Abstract
According to the observational statistics a large majority of all GRBs exhibit X‐ray emission. In addition, a dedicated separate group of GRB, the XRFs, exists which emission dominates in the X‐ray spectral range. And the third group of GRB related objects (yet hypothetical) are the group of off‐axis observed GRBs (orphan afterglows). These facts justify the consideration of an independent experiment for monitoring, detection and analyses of GRBs and others fast X‐ray transients in X‐rays. We will present and discuss such experiment based on wide‐field X‐ray telescopes of Lobster Eye type. The wide field and fine sensitivity of Lobster Eye X‐ray All‐Sky Monitor make such instruments important tools in study of GRBs and related objects.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.