X-ray astronomy 2000: Wide field X-ray monitoring with lobster-eye telescopes

Details X-ray astronomy 2000: Wide field X-ray monitoring with lobster-eye telescopes X-ray astronomy 2000: Wide field X-ray monitoring with lobster-eye telescopes

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..654i&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

Astronomy and Astrophysics

Astronomy

X-Ray Sources, X-Ray Bursts, X- And Gamma-Ray Sources, Mirrors, Gratings, And Detectors, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

The recently available first prototypes of innovative very wide field X-ray telescopes of Lobster-Eye type confirm the feasibility to develop such flight instruments in a near future. These devices are expected to allow very wide field (more than 1000 square degrees) monitoring of the sky in X-rays (up to 10 keV and perhaps even more) with faint limits. We will discuss the recent status of the development of very wide field X-ray telescopes as well as related scientific questions including expected major contributions such as monitoring and study of X-ray afterglows of Gamma Ray Bursts. .

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