J/ApJ/907/67ivo://CDS.VizieR/J/ApJ/907/67doi:10.26093/cds/vizier.19070067CDSAlbert A.Alvarez C.Camacho J.R.A.Arteaga-Velazquez J.C.,Arunbabu K.P.Rojas D.A.Solares H.A.A.Baghmanyan V.Belmont-Moreno E.,BenZvi S.Y.Brisbois C.Caballero-Mora K.S.Capistran T.Carraminana A.,Casanova S.Cotti U.Cotzomi J.de Leon S.C.De la Fuente E.,Dingus B.L.DuVernois M.A.Durocher M.Diaz-Velez J.C.Engel K.,Espinoza C.Fan K.L.Alonso M.F.Fleischhack H.Fraija N.,Galvan-Gamez A.Garcia D.Garcia-Gonzalez J.A.Garfias F.Gonzalez M.M.,Goodman J.A.Harding J.P.Hernandez S.Hona B.Huang D.,Hueyotl-Zahuantitla F.Huntemeyer P.Iriarte A.Jardin-Blicq A.,Joshi V.Kieda D.Kunde G.J.Lara A.Lee W.H.Vargas H.L.,Linnemann J.T.Longinotti A.L.Luis-Raya G.Lundeen J.Malone K.,Martinez O.Martinez-Castellanos I.Martinez-Castro J.Matthews J.A.,Miranda-Romagnoli P.Morales-Soto J.A.Moreno E.Mostafa M.,Nayerhoda A.Nellen L.Newbold M.Nisa M.U.Noriega-Papaqui R.,Olivera-Nieto L.Peisker A.Perez-Perez E.G.Rho C.D.Rosa-Gonzalez D.,Ruiz-Velasco E.Salazar H.Greus F.S.Sandoval A.Schneider M.,Schoorlemmer H.Smith A.J.Springer R.W.Tollefson K.Torres I.,Torres-Escobedo R.Urena-Mena F.Villasenor L.Weisgarber T.Willox E.,Zepeda A.Zhou H.de Leon C.The HAWC collaboration2022-08-26T06:42:35Z2022-06-27T07:43:52ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fractive-galactic-nucleigamma-ray-astronomysurveysThe High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory 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 1523days 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 Third Catalog of Hard Fermi-LAT sources culminating within 40{deg} 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 Mkn421 and Mkn501, the two brightest blazars in the TeV sky, at 65{sigma} and 17{sigma} level, respectively. Marginal evidence, just above the 3{sigma} level, was found for three other known very high-energy emitters: the radio galaxy M87 and the BL Lac objects VERJ0521+211 and 1ES1215+303, the latter two at z~0.1. We find a 4.2{sigma} evidence for collective emission from the set of 30 previously reported very high-energy sources, with Mkn421 and Mkn501 excluded. 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.2021ApJ...907...67Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/907/67CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/175/97 : CGRaBS survey of {gamma}-ray blazar candidates (Healey+, 2008)J/ApJ/764/135 : Spectroscopic redshifts of BL Lac objects (Shaw+, 2013)J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)J/A+A/593/A91 : Mrk 421 multi-wavelength variability, 2007-2009 (Ahnen+, 2016)J/ApJS/232/18 : The third Fermi-LAT >10GeV catalog (3FHL) (Ajello+, 2017)J/A+A/612/A1 : H.E.S.S. Galactic Plane Survey (HESS+, 2018)J/ApJS/247/16 : Extreme high-frequency-peaked BL Lac objects (Acciari+, 2020)J/ApJ/891/170 : 10yr radio-to-gamma-ray obs. of 1ES 1215+30.3 (Valverde+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/907/67https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/907/67http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/907/67https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/907/67https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/907/67http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/907/67GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/907/67/table3 (HAWC power-law fits and significances for the revised 136 AGNs from the 3FHL catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/907/67/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/907/67/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/907/67/table3?GETtext/xml+votable180.050000true1.999885347.20215810.0055555555555555566/18 398 514 615 717 988 1680 1700-1701 2273 2549 2621 2792 2929 4255 4317 4801 4882 5091 5423 5483 5522 5536 5918 6018 6088 6348 6436 6502 6647 6764 6910 6996 7233 7354 8374 8556 8751 8945 8972 9013 9049 9104 9501 9554 9612 9711 9855 9892 10033 10183 10605 10656 11426 11430 11444 12604 13098 13586 13640 13673 13705 13711 13820 13927 15495 16638 16806 17574 17754 17843 17917 17994 18270 19190 19589 19723 19831 20016 20083 20325 20478 20920 21758 21935 21972 22363 23085 23127 23134 23222 23835 24027 24260 25519 25542 25734 25760 26074 26242 26292 26322 26626 26964 27765 27945 28138-28139 28225 28249 28352 28454 28492 28498 28517 28546 29017 30015 30039 30842 31407 31461 31666 32311 32345 32621 36278 36296 36342 36548 40689 48603 48878 49141https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/907/67?format=asciiGamma-raydefaultJ/ApJ/907/67/table3HAWC power-law fits and significances for the revised 136 AGNs from the 3FHL catalog3FHLSource name from 3FHL catalogmeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameOther identifiermeta.idcharClassIdentification or association class given in 3FHL (1)src.classcharz[0.003/0.3] 3FHL redshiftsrc.redshiftfloatTS[-5.82/4167] Test statistics and significances estimatedstat.fit.goodnessdoublee_TS[-3/65] Error on TSstat.errorfloatK[-99/29.5] Power-law normalization at 1 TeV (10^-12^/TeV/cm^2^/s)stat.fit.paramfloate_K[0.16/71] Error on Kstat.errorfloatl_K[0.24/107] 2sigma upper limit (in same unit) on K (2)meta.code.errorfloatSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPosition from SIMBAD (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD (declination part)degpos.eq.dec;meta.main