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High–Energy Astrophysics with Lobster Eye X-ray ASM

Published online by Cambridge University Press:  12 May 2006

R. Hudec ,
V. Simon ,
L. Sveda ,
L. Pina  and
A. Inneman
R. Hudec
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ–251 65 Ondrejov, Czech Republic email: rhudec@asu.cas.cz
V. Simon
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ–251 65 Ondrejov, Czech Republic email: rhudec@asu.cas.cz
L. Sveda
Affiliation:
Czech Technical University, Faculty of Nuclear Physics, Prague, Czech Republic
L. Pina
Affiliation:
Czech Technical University, Faculty of Nuclear Physics, Prague, Czech Republic
A. Inneman
Affiliation:
Center for Advanced X-ray Technologies, Reflex sro, Prague, Czech Republic
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Abstract

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We report on astrophysical aspects of fully innovative very wide–field X-ray telescopes with high sensitivity. They are expected to contribute essentially to study of various astrophysical objects such as AGN, SNe, Gamma-ray bursts (GRBs), X-ray flashes (XRFs), galactic binary sources, stars, CVs, X-ray novae, various transient sources, etc.

Keywords

X-ray telescopesAll-Sky Monitor
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 39 - 40
Copyright
2006 International Astronomical Union