , C. R. Hall , S. Hans , K. Hanzel , S. J. Haselschwardt , S. A. Hertel , S. Hillbrand , C. Hjemfelt , M. D. Hoff , B. Holbrook , E. Holtom , E. W. Hoppe , J. Y-K. Hor , M. Horn , D. Q. Huang , T. W. Hurteau , C. M. Ignarra , R. G. Jacobsen , W. Ji , A. Kaboth , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , A. V. Khromov , A. M. Konovalov , E. V. Korolkova , M. Koyuncu , H. Kraus , H. J. Krebs , V. A. Kudryavtsev , A. V. Kumpan , S. Kyre , C. Lee , H. S. Lee , J. Lee , D. S. Leonard , R. Leonard , K. T. Lesko , C. Levy , F. -T. Liao , J. Lin , A. Lindote , R. E. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , B. Lopez Paredes , W. Lorenzon , S. Luitz , P. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , D. J. Markley , T. J. Martin , M. F. Marzioni , C. T. McConnell , D. N. McKinsey , D. -M. Mei , Y. Meng , E. H. Miller , E. Mizrachi , J. Mock , M. E. Monzani , J. A. Morad , B. J. Mount , A. St. J. Murphy , C. Nehrkorn , H. N. Nelson , F. Neves , J. A. Nikkel , J. O'Dell , K. O'Sullivan , I. Olcina , M. A. Olevitch , K. C. Oliver-Mallory , K. J. Palladino , E. K. Pease , A. Piepke , S. Powell , R. M. Preece , K. Pushkin , B. N. Ratcliff , J. Reichenbacher , L. Reichhart , C. A. Rhyne , A. Richards , J. P. Rodrigues , H. J. Rose , R. Rosero , P. Rossiter , J. S. Saba , M. Sarychev , R. W. Schnee , M. Schubnell , P. R. Scovell , S. Shaw , T. A. Shutt , C. Silva , K. Skarpaas , W. Skulski , M. Solmaz , V. N. Solovov , P. Sorensen , V. V. Sosnovtsev , I. Stancu , M. R. Stark , S. Stephenson , T. M. Stiegler , K. Stifter , T. J. Sumner , M. Szydagis , D. J. Taylor , W. C. Taylor , D. Temples , P. A. Terman , K. J. Thomas , J. A. Thomson , D. R. Tiedt , M. Timalsina , W. H. To , A. Tomás , T. E. Tope , M. Tripathi , L. Tvrznikova , J. Va'vra , A. Vacheret , M. G. D. van der Grinten , J. R. Verbus , C. O. Vuosalo , W. L. Waldron , R. Wang , R. Watson , R. C. Webb , W. -Z. Wei , M. While , D. T. White , T. J. Whitis , W. J. Wisniewski , M. S. Witherell , F. L. H. Wolfs , D. Woodward , S. Worm , J. Xu , M. Yeh , J. Yin , C. Zhang

X-ray and Gamma-ray polarization measurements of the prompt emission of Gamma-ray bursts (GRBs) are believed to be extremely important for testing various models of GRBs. So far, the available measurements of hard X-ray polarization of GRB…

The proposed Daksha mission comprises of a pair of highly sensitive space telescopes for detecting and characterising high-energy transients such as electromagnetic counterparts of gravitational wave events and gamma-ray bursts (GRBs).…

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…

Instrumentation and Methods for Astrophysics · Physics 2024-11-20 Vincent Tatischeff , Philippe Laurent

A future mission in medium-energy gamma-ray astrophysics would allow for many scientific advancements, e.g. a possible explanation for the excess positron emission from the Galactic Center, a better understanding of nucleosynthesis and…

Instrumentation and Methods for Astrophysics · Physics 2018-06-20 Michelle Galloway , Andreas Zoglauer , Steven E. Boggs , Mark Amman

As part of the T-REX project, a number of R&D and prototyping activities have been carried out during the last years to explore the applicability of Micromegas-read gaseous TPCs in rare event searches like double beta decay (DBD), axion…

We have assembled a tiled array (220 cm2) of fine pixel (0.6 mm) imaging CZT detectors for a balloon borne wide-field hard X-ray telescope, ProtoEXIST2. ProtoEXIST2 is a prototype experiment for a next generation hard X-ray imager MIRAX-HXI…

Instrumentation and Methods for Astrophysics · Physics 2016-10-26 Jaesub Hong , Branden Allen , Jonathan Grindlay , Barbara Rodrigues , Jon Robert Ellis , Robert Baker , Scott Barthelmy , Peter Mao , Hiromasa Miyasaka , Jeff Apple

The sensitivity of astronomical X-ray detectors is limited by the instrumental background. The background is especially important when observing low surface brightness sources that are critical for many of the science cases targeted by…

Instrumentation and Methods for Astrophysics · Physics 2022-08-18 D. R. Wilkins , S. W. Allen , E. D. Miller , M. Bautz , T. Chattopadhyay , R. Foster , C. E. Grant , S. Hermann , R. Kraft , R. G. Morris , P. Nulsen , G. Schellenberger
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