X-Ray Monitoring of GRBs with Lobster Eye Telescopes

Details X-Ray Monitoring of GRBs with Lobster Eye Telescopes X-Ray Monitoring of GRBs with Lobster Eye Telescopes

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..712s&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 712-718 (2004).

Computer Science

Databases

Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray Sources, X-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

We present here the soft X-ray All-Sky Monitor (ASM). It is based on the current technological capabilities, sensitive in the ~ 0.1 - 10.0 keV range with angular resolution of ~ 3 - 4 arcmin, and has a limiting detectable flux ~ 10-12 erg/s/cm2 for daily scans in the mentioned energy range. The ASM will play a key role in studying transient X-ray sources like XRBs, GRBs, XRFs, X-ray novae, as well as in the study of the long term variability of X-ray sources like XRBs, AGN, or stellar X-ray flares.

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