{"paper":{"title":"Multi-wavelength Temporal Variability of the Blazar 3C 454.3 during 2014 Activity Phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"2), 4), Alok C. Gupta (3, Brazil (3) ARIES, China (5) TIFR, India), India (2) IAG-USP, India (4) SAO, K. P. Singh (5) ((1) IUCAA, Mumbai, Nainital, Pankaj Kushwaha (1, Pune, Ranjeev Misra (1), Shanghai","submitted_at":"2016-09-22T13:10:15Z","abstract_excerpt":"We present a multi-wavelength temporal analysis of the blazar 3C 454.3 during the high $\\gamma$-ray active period from May-December, 2014. Except for X-rays, the period is well sampled at near-infrared (NIR)-optical by the \\emph{SMARTS} facility and the source is detected continuously on daily timescale in the \\emph{Fermi}-LAT $\\gamma$-ray band. The source exhibits diverse levels of variability with many flaring/active states in the continuously sampled $\\gamma$-ray light curve which are also reflected in the NIR-optical light curves and the sparsely sampled X-ray light curve by the \\emph{Swif"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.06952","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"}