Scientific Productivity with X-ray All-Sky Monitors

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dc.creatorRemillard, Ronald A.
dc.creatorLevine, Alan M.
dc.creatorMcClintock, Jeffrey E.
dc.date2009-03-18
dc.date.accessioned2026-07-07T12:53:38Z
dc.date.available2026-07-07T12:53:38Z
dc.descriptionWe outline scientific objectives for monitoring X-ray sources and transients with wide-angle, coded mask cameras. It is now possible to instantaneously view half of the sky over long time intervals, gaining access to events of extraordinary interest. Solid state detectors can raise the quality of data products for bright sources to levels associated with pointed instruments. There are diverse ways to advance high energy astrophysics and quantitative applications for general relativity.
dc.description7 pages, 2 figures, white paper for NASA Astronomy & Astrophysics Decadal Survey 2010
dc.identifierhttps://arxiv.org/abs/0903.3195
dc.identifierhttp://arxiv.org/abs/0903.3195
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223688
dc.subjectHigh Energy Astrophysical Phenomena
dc.subjectInstrumentation and Methods for Astrophysics
dc.titleScientific Productivity with X-ray All-Sky Monitors
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