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The High Energy X-ray telescope (HE) on-board the Hard X-ray Modulation Telescope (\textit{Insight}-HXMT) can serve as a wide Field of View (FOV) gamma-ray monitor with high time resolution ($\mu$s) and large effective area (up to thousands…

Despite the impressive progresses achieved both by X-ray and gamma-ray observatories in the last decades, the energy range between $\sim 200\,\mathrm{keV}$ and $\sim 50\,\mathrm{MeV}$ remains poorly explored. COMPTEL, on-board CGRO…

天体物理仪器与方法 · 物理学 2022-08-10 Giulio Lucchetta

The Hard X-ray Modulation Telescope ($Insight$-HXMT) was successfully launched on June 15th, 2017. It performs broad band X-ray scan survey of the Galactic Plane to detect new black holes and other objects in active states. It also observes…

天体物理仪器与方法 · 物理学 2022-01-03 S. M. Jia , X. Ma , Y. Huang , W. Z. Zhang , G. Ou , L. M. Song , J. L. Qu , S. Zhang , L. Chen

Extended results on the cosmic-ray electron + positron spectrum from 11 GeV to 4.8 TeV are presented based on observations with the Calorimetric Electron Telescope (CALET) on the International Space Station utilizing the data up to November…

The high-frequency-peaked BL Lacertae object 1ES 0229+200 is a relatively distant (z = 0.1396), hard-spectrum (Gamma ~ 2.5), very-high-energy-emitting (E > 100 GeV) gamma-ray blazar. Very-high-energy measurements of this active galactic…

The Nuclear Compton Telescope (NCT) is a balloon-borne Compton telescope designed for the study of astrophysical sources in the soft gamma-ray regime (200 keV--20 MeV). NCT's ten high-purity germanium crossed-strip detectors measure the…

The detection of the high-frequency peaked BL Lac object (HBL) SHBL J001355.9-185406 ($z$=0.095) at high (HE; 100 MeV$<$E$<$300 GeV) and very high-energy (VHE; $E>100\,{\rm GeV}$) with the \fer\ Large Area Telescope (LAT) and the High…

高能天体物理现象 · 物理学 2013-11-19 H. E. S. S. Collaboration , : , A. Abramowski , F. Acero , F. Aharonian , A. G. Akhperjanian , E. Angüner , G. Anton , S. Balenderan , A. Balzer , A. Barnacka , Y. Becherini , J. Becker Tjus , K. Bernlöhr , E. Birsin , E. Bissaldi , J. Biteau , C. Boisson , J. Bolmont , P. Bordas , J. Brucker , F. Brun , P. Brun , T. Bulik , S. Carrigan , S. Casanova , M. Cerruti , P. M. Chadwick , R. Chalme-Calvet , R. C. G. Chaves , A. Cheesebrough , M. Chrétien , S. Colafrancesco , G. Cologna , J. Conrad , C. Couturier , M. Dalton , M. K. Daniel , I. D. Davids , B. Degrange , C. Deil , P. deWilt , H. J. Dickinson , A. Djannati-Ataï , W. Domainko , L. O'C. Drury , G. Dubus , K. Dutson , J. Dyks , M. Dyrda , T. Edwards , K. Egberts , P. Eger , P. Espigat , C. Farnier , S. Fegan , F. Feinstein , M. V. Fernandes , D. Fernandez , A. Fiasson , G. Fontaine , A. Förster , M. Füßling , M. Gajdus , Y. A. Gallant , T. Garrigoux , H. Gast , B. Giebels , J. F. Glicenstein , D. Göring , M. -H. Grondin , M. Grudzińska , S. Häffner , J. D. Hague , J. Hahn , J. Harris , G. Heinzelmann , G. Henri , G. Hermann , O. Hervet , A. Hillert , J. A. Hinton , W. Hofmann , P. Hofverberg , M. Holler , D. Horns , A. Jacholkowska , C. Jahn , M. Jamrozy , M. Janiak , F. Jankowsky , I. Jung , M. A. Kastendieck , K. Katarzyński , U. Katz , S. Kaufmann , B. Khélifi , M. Kieffer , S. Klepser , D. Klochkov , W. Kluźniak , T. Kneiske , D. Kolitzus , Nu. Komin , K. Kosack , S. Krakau , F. Krayzel , P. P. Krüger , H. Laffon , G. Lamanna , J. Lefaucheur , M. Lemoine-Goumard , J. -P. Lenain , D. Lennarz , T. Lohse , A. Lopatin , C. -C. Lu , V. Marandon , A. Marcowith , G. Maurin , N. Maxted , M. Mayer , T. J. L. McComb , M. C. Medina , J. Méhault , U. Menzler , M. Meyer , R. Moderski , M. Mohamed , E. Moulin , T. Murach , C. L. Naumann , M. de Naurois , D. Nedbal , J. Niemiec , S. J. Nolan , L. Oakes , S. Ohm , E. de Oña Wilhelmi , B. Opitz , M. Ostrowski , I. Oya , M. Panter , R. D. Parsons , M. Paz Arribas , N. W. Pekeur , G. Pelletier , J. Perez , P. -O. Petrucci , B. Peyaud , S. Pita , H. Poon , G. Pühlhofer , M. Punch , A. Quirrenbach , S. Raab , M. Raue , A. Reimer , O. Reimer , M. Renaud , R. de los Reyes , F. Rieger , L. Rob , S. Rosier-Lees , G. Rowell , B. Rudak , C. B. Rulten , V. Sahakian , D. A. Sanchez , A. Santangelo , R. Schlickeiser , F. Schüssler , A. Schulz , U. Schwanke , S. Schwarzburg , S. Schwemmer , H. Sol , G. Spengler , F. Spieß , Ł. Stawarz , R. Steenkamp , C. Stegmann , F. Stinzing , K. Stycz , I. Sushch , A. Szostek , J. -P. Tavernet , R. Terrier , M. Tluczykont , C. Trichard , K. Valerius , C. van Eldik , G. Vasileiadis , C. Venter , A. Viana , P. Vincent , H. J. Völk , F. Volpe , M. Vorster , S. J. Wagner , P. Wagner , M. Ward , M. Weidinger , R. White , A. Wierzcholska , P. Willmann , A. Wörnlein , D. Wouters , M. Zacharias , A. Zajczyk , A. A. Zdziarski , A. Zech , H. -S. Zechlin

The All-Sky Monitor on the Rossi X-ray Timing Explorer has been monitoring the sky in the 1.5 - 12 keV band since late February. The instrument consists of three coded-aperture cameras which can be rotated to view different regions by a…

The Infra-Red Telescope (IRT) on board the Transient High Energy Sky and Early Universe Surveyor (THESEUS) ESA M5 candidate mission will play a key role in identifying and characterizing moderate to high redshift Gamma-Ray Bursts…

In the past few decades, X-ray astronomy satellites equipped with grating spectrometers and microcalorimeters have enabled high-resolution spectroscopic observations of astrophysical objects. The need for accurate atomic data has arose as…

The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture telescope array, incorporating 8m^2 of pixellated Cd-Zn-Te (CZT) detectors, to conduct a full-sky imaging and temporal hard x-ray (10-600 keV)…

天体物理学 · 物理学 2009-11-07 J. E. Grindlay , W. W. Craig , N. Gehrels , F. A. Harrison , J. Hong

During 1997, the BL Lac object Mkn 501 went into an extraordinary state of high X-ray and TeV gamma-ray activity, lasting more than 6 months. In this paper we report on the TeV emission characteristics of the source in the subsequent years…

天体物理学 · 物理学 2018-04-18 The HEGRA Collaboration , F. Aharonian , A. Akhperjanian , J. Barrio

A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and medium (ABRIXAS2) x-ray surveys into the 10-100 keV band (and beyond) at comparable sensitivity (~0.05 mCrab). This would enable discovery…

Sharjah-Sat-1 is a 3U cubesat with a CdZnTe based hard X-ray detector, called iXRD (improved X-ray Detector) as a scientific payload with the primary objective of monitoring bright X-ray sources in the galaxy. We investigated the effects of…

仪器与探测器 · 物理学 2023-01-10 Ali M. Altingun , Emrah Kalemci , Efe Oztaban

The Solar X-ray Monitor (abbreviated as XSM) on board India's Chandrayaan-2 mission is designed to carry out broadband spectroscopy of the Sun from lunar orbit. It observes the Sun as a star and measures the spectrum every second in the…

The Lunar Electromagnetic Monitor in X-rays (LEM-X) is a proposed wide-field X-ray observatory designed for deployment on the Moon's surface. Its primary scientific goal is to enhance multi-messenger astrophysics by detecting, localizing,…

LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the…

天体物理仪器与方法 · 物理学 2024-06-08 T. Ghigna , A. Adler , K. Aizawa , H. Akamatsu , R. Akizawa , E. Allys , A. Anand , J. Aumont , J. Austermann , S. Azzoni , C. Baccigalupi , M. Ballardini , A. J. Banday , R. B. Barreiro , N. Bartolo , S. Basak , A. Basyrov , S. Beckman , M. Bersanelli , M. Bortolami , F. Bouchet , T. Brinckmann , P. Campeti , E. Carinos , A. Carones , F. J. Casas , K. Cheung , Y. Chinone , L. Clermont , F. Columbro , A. Coppolecchia , D. Curtis , P. de Bernardis , T. de Haan , E. de la Hoz , M. De Petris , S. Della Torre , G. Delle Monache , E. Di Giorgi , C. Dickinson , P. Diego-Palazuelos , J. J. Díaz García , M. Dobbs , T. Dotani , G. D'Alessandro , H. K. Eriksen , J. Errard , T. Essinger-Hileman , N. Farias , E. Ferreira , C. Franceschet , U. Fuskeland , G. Galloni , M. Galloway , K. Ganga , M. Gerbino , M. Gervasi , R. T. Génova-Santos , S. Giardiello , C. Gimeno-Amo , E. Gjerløw , R. González González , L. Grandsire , A. Gruppuso , N. W. Halverson , P. Hargrave , S. E. Harper , M. Hazumi , S. Henrot-Versillé , L. T. Hergt , D. Herranz , E. Hivon , R. A. Hlozek , T. D. Hoang , J. Hubmayr , K. Ichiki , K. Ikuma , H. Ishino , G. Jaehnig , B. Jost , K. Kohri , K. Konishi , L. Lamagna , M. Lattanzi , C. Leloup , F. Levrier , A. I. Lonappan , G. Luzzi , J. Macias-Perez , B. Maffei , E. Marchitelli , E. Martínez-González , S. Masi , S. Matarrese , T. Matsumura , S. Micheli , M. Migliaccio , M. Monelli , L. Montier , G. Morgante , L. Mousset , Y. Nagano , R. Nagata , P. Natoli , A. Novelli , F. Noviello , I. Obata , A. Occhiuzzi , K. Odagiri , R. Omae , L. Pagano , A. Paiella , D. Paoletti , G. Pascual-Cisneros , G. Patanchon , V. Pavlidou , F. Piacentini , M. Piat , G. Piccirilli , M. Pinchera , G. Pisano , L. Porcelli , N. Raffuzzi , C. Raum , M. Remazeilles , A. Ritacco , J. Rubino-Martin , M. Ruiz-Granda , Y. Sakurai , G. Savini , D. Scott , Y. Sekimoto , M. Shiraishi , G. Signorelli , S. L. Stever , R. M. Sullivan , A. Suzuki , R. Takaku , H. Takakura , S. Takakura , Y. Takase. A. Tartari , K. Tassis , K. L. Thompson , M. Tomasi , M. Tristram , C. Tucker , L. Vacher , B. van Tent , P. Vielva , K. Watanuki , I. K. Wehus , B. Westbrook , G. Weymann-Despres , B. Winter , E. J. Wollack , A. Zacchei , M. Zannoni , Y. Zhou , the LiteBIRD Collaboration

ESA's hard X-ray and soft gamma-ray observatory INTEGRAL is covering the 3 keV to 10 MeV energy band, with excellent sensitivity during long and uninterrupted observations of a large field of view (~100 square degrees), with ms time…

高能天体物理现象 · 物理学 2011-10-31 Christoph Winkler , Roland Diehl , Pietro Ubertini , Jörn Wilms

Observations of the Crab Nebula at 850 micron made with the "Submillimetre Common-User Bolometer Array" (SCUBA) on the James Clerk Maxwell Telescope are presented. A variety of chop-throws and scanning directions was used in these…

天体物理学 · 物理学 2007-05-23 D. A. Green

We report on the construction, operation experience, and preliminary background measurements of an InGrid detector, i.e. a MicroMegas detector with CMOS pixel readout. The detector was mounted in the focal plane of the Abrixas X-Ray…

仪器与探测器 · 物理学 2015-09-07 Klaus Desch , Jochen Kaminski , Christoph Krieger , Michael Lupberger
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