ABSTRACT
We report on technical and astrophysical aspects of Lobster‐Eye wide‐field X‐ray telescopes expected to monitor the sky with high sensitivity and angular resolution of order of 1 arcmin. They will 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.
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