X-ray emission study of extreme blazars using AstroSat
dc.contributor.author | Goswami, P. | |
dc.contributor.author | Sinha, A. | |
dc.contributor.author | Mankuzhiyil, N. | |
dc.contributor.author | Sahayanathan, S. | |
dc.date.accessioned | 2024-08-13T10:49:37Z | |
dc.date.available | 2024-08-13T10:49:37Z | |
dc.date.issued | 2022 | |
dc.description.division | ApSD | en |
dc.format.extent | 4611 bytes | |
dc.format.mimetype | text/html | |
dc.identifier.source | Proceedings of Science, 2022. Vol. 395: Article no. 961 | en |
dc.identifier.uri | http://hdl.handle.net/123456789/27127 | |
dc.language.iso | en | en |
dc.subject | X-ray emission study | en |
dc.subject | extreme blazars | en |
dc.subject | AstroSat | en |
dc.subject | synchrotron peak energy | en |
dc.title | X-ray emission study of extreme blazars using AstroSat | en |
dc.type | Article | en |