{ "id": "1602.04180", "version": "v1", "published": "2016-02-12T19:31:55.000Z", "updated": "2016-02-12T19:31:55.000Z", "title": "INTEGRAL upper limits on gamma-ray emission associated with the gravitational wave event GW150914", "authors": [ "V. Savchenko", "C. Ferrigno", "S. Mereghetti", "L. Natalucci", "A. Bazzano", "E. Bozzo", "T. J. -L. Courvoisier", "S. Brandt", "L. Hanlon", "E. Kuulkers", "P. Laurent", "F. Lebrun", "J. P. Roques", "P. Ubertini", "G. Weidenspointner" ], "comment": "submitted to ApJL", "categories": [ "astro-ph.HE" ], "abstract": "Using observations of the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL), we put tight upper limits on the gamma-ray and hard X-ray prompt emission associated with the gravitational wave event \\gwevent, discovered by the LIGO/Virgo collaboration. The omni-directional view of the INTEGRAL/SPI-ACS has allowed us to constrain the fraction of energy emitted in the hard X-ray electromagnetic component for the full high-probability sky region of LIGO/Virgo trigger. Our upper limits on the hard X-ray fluence at the time of the event range from $F_{\\gamma}=2 \\times 10^{-8}$ erg cm$^{-2}$ to $F_{\\gamma}=10^{-6}$ erg cm$^{-2}$ in the 75 keV - 2 MeV energy range for typical spectral models. Our results constrain the ratio of the energy promptly released in gamma-rays in the direction of the observer to the gravitational wave energy E$_\\gamma/$E$_{GW}<10^{-6}$. We discuss the implication of gamma-ray limits on the characteristics of the gravitational wave source, based on the available predictions for prompt electromagnetic emission.", "revisions": [ { "version": "v1", "updated": "2016-02-12T19:31:55.000Z" } ], "analyses": { "keywords": [ "gravitational wave event gw150914", "integral upper limits", "gamma-ray emission", "hard x-ray prompt emission" ], "publication": { "doi": "10.3847/2041-8205/820/2/L36" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1421416 } } }