{"paper":{"title":"A time dependent approach to model X-ray and $\\gamma$--ray light curves of Mrk 421 observed during the flare in February 2010","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A Goyal, A K Tickoo, A Sinha, C K Bhat, H C Goyal, K Chanchalani, K K Singh, K K Yadav, K Venugopal, M K Koul, M Kothari, N Bhatt, N Chouhan, N K Agarwal, N Kumar, P Chandra, P Marandi, R C Rannot, R Koul, S Sahayanathan, V K Dhar","submitted_at":"2017-01-06T07:04:32Z","abstract_excerpt":"Strong X-ray and $\\gamma$--ray flares have been detected in February 2010 from the high synchrotron peaked blazar Mrk 421 (z=0.031). With the motivation of understanding the physics involved in this flaring activity, we study the variability of the source in X-ray and $\\gamma$--ray energy bands during the period February 10-23, 2010 (MJD 55237-55250). We use near simultaneous X-ray data collected by \\emph{MAXI}, \\emph{Swift}-XRT and $\\gamma$--ray data collected by \\emph{Fermi}-LAT and \\emph{TACTIC} along with the optical V-band observations by \\emph{SPOL} at Steward Observatory. We observe tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01557","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}