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dc.contributor.authorConnolly, M.P.
dc.contributor.authorGillanders, Gary
dc.contributor.authorMoriarty, P.
dc.contributor.authorLang, Mark
dc.date.accessioned2016-04-13T13:53:32Z
dc.date.available2016-04-13T13:53:32Z
dc.date.issued2015-01-20
dc.identifier.citationAliu, E,Archer, A,Aune, T,Barnacka, A,Behera, B,Beilicke, M,Benbow, W,Berger, K,Bird, R,Buckley, JH,Bugaev, V,Byrum, K,Cardenzana, JV,Cerruti, M,Chen, X,Ciupik, L,Connolly, MP,Cui, W,Dickinson, HJ,Dumm, J,Eisch, JD,Errando, M,Falcone, A,Federici, S,Feng, Q,Finley, JP,Fortin, P,Fortson, L,Furniss, A,Galante, N,Gillanders, GH,Griffin, S,Griffiths, ST,Grube, J,Gyuk, G,Hakansson, N,Hanna, D,Holder, J,Hughes, G,Humensky, TB,Johnson, CA,Kaaret, P,Kar, P,Kertzman, M,Khassen, Y,Kieda, D,Krawczynski, H,Krennrich, F,Kumar, S,Lang, MJ,Madhavan, A,McArthur, S,McCann, A,Meagher, K,Millis, J,Moriarty, P,Nieto, D,de Bhroithe, AO,Ong, RA,Orr, M,Otte, AN,Park, N,Perkins, JS,Pohl, M,Popkow, A,Prokoph, H,Pueschel, E,Quinn, J,Ragan, K,Rajotte, J,Reyes, LC,Reynolds, PT,Richards, GT,Roache, E,Sembroski, GH,Sha (2015) 'VERITAS OBSERVATIONS OF THE BL LAC OBJECT PG 1553+113'. Astrophysical Journal, 799 .en_IE
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/10379/5675
dc.description.abstractWe present results from VERITAS observations of the BL Lac object PG 1553+113 spanning the years 2010, 2011, and 2012. The time-averaged spectrum, measured between 160 and 560 GeV, is well described by a power law with a spectral index of 4.33 +/- 0.09. The time-averaged integral flux above 200 GeV measured for this period was (1.69 +/- 0.06) x 10(-11) photons cm(-2) s(-1), corresponding to 6.9% of the Crab Nebula flux. We also present the combined gamma-ray spectrum from the Fermi Large Area Telescope and VERITAS covering an energy range from 100 MeV to 560 GeV. The data are well fit by a power law with an exponential cutoff at 101.9 +/- 3.2 GeV. The origin of the cutoff could be intrinsic to PG 1553+113 or be due to the gamma-ray opacity of our universe through pair production off the extragalactic background light (EBL). Given lower limits to the redshift of z > 0.395 based on optical/UV observations of PG 1553+113, the cutoff would be dominated by EBL absorption. Conversely, the small statistical uncertainties of the VERITAS energy spectrum have allowed us to provide a robust upper limit on the redshift of PG 1553+113 of zen_IE
dc.description.sponsorshipThis research is supported by grants from the U.S. Department of Energy Office of Science, the U.S. National Science Foundation and the Smithsonian Institution, by NSERC in Canada, by Science Foundation Ireland (SFI 10/RFP/AST2748) and by STFC in the U.K.en_IE
dc.formatapplication/pdfen_IE
dc.language.isoenen_IE
dc.publisherAmerican Astronomical Societyen_IE
dc.relation.ispartofAstrophysical Journalen
dc.subjectBL Lacertae objects: generalen_IE
dc.subjectPG-1553+113en_IE
dc.subjectPhysicsen_IE
dc.subjectExtragalactic background lighten_IE
dc.subjectLacertae objectsen_IE
dc.subjectGamma raysen_IE
dc.subjectOptical spectroscopyen_IE
dc.subjectModelen_IE
dc.subjectRadiationen_IE
dc.subjectSpectraen_IE
dc.subjectTelescopeen_IE
dc.subjectBlazarsen_IE
dc.titleVERITAS observations of the BL Lac object PG 1553+113en_IE
dc.typeArticleen_IE
dc.date.updated2016-04-13T10:24:55Z
dc.identifier.doi10.1088/0004-637X/799/1/7
dc.local.publishedsourcehttp://iopscience.iop.org/article/10.1088/0004-637X/799/1/7/metaen_IE
dc.description.peer-reviewedpeer-reviewed
dc.contributor.funder|~|
dc.internal.rssid8514397
dc.local.contactMark Lang, School Of Physics, Room 147, Arts/Science Building, Nui Galway. 3241 Email: mark.lang@nuigalway.ie
dc.local.copyrightcheckedNo
dc.local.versionACCEPTED
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