William W. Zhang,1 Robert Petre,1 Andrew G. Peele,2 Keith Jahoda,1 F. E. Marshall,1 Yang Soong,3 Nicholas E. White1
1NASA Goddard Space Flight Ctr. (United States) 2National Research Council (United States) 3NASA Goddard Space Flight Ctr. and Universities' Space Research Association (United States)
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We present a conceptual design for a new x-ray all sky monitor (ASM). Compared with previous ASMs, its salient features are: (1) it has a focusing capability that increases the signal to background ratio by a factor of 3; (2) it has a broad-band width: 200 eV to 15 keV; (3) it has a large x-ray collection area: approximately 102 cm2; (4) it has a duty cycle of nearly 100%, and (5) it can measure the position of a new source with an accuracy of a few minutes of arc. These features combined open up an opportunity for discovering new phenomena as well as monitoring existing phenomena with unprecedented coverage and sensitivity.
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William W. Zhang, Robert Petre, Andrew G. Peele, Keith Jahoda, F. E. Marshall, Yang Soong, Nicholas E. White, "Broadband and large-area x-ray omni sky monitor (BLOSM)," Proc. SPIE 3114, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VIII, (15 October 1997); https://doi.org/10.1117/12.283787