{ "id": "1209.0353", "version": "v1", "published": "2012-09-03T13:50:30.000Z", "updated": "2012-09-03T13:50:30.000Z", "title": "Correlation between Ultra-high Energy Cosmic Rays and Active Galactic Nuclei from Fermi Large Area Telescope", "authors": [ "Jihyun Kim", "Hang Bae Kim" ], "comment": "14 pages, 3 figures, 1 table", "journal": "J.Korean Phys.Soc. Volume 61, Issue 11, 1911-1917 (2012)", "doi": "10.3938/jkps.61.1911", "categories": [ "astro-ph.HE" ], "abstract": "We study the possibility that the $\\gamma$-ray loud active galactic nuclei (AGN) are the sources of ultra-high energy cosmic rays (UHECR), through the correlation analysis of their locations and the arrival directions of UHECR. We use the $\\gamma$-ray loud AGN with $d\\le 100 {\\rm Mpc}$ from the second Fermi Large Area Telescope AGN catalog and the UHECR data with $E\\ge 55 {\\rm EeV}$ observed by Pierre Auger Observatory. The distribution of arrival directions expected from the $\\gamma$-ray loud AGN is compared with that of the observed UHECR using the correlational angular distance distribution and the Kolmogorov-Smirnov test. We conclude that the hypothesis that the $\\gamma$-ray loud AGN are the dominant sources of UHECR is disfavored unless there is a large smearing effect due to the intergalactic magnetic fields.", "revisions": [ { "version": "v1", "updated": "2012-09-03T13:50:30.000Z" } ], "analyses": { "keywords": [ "fermi large area telescope", "ultra-high energy cosmic rays", "ray loud agn", "large area telescope agn", "area telescope agn catalog" ], "tags": [ "journal article" ], "publication": { "journal": "Journal of Korean Physical Society", "year": 2012, "month": "Dec", "volume": 61, "number": 11, "pages": 1911 }, "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1184138, "adsabs": "2012JKPS...61.1911K" } } }