Veritas upper limit on the very high energy emission from the radio galaxy NGC 1275
dc.contributor.author | A. ACCIARI, V. | |
dc.contributor.author | ALIU, E. | |
dc.contributor.author | ARLEN, T. | |
dc.contributor.author | AUNE, T. | |
dc.contributor.author | BAUTISTA, M. | |
dc.contributor.author | BEILICKE, M. | |
dc.contributor.author | BENBOW, W. | |
dc.contributor.author | BOLTUCH, D. | |
dc.contributor.author | M. BRADBURY, S. | |
dc.contributor.author | H. BUCKLEY, J. | |
dc.contributor.author | BUGAEV, V. | |
dc.contributor.author | BYRUM, K. | |
dc.contributor.author | CANNON, A. | |
dc.contributor.author | CELIK, O. | |
dc.contributor.author | CESARINI, A. | |
dc.contributor.author | CIUPIK, L. | |
dc.contributor.author | COGAN, P. | |
dc.contributor.author | CUI, W. | |
dc.contributor.author | DICKHERBER, R. | |
dc.contributor.author | DUKE, C. | |
dc.contributor.author | J. FEGAN, S. | |
dc.contributor.author | P. FINLEY, J. | |
dc.contributor.author | FORTIN, P. | |
dc.contributor.author | FORTSON, L. | |
dc.contributor.author | FURNISS, A. | |
dc.contributor.author | GALANTE, N. | |
dc.contributor.author | GALL, D. | |
dc.contributor.author | GIBBS, K. | |
dc.contributor.author | H. GILLANDERS, G. | |
dc.contributor.author | GODAMBE, S. | |
dc.contributor.author | GRUBE, J. | |
dc.contributor.author | GUENETTE, R. | |
dc.contributor.author | GYUK, G. | |
dc.contributor.author | HANNA, D. | |
dc.contributor.author | HOLDER, J. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | HORAN, D. | |
dc.contributor.author | M. HUI, C. | |
dc.contributor.author | B. HUMENSKY, T. | |
dc.contributor.author | IMRAN, A. | |
dc.contributor.author | KAARET, P. | |
dc.contributor.author | KARLSSON, N. | |
dc.contributor.author | KERTZMAN, M. | |
dc.contributor.author | KIEDA, D. | |
dc.contributor.author | KONOPELKO, A. | |
dc.contributor.author | KRAWCZYNSKI, H. | |
dc.contributor.author | KRENNRICH, F. | |
dc.contributor.author | J. LANG, M. | |
dc.contributor.author | LEBOHEC, S. | |
dc.contributor.author | MAIER, G. | |
dc.contributor.author | MCCANN, A. | |
dc.contributor.author | MCCUTCHEON, M. | |
dc.contributor.author | MILLIS, J. | |
dc.contributor.author | MORIARTY, P. | |
dc.contributor.author | MUKHERJEE, R. | |
dc.contributor.author | A. ONG, R. | |
dc.contributor.author | N. OTTE, A. | |
dc.contributor.author | PANDEL, D. | |
dc.contributor.author | S. PERKINS, J. | |
dc.contributor.author | POHL, M. | |
dc.contributor.author | QUINN, J. | |
dc.contributor.author | RAGAN, K. | |
dc.contributor.author | T. REYNOLDS, P. | |
dc.contributor.author | ROACHE, E. | |
dc.contributor.author | J. ROSE, H. | |
dc.contributor.author | SCHROEDTER, M. | |
dc.contributor.author | H. SEMBROSKI, G. | |
dc.contributor.author | W. SMITH, A. | |
dc.contributor.author | STEELE, D. | |
dc.contributor.author | P. SWORDY, S. | |
dc.contributor.author | THEILING, M. | |
dc.contributor.author | A. TONER, J. | |
dc.contributor.author | VARLOTTA, A. | |
dc.contributor.author | V. VASSILIEV, V. | |
dc.contributor.author | VINCENT, Serge | |
dc.contributor.author | G. WAGNER, R. | |
dc.contributor.author | P. WAKELY, S. | |
dc.contributor.author | E. WARD, J. | |
dc.contributor.author | C. WEEKES, T. | |
dc.contributor.author | WEINSTEIN, A. | |
dc.contributor.author | WEISGARBER, T. | |
dc.contributor.author | A. WILLIAMS, D. | |
dc.contributor.author | WISSEL, S. | |
dc.contributor.author | WOOD, M. | |
dc.contributor.author | ZITZER, B. | |
dc.contributor.author | KATAOKA, J. | |
dc.contributor.author | CAVAZZUTI, E. | |
dc.contributor.author | C. CHEUNG, C. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | LOTT, B. | |
dc.contributor.author | J. THOMPSON, D. | |
dc.contributor.author | TOSTI, G. | |
dc.date.issued | 2009-12-01 | |
dc.identifier.issn | 2041-8205 | |
dc.description.abstractEn | The recent detection by the Fermi γ-ray space telescope of high-energy γ-rays from the radio galaxy NGC 1275 makes the observation of the very high energy (VHE: E>100 GeV) part of its broadband spectrum particularly interesting, especially for the understanding of active galactic nuclei with misaligned multi-structured jets. The radio galaxy NGC 1275 was recently observed by VERITAS at energies above 100 GeV for about 8 hr. No VHE γ-ray emission was detected by VERITAS from NGC 1275. A 99% confidence level upper limit of 2.1% of the Crab Nebula flux level is obtained at the decorrelation energy of approximately 340 GeV, corresponding to 19% of the power-law extrapolation of the Fermi Large Area Telescope result. | |
dc.language.iso | en | |
dc.publisher | Bristol : IOP Publishing | |
dc.subject.en | Perseus A) | |
dc.subject.en | galaxies: Seyfert | |
dc.subject.en | gamma rays: observations | |
dc.subject.en | galaxies: individual (NGC 1275 | |
dc.subject.en | 3C 84 | |
dc.title.en | Veritas upper limit on the very high energy emission from the radio galaxy NGC 1275 | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1088/0004-637X/706/2/L275 | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.identifier.arxiv | 0911.0740 | |
bordeaux.journal | The Astrophysical journal letters | |
bordeaux.page | L275-L280 | |
bordeaux.volume | 706 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00460536 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00460536v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=The%20Astrophysical%20journal%20letters&rft.date=2009-12-01&rft.volume=706&rft.spage=L275-L280&rft.epage=L275-L280&rft.eissn=2041-8205&rft.issn=2041-8205&rft.au=A.%20ACCIARI,%20V.&ALIU,%20E.&ARLEN,%20T.&AUNE,%20T.&BAUTISTA,%20M.&rft.genre=article |
Fichier(s) constituant ce document
Fichiers | Taille | Format | Vue |
---|---|---|---|
Il n'y a pas de fichiers associés à ce document. |