{ "id": "2009.09039", "version": "v1", "published": "2020-09-18T19:37:04.000Z", "updated": "2020-09-18T19:37:04.000Z", "title": "A survey of active galaxies at TeV photon energies with the HAWC gamma-ray observatory", "authors": [ "A. Albert", "C. Alvarez", "J. R. Angeles Camacho", "J. C. Arteaga-Velázquez", "K. P. Arunbabu", "D. Avila Rojas", "H. A. Ayala Solares", "V. Baghmanyan", "E. Belmont-Moreno", "S. Y. BenZvi", "C. Brisbois", "K. S. Caballero-Mora", "T. Capistrán", "A. Carramiñana", "S. Casanova", "U. Cotti", "J. Cotzomi", "S. Coutiño de León", "E. De la Fuente", "B. L. Dingus", "M. A. DuVernois", "M. Durocher", "J. C. Díaz-Vélez", "K. Engel", "C. Espinoza", "K. L. Fan", "M. Fernández Alonso", "H. Fleischhack", "N. Fraija", "A. Galván-Gámez", "D. García", "J. A. García-González", "F. Garfias", "M. M. González", "J. A. Goodman", "J. P. Harding", "S. Hernández", "B. Hona", "D. Huang", "F. Hueyotl-Zahuantitla", "P. Hüntemeyer", "A. Iriarte", "A. Jardin-Blicq", "V. Joshi", "D. Kieda", "A. Lara", "W. H. Lee", "H. León Vargas", "J. T. Linnemann", "A. L. Longinotti", "G. Luis-Raya", "J. Lundeen", "K. Malone", "O. Martínez", "I. Martinez-Castellanos", "J. Martínez-Castro", "J. A. Matthews", "P. Miranda-Romagnoli", "J. A. Morales-Soto", "E. Moreno", "M. Mostafá", "A. Nayerhoda", "L. Nellen", "M. Newbold", "M. U. Nisa", "R. Noriega-Papaqui", "L. Olivera-Nieto", "A. Peisker", "E. G. Pérez-Pérez", "C. D. Rho", "D. Rosa-González", "E. Ruiz-Velasco", "H. Salazar", "F. Salesa Greus", "A. Sandoval", "M. Schneider", "H. Schoorlemmer", "A. J. Smith", "R. W. Springer", "K. Tollefson", "I. Torres", "R. Torres-Escobedo", "F. Ureña-Mena", "L. Villaseñor", "T. Weisgarber", "E. Willox", "A. Zepeda", "H. Zhou", "C. de León" ], "comment": "The HAWC survey of Fermi 3FHL AGNs: 30 pages, 13 figures. Submitted to the Astrophysical Journal", "categories": [ "astro-ph.HE" ], "abstract": "The High Altitude Water Cherenkov Gamma-Ray Observatory (HAWC) continuously detects TeV photons and particles within its large field-of-view, accumulating every day a deeper exposure of two thirds of the sky. We analyzed 1523~days of HAWC live data acquired over four and a half years, in a follow-up analysis of {138} nearby ($z<0.3$) active galactic nuclei from the {\\em Fermi} 3FHL catalog culminating within $40^\\circ$ of the zenith at Sierra Negra, the HAWC site. This search for persistent TeV emission used a maximum-likelihood analysis assuming intrinsic power-law spectra attenuated by pair production of gamma-ray photons with the extragalactic background light. HAWC clearly detects persistent emission from Mkn~421 and Mkn~501, the two brightest blazars in the TeV sky, at 65$\\sigma$ and 17$\\sigma$ level, respectively. {Weaker evidence for long-term emission is found for three other known very-high energy emitters:} the radiogalaxy M87 and the BL Lac objects VER~J0521+211 and 1ES~1215+303, the later two at $z\\sim 0.1$. We find evidence for collective emission from the set of 30 previously reported very high-energy sources that excludes Mkn~421 and Mkn~501 with a random probability $\\sim 10^{-5}$. Upper limits are presented for the sample under the power-law assumption and in the predefined (0.5-2.0), (2.0-8.0) and (8.0-32.0) TeV energy intervals.", "revisions": [ { "version": "v1", "updated": "2020-09-18T19:37:04.000Z" } ], "analyses": { "keywords": [ "hawc gamma-ray observatory", "tev photon energies", "altitude water cherenkov gamma-ray", "water cherenkov gamma-ray observatory", "clearly detects persistent emission" ], "note": { "typesetting": "TeX", "pages": 30, "language": "en", "license": "arXiv", "status": "editable" } } }