Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT
dc.contributor.author | ABDO, A.A. | |
dc.contributor.author | ACKERMANN, Markus | |
dc.contributor.author | AJELLO, Marco | |
dc.contributor.author | ANDERSON, B. | |
dc.contributor.author | B. ATWOOD, W. | |
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 | G. BARING, M. | |
dc.contributor.author | BASTIERI, D. | |
dc.contributor.author | M. BAUGHMAN, B. | |
dc.contributor.author | BECHTOL, K. | |
dc.contributor.author | BELLAZZINI, R. | |
dc.contributor.author | BERENJI, B. | |
dc.contributor.author | F. BIGNAMI, G. | |
dc.contributor.author | D. BLANDFORD, R. | |
dc.contributor.author | D. BLOOM, E. | |
dc.contributor.author | BONAMENTE, E. | |
dc.contributor.author | W. 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 | H. BURNETT, T. | |
dc.contributor.author | A. CALIANDRO, G. | |
dc.contributor.author | A. CAMERON, R. | |
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 | CECCHI, C. | |
dc.contributor.author | CELIK, O. | |
dc.contributor.author | CHEKHTMAN, A. | |
dc.contributor.author | C. CHEUNG, C. | |
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 | CONRAD, J. | |
dc.contributor.author | CUTINI, S. | |
dc.contributor.author | D. DERMER, C. | |
dc.contributor.author | DE ANGELIS, A. | |
dc.contributor.author | DE LUCA, A. | |
dc.contributor.author | DE PALMA, F. | |
dc.contributor.author | W. DIGEL, S. | |
dc.contributor.author | DORMODY, M. | |
dc.contributor.author | DO COUTO E SILVA, E. | |
dc.contributor.author | S. DRELL, P. | |
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 | J. FEGAN, S. | |
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 | A. GRENIER, I. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | GRONDIN, M.-H. | |
dc.contributor.author | E. GROVE, J. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | GUILLEMOT, L. | |
dc.contributor.author | GUIRIEC, S. | |
dc.contributor.author | GWON, C. | |
dc.contributor.author | HANABATA, Y. | |
dc.contributor.author | K. HARDING, A. | |
dc.contributor.author | HAYASHIDA, M. | |
dc.contributor.author | HAYS, E. | |
dc.contributor.author | E. HUGHES, R. | |
dc.contributor.author | JOHANNESSON, G. | |
dc.contributor.author | P. JOHNSON, R. | |
dc.contributor.author | J. JOHNSON, T. | |
dc.contributor.author | N. JOHNSON, W. | |
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 | L. KOCIAN, M. | |
dc.contributor.author | KUSS, M. | |
dc.contributor.author | LANDE, J. | |
dc.contributor.author | LATRONICO, L. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | LEMOINE-GOUMARD, M. | |
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 | N. LOVELLETTE, M. | |
dc.contributor.author | LUBRANO, P. | |
dc.contributor.author | M. MADEJSKI, G. | |
dc.contributor.author | MAKEEV, A. | |
dc.contributor.author | MARELLI, M. | |
dc.contributor.author | N. MAZZIOTTA, M. | |
dc.contributor.author | MCCONVILLE, W. | |
dc.contributor.author | E. MCENERY, J. | |
dc.contributor.author | MEURER, C. | |
dc.contributor.author | F. MICHELSON, P. | |
dc.contributor.author | MITTHUMSIRI, W. | |
dc.contributor.author | MIZUNO, T. | |
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 | 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 | OMODEI, N. | |
dc.contributor.author | ORLANDO, E. | |
dc.contributor.author | F. ORMES, J. | |
dc.contributor.author | PANEQUE, D. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | PARENT, D. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | PELASSA, V. | |
dc.contributor.author | PEPE, M. | |
dc.contributor.author | PESCE-ROLLINS, M. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | PIERBATTISTA, M. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | PIRON, F. | |
dc.contributor.author | PORTER, T.A. | |
dc.contributor.author | R. PRIMACK, J. | |
dc.contributor.author | RAINO, S. | |
dc.contributor.author | RANDO, R. | |
dc.contributor.author | S. RAY, P. | |
dc.contributor.author | RAZZANO, M. | |
dc.contributor.author | REA, N. | |
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 | RITZ, S. | |
dc.contributor.author | S. ROCHESTER, L. | |
dc.contributor.author | Y. RODRIGUEZ, A. | |
dc.contributor.author | W. ROMANI, R. | |
dc.contributor.author | RYDE, F. | |
dc.contributor.author | F.-W. SADROZINSKI, H. | |
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. | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | SGRO, C. | |
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 | 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 | TANAKA, T. | |
dc.contributor.author | G. THAYER, J. | |
dc.contributor.author | J. THOMPSON, D. | |
dc.contributor.author | TIBALDO, L. | |
dc.contributor.author | TIBOLLA, O. | |
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 | VAN ETTEN, A. | |
dc.contributor.author | VASILEIOU, V. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | VILCHEZ, N. | |
dc.contributor.author | VITALE, V. | |
dc.contributor.author | P. WAITE, A. | |
dc.contributor.author | WANG, P. | |
dc.contributor.author | WATTERS, K. | |
dc.contributor.author | L. WINER, B. | |
dc.contributor.author | T. WOLFF, M. | |
dc.contributor.author | S. WOOD, K. | |
dc.contributor.author | YLINEN, T. | |
dc.contributor.author | ZIEGLER, M. | |
dc.date.issued | 2009-08-14 | |
dc.identifier.issn | 0036-8075 | |
dc.description.abstractEn | Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the lectromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently, only seven were observed to pulse in gamma rays and these were all discovered at other wavelengths. The Fermi Large Area Telescope makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants. | |
dc.language.iso | en | |
dc.publisher | American Association for the Advancement of Science (AAAS) | |
dc.title.en | Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1126/science.1175558 | |
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 | 1009.0748 | |
bordeaux.journal | Science | |
bordeaux.page | 840-844 | |
bordeaux.volume | 325 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00402843 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00402843v1 | |
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