{"paper":{"title":"Evidence for two Lognormal States in Multi-wavelength Flux Variation of FSRQ PKS 1510-089","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"(2) TIFR, 5), (5) IAG-USP, Ahmedabad, Brazil), India, K. P. Singh (2), K. S. Baliyan (4) ((1) IUCAA, Mumbai (3) BARC, Mumbai (4) PRL, Pankaj Kushwaha (1, Pune, Ranjeev Misra (1), S. Sahayanathan (3), Sunil Chandra (2)","submitted_at":"2016-04-15T02:20:13Z","abstract_excerpt":"We present a systematic characterization of multi-wavelength emission from blazar PKS 1510-089 using well-sampled data at infrared(IR)-optical, X-ray and $\\gamma$-ray energies. The resulting flux distributions, except at X-rays, show two distinct lognormal profiles corresponding to a high and a low flux level. The dispersions exhibit energy dependent behavior except for the LAT $\\gamma$-ray and optical B-band. During the low level flux states, it is higher towards the peak of the spectral energy distribution, with $\\gamma$-ray being intrinsically more variable followed by IR and then optical, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.04335","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"}