dc.contributor.author | ABDO, A.A. | |
dc.contributor.author | ACKERMANN, Markus | |
dc.contributor.author | AJELLO, Marco | |
dc.contributor.author | AXELSSON, Magnus | |
dc.contributor.author | BALDINI, Luca | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | BALLET, Jean | |
dc.contributor.author | BARBIELLINI, Guido | |
dc.contributor.author | BASTIERI, D. | |
dc.contributor.author | BAUGHMAN, B.M. | |
dc.contributor.author | BECHTOL, K. | |
dc.contributor.author | BELLAZZINI, R. | |
dc.contributor.author | BERENJI, B. | |
dc.contributor.author | BLANDFORD, R.D. | |
dc.contributor.author | BLOOM, E.D. | |
dc.contributor.author | BONAMENTE, E. | |
dc.contributor.author | BORGLAND, A. | |
dc.contributor.author | BREGEON, J. | |
dc.contributor.author | BREZ, A. | |
dc.contributor.author | BRIGIDA, M. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | BRUEL, Pascal | |
dc.contributor.author | BURNETT, T. H. | |
dc.contributor.author | BUSON, S. | |
dc.contributor.author | CALIANDRO, G. A. | |
dc.contributor.author | CAMERON, R. A. | |
dc.contributor.author | CARAVEO, P. A. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CASANDJIAN, J. M. | |
dc.contributor.author | CAVAZZUTI, E. | |
dc.contributor.author | CECCHI, C. | |
dc.contributor.author | CELIK, O. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CHARLES, E. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CHATY, S. | |
dc.contributor.author | CHEKHTMAN, A. | |
dc.contributor.author | CHIANG, J. | |
dc.contributor.author | CIPRINI, S. | |
dc.contributor.author | CLAUS, R. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | COHEN-TANUGI, J. | |
dc.contributor.author | COLAFRANCESCO, S. | |
dc.contributor.author | COMINSKY, L. R. | |
dc.contributor.author | CONRAD, J. | |
dc.contributor.author | COSTAMANTE, L. | |
dc.contributor.author | CUTINI, S. | |
dc.contributor.author | DERMER, C. D. | |
dc.contributor.author | DE ANGELIS, A. | |
dc.contributor.author | DE PALMA, F. | |
dc.contributor.author | DIGEL, S. W. | |
dc.contributor.author | SILVA, E. Do Couto E | |
dc.contributor.author | DRELL, P. S. | |
dc.contributor.author | DUBOIS, R. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | DUMORA, D. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | FARNIER, C. | |
dc.contributor.author | FAVUZZI, C. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | FEGAN, S. J. | |
dc.contributor.author | FOCKE, W. B. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | FORTIN, P. | |
dc.contributor.author | FRAILIS, M. | |
dc.contributor.author | FUHRMANN, L. | |
dc.contributor.author | FUKAZAWA, Y. | |
dc.contributor.author | FUNK, S. | |
dc.contributor.author | FUSCO, P. | |
dc.contributor.author | GARGANO, F. | |
dc.contributor.author | GASPARRINI, D. | |
dc.contributor.author | GEHRELS, N. | |
dc.contributor.author | GERMANI, S. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | GIEBELS, B. | |
dc.contributor.author | GIGLIETTO, N. | |
dc.contributor.author | GIOMMI, P. | |
dc.contributor.author | GIORDANO, F. | |
dc.contributor.author | GLANZMAN, T. | |
dc.contributor.author | GODFREY, G. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | GRENIER, I. A. | |
dc.contributor.author | GROVE, J. E. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | GUILLEMOT, L. | |
dc.contributor.author | GUIRIEC, S. | |
dc.contributor.author | HADASCH, D. | |
dc.contributor.author | HANABATA, Y. | |
dc.contributor.author | HARDING, A. K. | |
dc.contributor.author | HAYASHIDA, M. | |
dc.contributor.author | HAYS, E. | |
dc.contributor.author | HEALEY, S. E. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | HORAN, D. | |
dc.contributor.author | HUGHES, R. E. | |
dc.contributor.author | ITOH, R. | |
dc.contributor.author | JACKSON, M. S. | |
dc.contributor.author | JOHANNESSON, G. | |
dc.contributor.author | JOHNSON, A. S. | |
dc.contributor.author | JOHNSON, W. N. | |
dc.contributor.author | KADLER, M. | |
dc.contributor.author | KAMAE, T. | |
dc.contributor.author | KATAGIRI, H. | |
dc.contributor.author | KATAOKA, J. | |
dc.contributor.author | KAWAI, N. | |
dc.contributor.author | KERR, M. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | KNÖDLSEDER, Jürgen | |
dc.contributor.author | KOCIAN, M. L. | |
dc.contributor.author | KUSS, M. | |
dc.contributor.author | LANDE, J. | |
dc.contributor.author | LATRONICO, L. | |
dc.contributor.author | LONGO, F. | |
dc.contributor.author | LOPARCO, F. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | LOTT, B. | |
dc.contributor.author | LOVELLETTE, M. N. | |
dc.contributor.author | LUBRANO, P. | |
dc.contributor.author | MADEJSKI, G. M. | |
dc.contributor.author | MAKEEV, A. | |
dc.contributor.author | MAX-MOERBECK, W. | |
dc.contributor.author | MAZZIOTTA, M. N. | |
dc.contributor.author | MCCONVILLE, W. | |
dc.contributor.author | MCENERY, J. E. | |
dc.contributor.author | MEURER, C. | |
dc.contributor.author | MICHELSON, P. F. | |
dc.contributor.author | MITTHUMSIRI, W. | |
dc.contributor.author | MIZUNO, T. | |
dc.contributor.author | A. MOISEEV, A. | |
dc.contributor.author | MONTE, C. | |
dc.contributor.author | E. MONZANI, M. | |
dc.contributor.author | MORSELLI, A. | |
dc.contributor.author | V. MOSKALENKO, I. | |
dc.contributor.author | MURGIA, S. | |
dc.contributor.author | NESTORAS, I. | |
dc.contributor.author | NILSSON, K. | |
dc.contributor.author | NIZHELSKY, N.A. | |
dc.contributor.author | L. NOLAN, P. | |
dc.contributor.author | P. NORRIS, J. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | NUSS, E. | |
dc.contributor.author | OHSUGI, T. | |
dc.contributor.author | OJHA, R. | |
dc.contributor.author | OMODEI, N. | |
dc.contributor.author | ORLANDO, E. | |
dc.contributor.author | F. ORMES, J. | |
dc.contributor.author | OSBORNE, J. | |
dc.contributor.author | OZAKI, M. | |
dc.contributor.author | PACCIANI, L. | |
dc.contributor.author | PADOVANI, P. | |
dc.contributor.author | PAGANI, C. | |
dc.contributor.author | PAGE, K. | |
dc.contributor.author | PANEQUE, D. | |
dc.contributor.author | H. PANETTA, J. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | PARENT, D. | |
dc.contributor.author | PASANEN, M. | |
dc.contributor.author | PAVLIDOU, V. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | PELASSA, V. | |
dc.contributor.author | PEPE, M. | |
dc.contributor.author | PERRI, M. | |
dc.contributor.author | PESCE-ROLLINS, M. | |
dc.contributor.author | PIRANOMONTE, S. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | PIRON, F. | |
dc.contributor.author | PITTORI, C. | |
dc.contributor.author | PORTER, T.A. | |
dc.contributor.author | PUCCETTI, S. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | RAHOUI, F. | |
dc.contributor.author | RAINÒ, S. | |
dc.contributor.author | RAITERI, C. | |
dc.contributor.author | RANDO, R. | |
dc.contributor.author | RAZZANO, M. | |
dc.contributor.author | REIMER, A. | |
dc.contributor.author | REIMER, O. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | REPOSEUR, T. | |
dc.contributor.author | L. RICHARDS, J. | |
dc.contributor.author | RITZ, S. | |
dc.contributor.author | S. ROCHESTER, L. | |
dc.contributor.author | Y. RODRIGUEZ, A. | |
dc.contributor.author | W. ROMANI, R. | |
dc.contributor.author | A. ROS, J. | |
dc.contributor.author | ROTH, M. | |
dc.contributor.author | ROUSTAZADEH, P. | |
dc.contributor.author | RYDE, F. | |
dc.contributor.author | F.-W. SADROZINSKI, H. | |
dc.contributor.author | SADUN, A. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | SANCHEZ, D. | |
dc.contributor.author | SANDER, A. | |
dc.contributor.author | M. SAZ PARKINSON, P. | |
dc.contributor.author | D. SCARGLE, J. | |
dc.contributor.author | SELLERHOLM, A. | |
dc.contributor.author | SGRÒ, C. | |
dc.contributor.author | S. SHAW, M. | |
dc.contributor.author | A. SIGUA, L. | |
dc.contributor.author | J. SISKIND, E. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | SMITH, David Stanley | |
dc.contributor.author | D. SMITH, P. | |
dc.contributor.author | SPANDRE, G. | |
dc.contributor.author | SPINELLI, P. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | STARCK, Jean-Luc | |
dc.contributor.author | STEVENSON, M. | |
dc.contributor.author | STRATTA, G. | |
dc.contributor.author | S. STRICKMAN, M. | |
dc.contributor.author | J. SUSON, D. | |
dc.contributor.author | TAJIMA, H. | |
dc.contributor.author | TAKAHASHI, H. | |
dc.contributor.author | TAKAHASHI, T. | |
dc.contributor.author | O. TAKALO, L. | |
dc.contributor.author | TANAKA, T. | |
dc.contributor.author | B. THAYER, J. | |
dc.contributor.author | G. THAYER, J. | |
dc.contributor.author | J. THOMPSON, D. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | TIBALDO, L. | |
dc.contributor.author | F. TORRES, D. | |
dc.contributor.author | TOSTI, G. | |
dc.contributor.author | TRAMACERE, A. | |
dc.contributor.author | UCHIYAMA, Y. | |
dc.contributor.author | L. USHER, T. | |
dc.contributor.author | VASILEIOU, V. | |
dc.contributor.author | VERRECCHIA, F. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | VILCHEZ, N. | |
dc.contributor.author | VILLATA, M. | |
dc.contributor.author | VITALE, V. | |
dc.contributor.author | P. WAITE, A. | |
dc.contributor.author | WANG, P. | |
dc.contributor.author | L. WINER, B. | |
dc.contributor.author | S. WOOD, K. | |
dc.contributor.author | YLINEN, T. | |
dc.contributor.author | A. ZENSUS, J. | |
dc.contributor.author | V. ZHEKANIS, G. | |
dc.contributor.author | ZIEGLER, M. | |
dc.date.issued | 2010-06 | |
dc.identifier.issn | 0004-637X | |
dc.description.abstractEn | We have conducted a detailed investigation of the broad-band spectral properties of the \gamma-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS). By combining our accurately estimated Fermi gamma-ray spectra with Swift, radio, infra-red, optical and other hard X-ray/gamma-ray data, collected within three months of the LBAS data taking period, we were able to assemble high-quality and quasi-simultaneous Spectral Energy Distributions (SED) for 48 LBAS blazars.The SED of these gamma-ray sources is similar to that of blazars discovered at other wavelengths, clearly showing, in the usual Log $\nu $ - Log $\nu$ F$_\nu$ representation, the typical broad-band spectral signatures normally attributed to a combination of low-energy synchrotron radiation followed by inverse Compton emission of one or more components. We have used these SEDs to characterize the peak intensity of both the low and the high-energy components. The results have been used to derive empirical relationships that estimate the position of the two peaks from the broad-band colors (i.e. the radio to optical and optical to X-ray spectral slopes) and from the gamma-ray spectral index. Our data show that the synchrotron peak frequency $\nu_p^S$ is positioned between 10$^{12.5}$ and 10$^{14.5}$ Hz in broad-lined FSRQs and between $10^{13}$ and $10^{17}$ Hz in featureless BL Lacertae objects.We find that the gamma-ray spectral slope is strongly correlated with the synchrotron peak energy and with the X-ray spectral index, as expected at first order in synchrotron - inverse Compton scenarios. However, simple homogeneous, one-zone, Synchrotron Self Compton (SSC) models cannot explain most of our SEDs, especially in the case of FSRQs and low energy peaked (LBL) BL Lacs. (...) | |
dc.language.iso | en | |
dc.publisher | American Astronomical Society | |
dc.subject.en | galaxies: active | |
dc.subject.en | gamma rays: galaxies | |
dc.subject.en | quasars: general | |
dc.subject.en | radiation mechanisms: non-thermal | |
dc.subject.en | BL Lacertae objects: general | |
dc.title.en | The Spectral Energy Distribution of Fermi bright blazars | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1088/0004-637X/716/1/30 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.identifier.arxiv | 0912.2040 | |
bordeaux.journal | The Astrophysical Journal | |
bordeaux.page | 30-70 | |
bordeaux.volume | 716 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00496030 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00496030v1 | |
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