{ "id": "2008.09330", "version": "v1", "published": "2020-08-21T06:53:31.000Z", "updated": "2020-08-21T06:53:31.000Z", "title": "Temporal and Spectral Variability of OJ 287 before the April--June 2020 Outburst", "authors": [ "Nibedita Kalita", "Alok C. Gupta", "Minfeng Gu" ], "comment": "11 pages, 4 figures, published in the special issue \"X-Ray Flux and Spectral Variability of Blazars\" of Galaxies journal", "journal": "Galaxies 2020, 8, 58", "doi": "10.3390/galaxies8030058", "categories": [ "astro-ph.HE" ], "abstract": "We present the results of a temporal and spectral study of the BL Lacertae object OJ 287 in optical, UV, and X-ray bands with observations performed by Swift satellite during September 2019--March 2020. In this period, the source showed moderate variability characterized by variability amplitude of $\\sim$22--31% in all the wavelengths on a short timescale, except the hard X-ray band which was variable by only $\\sim$8%. We observed that the X-ray flux of the source was significantly dominated by the soft photons below $2$ keV. Soft lags of $\\sim$45 days were detected between the optical/UV and soft X-ray emissions, while there is no correlation between the hard X-rays and the lower energy bands indicating the presence of two emission components or electron populations. Although two components contribute to the X-ray emission, most of the 0.3--10 keV spectra were well fitted with an absorbed power-law model which outlines the dominance of synchrotron over inverse Compton (IC) mechanism. The X-ray spectra follow a weak \"softer when brighter\" trend.", "revisions": [ { "version": "v1", "updated": "2020-08-21T06:53:31.000Z" } ], "analyses": { "keywords": [ "spectral variability", "bl lacertae object oj", "april-june", "lower energy bands", "hard x-ray band" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }