Proposed (to) EXIST: Hard X-ray Imaging All Sky Survey/Monitor
| dc.creator | Grindlay, J. E. | |
| dc.creator | Prince, T. A. | |
| dc.creator | Harrison, F. | |
| dc.creator | Gehrels, N. | |
| dc.creator | Hailey, C. J. | |
| dc.creator | Ramsey, B. | |
| dc.creator | Weisskopf, M. C. | |
| dc.creator | Skinner, G. K. | |
| dc.creator | Ubertini, P. | |
| dc.date | 1998-01-01 | |
| dc.date.accessioned | 2026-07-07T02:25:42Z | |
| dc.date.available | 2026-07-07T02:25:42Z | |
| dc.description | 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, which would conduct the first imaging all-sky hard x-ray survey as well as provide a sensitive all sky monitor. With $\sim 60%$ sky coverage each orbit, and full sky coverage each 50 days, hard x-ray studies of gamma-ray bursts, AGN, galactic transients, x-ray binaries and accretion-powered pulsars can be conducted over a wide range of timescales. We summarize the scientific objectives of EXIST for both the survey and monitoring objectives. We describe the mission concept and the instrumentation approach, which would incorporate a large area array of Cd-Zn-Te (CZT) detectors, as well as some of our ongoing development of CZT array detectors. | |
| dc.description | 6 pages latex (needs RIKEN2A.sty, WORKSHOP.sty and psbox.sty) plus 3 postscript figures. Invited talk presented at Riken Workshop on All Sky Monitors; to be published in "All Sky X-ray Observations in the Next Decade" (eds. M. Matsuoka and N. Kawai), 1998 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9712359 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9712359 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11980 | |
| dc.subject | Astrophysics | |
| dc.title | Proposed (to) EXIST: Hard X-ray Imaging All Sky Survey/Monitor | |
| dc.type | text |