{ "id": "1103.3946", "version": "v1", "published": "2011-03-21T09:04:01.000Z", "updated": "2011-03-21T09:04:01.000Z", "title": "Contribution of the Gamma-ray Loud Radio Galaxies Core Emissions to the Cosmic MeV and GeV Gamma-Ray Background Radiation", "authors": [ "Yoshiyuki Inoue" ], "comment": "9 pages, accepted for publication in ApJ", "categories": [ "astro-ph.HE", "astro-ph.CO" ], "abstract": "The Fermi gamma-ray satellite has recently detected gamma-ray emissions from radio galaxy cores. From these samples, we first examine the correlation between the luminosities at 5 GHz, L_{5GHz}, and at 0.1-10 GeV, L_{gamma}, of these gamma-ray loud radio galaxies. We find that the correlation is significant with L_{gamma} \\propto L_{5GHz}^{1.16} based on a partial correlation analysis. Using this correlation and the radio luminosity function (RLF) of radio galaxies, we further explore the contribution of gamma-ray loud radio galaxies to the unresolved extragalactic gamma-ray background (EGRB). The gamma-ray luminosity function is obtained by normalizing the RLF to reproduce the source count distribution of the Fermi gamma-ray loud radio galaxies. We find that gamma-ray loud radio galaxies will explain ~25% of the unresolved Fermi EGRB flux above 100 MeV and will also make a significant contribution to the EGRB in the 1-30 MeV energy band. Since blazars explain 22% of the EGRB above 100 MeV, radio loud active galactic nuclei (AGNs) population explains ~47% of the unresolved EGRB. We further make an interpretation on the origin of the EGRB. The observed EGRB spectrum at 0.2-100 GeV does not show an absorption signature by the extragalactic background light. Thus, the dominant population of the origin of EGRB at very high energy (>30 GeV) might be nearby gamma-ray emitting sources or sources with very hard gamma-ray spectrum.", "revisions": [ { "version": "v1", "updated": "2011-03-21T09:04:01.000Z" } ], "analyses": { "keywords": [ "radio galaxy", "loud radio galaxies core emissions", "gamma-ray loud radio galaxies core", "gev gamma-ray background radiation" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/733/1/66", "journal": "The Astrophysical Journal", "year": 2011, "month": "May", "volume": 733, "number": 1, "pages": 66 }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 893238, "adsabs": "2011ApJ...733...66I" } } }