Statistics – Applications
Scientific paper
Mar 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.3708r&link_type=abstract
American Astronomical Society, HEAD meeting #10, #37.08
Statistics
Applications
Scientific paper
The Advanced X-ray Timing Array (AXTAR) is an X-ray observatory combining very large collecting area, broadband spectral coverage, high time resolution, highly flexible scheduling, and an ability to respond promptly to time-critical targets of opportunity. It is optimized for submillisecond timing of bright Galactic X-ray sources in order to study phenomena at the natural time scales of neutron star surfaces and black hole event horizons, thus probing the physics of ultradense matter, strongly curved spacetimes, and intense magnetic fields. AXTAR's main instrument, the Large Area Timing Array (LATA), is a collimated, thick Si pixel detector with 2-50 keV coverage and 8 m2 collecting area. Key features of the LATA include: 1 µs absolute time accuracy, 600 eV energy resolution, and minimal deadtime even on sources as bright as Sco X-1. For timing observations of accreting neutron stars and black holes, AXTAR provides at least an order of magnitude improvement in sensitivity over both the Rossi X-ray Timing Explorer (RXTE) and Constellation-X. A sensitive Sky Monitor acts as a trigger for pointed observations of X-ray transients and also provides continuous monitoring of the X-ray sky with 20 times the sensitivity of the RXTE ASM and a source localization accuracy of 1 arcmin. The baseline mission concept builds on detector and electronics technology previously developed for other applications with support from NASA, DOE, DARPA, and DHS, and thus offers high scientific impact at moderate, known cost and minimal technical risk.
AXTAR Collaboration
Chakrabarty Deepto
Ray Paul Shelton
Strohmayer T.,
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