{
  "id": "2007.03105",
  "version": "v1",
  "published": "2020-07-06T22:47:45.000Z",
  "updated": "2020-07-06T22:47:45.000Z",
  "title": "Multiwavelength Analysis of the Variability of the Blazar 3C 273",
  "authors": [
    "Sunil Fernandes",
    "Víctor M. Patiño-Álvarez",
    "Vahram Chavushyan",
    "Eric M. Schlegel",
    "José Ramón Valdés"
  ],
  "comment": "14 pages, 11 figures, 3 tables",
  "categories": [
    "astro-ph.HE",
    "astro-ph.GA"
  ],
  "abstract": "We present multiwavelength light curves and polarimetric data of the Flat Spectrum Radio Quasar 3C 273 over 8 years. The wavelength range of our data set extends from radio to gamma-rays. We found that the optical emission in this source is dominated by the accretion disk during the entire time-frame of study. We additionally find that in contrast with the observed behaviour in other blazars, 3C 273 does not show a correlation between the gamma-ray spectral index and the gamma-ray luminosity. Finally, we identified an anti-correlation between the 15 GHz and V-band light curves for the time-range $JD_{245} = 4860 - 5760$, which we speculate is the consequence of the inner part of the accretion disk falling into the black hole, followed by the ejection of a component into the jet.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-07-06T22:47:45.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "blazar 3c",
      "multiwavelength analysis",
      "flat spectrum radio quasar 3c",
      "accretion disk",
      "variability"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 14,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}