Paper
15 October 1997 Broadband and large-area x-ray omni sky monitor (BLOSM)
William W. Zhang, Robert Petre, Andrew G. Peele, Keith Jahoda, F. E. Marshall, Yang Soong, Nicholas E. White
Author Affiliations +
Abstract
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.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
William W. Zhang, Robert Petre, Andrew G. Peele, Keith Jahoda, F. E. Marshall, Yang Soong, and 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
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Cited by 1 scholarly publication.
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KEYWORDS
X-rays

Reflectors

Sensors

Gamma radiation

Satellites

Glasses

Sun

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