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相关论文: Hard X-ray Timing with EXIST

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The Energetic X-ray Imaging Survey Telescope (EXIST) is under study for the proposed Black Hole Finder Probe, one of the three Einstein Probe missions in NASA's proposed Beyond Einstein Program. EXIST would have unique capabilities: it…

天体物理学 · 物理学 2009-11-13 Jonathan E. Grindlay

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…

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

EXIST is being studied as the Black Hole Finder Probe, one of the 3 Einstein Probe missions under NASA's Beyond Einstein program. The major science goals for EXIST include highly sensitive full-sky hard X-ray survey in a very wide energy…

天体物理学 · 物理学 2015-06-24 S. V. Vadawale , J. Hong , J. E. Grindlay , G. Skinner

With its large collection area, broad-band energy coverage from optical/NIR (0.3 to 2.2 micron) to soft/hard X-ray (0.1-600 keV), all-sky monitoring capability, and on-board follow-up, the proposed Energetic X-ray Imaging Survey Telescope…

The hard x-ray (10-600 keV) sky is inherently time variable and yet has neither been surveyed nor monitored with a sensitive imaging telescope. The Energetic X-ray Imaging Survey Telescope (EXIST) is a mission concept, proposed for MIDEX,…

The Energetic X-ray Imaging Survey Telescope (EXIST) is designed to i) use the birth of stellar mass black holes, as revealed by cosmic Gamma-Ray Bursts (GRBs), as probes of the very first stars and galaxies to exist in the Universe. Both…

The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed next generation multi-wavelength survey mission. The primary instrument is a High Energy telescope (HET) that conducts the deepest survey for Gamma-ray Bursts (GRBs),…

天体物理仪器与方法 · 物理学 2015-05-14 J. Hong , J. E. Grindlay , B. Allen , S. D. Barthelmy , G. K. Skinner , N. Gehrels , the EXIST HET Working Group

The synergy of GLAST and the proposed EXIST mission as the Black Hole Finder Probe in the Beyond Einstein Program is remarkable. With its full-sky per orbit hard X-ray imaging (3-600 keV) and "nuFnu" sensitivity comparable to GLAST, EXIST…

天体物理学 · 物理学 2008-11-26 Jonathan E. Grindlay , the EXIST Team

We use semi-analytic techniques to evaluate the burst sensitivity of designs for the EXIST hard X-ray survey mission. Applying these techniques to the mission design proposed for the Beyond Einstein program, we find that with its very large…

The Energetic X-ray Imaging Survey Telescope (EXIST) mission concept is optimized for study of high-z GRBs as probes of the early Universe. With a High Energy Telescope (HET) incorporating a 4.5m^2 5-600keV (CZT; 0.6mm pixels) detector…

宇宙学与河外天体物理 · 物理学 2009-06-25 Jonathan Grindlay , the EXIST Team

The hard X-ray sky now being studied by INTEGRAL and Swift and soon by NuSTAR is rich with energetic phenomena and highly variable non-thermal phenomena on a broad range of timescales. The High Energy Telescope (HET) on the proposed…

A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. The proposed Energetic X-ray Imaging Survey Telescope, EXIST, would yield the limiting (practical) GRB trigger sensitivity, broad-band…

One of the few remaining astronomical bands (factor of $\sim$10 in energy range) still without an all-sky imaging survey is the hard x-ray band (10-600 keV). This is in spite of sensitive imaging all-sky surveys already conducted at soft…

天体物理学 · 物理学 2015-06-24 Jonathan E. Grindlay

The recent hard X-ray surveys performed by INTEGRAL and Swift have started to reveal the demographics of compact sources including Super-Massive Black Holes hosted in AGNs and have proven invaluable in tracking explosive events as the death…

天体物理仪器与方法 · 物理学 2010-02-08 Jonathan E. Grindlay , Lorenzo Natalucci , EXIST Team

The SXI telescope is one of the three instruments on board EXIST, a multiwavelength observatory in charge of performing a global survey of the sky in hard X-rays searching for Supermassive Black Holes. One of the primary objectives of EXIST…

The Soft X-ray Imager (SXI) is one of the three instruments on board EXIST, a multi-wavelength observatory in charge of performing a global survey of the sky in hard X-rays searching for Super-massive Black Holes (Grindlay & Natalucci,…

LOFT-P is a concept for a NASA Astrophysics Probe-Class (<$1B) X-ray timing mission, based on the LOFT concept originally proposed to ESAs M3 and M4 calls. LOFT-P requires very large collecting area (>6 m^2, >10x RXTE), high time…

eXTP is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism. Primary targets include isolated and binary neutron stars, strong magnetic field systems like magnetars, and…

天体物理仪器与方法 · 物理学 2020-03-17 S. N. Zhang , M. Feroci , A. Santangelo , Y. W. Dong , H. Feng , F. J. Lu , K. Nandra , Z. S. Wang , S. Zhang , E. Bozzo , S. Brandt , A. De Rosa , L. J. Gou , M. Hernanz , M. van der Klis , X. D. Li , Y. Liu , P. Orleanski , G. Pareschi , M. Pohl , J. Poutanen , J. L. Qu , S. Schanne , L. Stella , P. Uttley , A. Watts , R. X. Xu , W. F. Yu , J. J. M. in 't Zand , S. Zane , L. Alvarez , L. Amati , L. Baldini , C. Bambi , S. Basso , S. Bhattacharyya , R. Bellazzini , T. Belloni , P. Bellutti , S. Bianchi , A. Brez , M. Bursa , V. Burwitz , C. Budtz-Jorgensen , I. Caiazzo , R. Campana , X. L. Cao , P. Casella , C. Y. Chen , L. Chen , T. X. Chen , Y. Chen , Y. Chen , Y. P. Chen , M. Civitani , F. Coti Zelati , W. Cui , W. W. Cui , Z. G. Dai , E. Del Monte , D. De Martino , S. Di Cosimo , S. Diebold , M. Dovciak , I. Donnarumma , V. Doroshenko , P. Esposito , Y. Evangelista , Y. Favre , P. Friedrich , F. Fuschino , J. L. Galvez , Z. L. Gao , M. Y. Ge , O. Gevin , D. Goetz , D. W. Han , J. Heyl , J. Horak , W. Hu , F. Huang , Q. S. Huang , R. Hudec , D. Huppenkothen , G. L. Israel , A. Ingram , V. Karas , D. Karelin , P. A. Jenke , L. Ji , T. Kennedy , S. Korpela , D. Kunneriath , C. Labanti , G. Li , X. Li , Z. S. Li , E. W. Liang , O. Limousin , L. Lin , Z. X. Ling , H. B. Liu , H. W. Liu , Z. Liu , B. Lu , N. Lund , D. Lai , B. Luo , T. Luo , B. Ma , S. Mahmoodifar , M. Marisaldi , A. Martindale , N. Meidinger , Y. P. Men , M. Michalska , R. Mignani , M. Minuti , S. Motta , F. Muleri , J. Neilsen , M. Orlandini , A T. Pan , A. Patruno , E. Perinati , A. Picciotto , C. Piemonte , M. Pinchera , A. Rachevski , M. Rapisarda , N. Rea , E. M. R. Rossi , A. Rubini , G. Sala , X. W. Shu , C. Sgro , Z. X. Shen , P. Soffitta , L. M. Song , G. Spandre , G. Stratta , T. E. Strohmayer , L. Sun , J. Svoboda , G. Tagliaferri , C. Tenzer , H. Tong , R. Taverna , G. Torok , R. Turolla , A. Vacchi , J. Wang , J. X. Wang , D. Walton , K. Wang , J. F. Wang , R. J. Wang , Y. F. Wang , S. S. Weng , J. Wilms , B. Winter , X. Wu , X. F. Wu , S. L. Xiong , Y. P. Xu , Y. Q. Xue , Z. Yan , S. Yang , X. Yang , Y. J. Yang , F. Yuan , W. M. Yuan , Y. F. Yuan , G. Zampa , N. Zampa , A. Zdziarski , C. Zhang , C. L. Zhang , L. Zhang , X. Zhang , Z. Zhang , W. D. Zhang , S. J. Zheng , P. Zhou , X. L. Zhou

Several payloads for hard X-ray (20-600 keV) imaging with coded aperture telescopes have been developed for balloon flight observations of cosmic x-ray sources. We briefly review the characteristics of these, particularly the EXITE2 system.…

天体物理学 · 物理学 2009-10-30 Jonathan E. Grindlay
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