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Discovery of Pulsations from the pulsars J0205+6449 in SNR 3C 58 with the Fermi Gammay-ray Space Telescope
dc.contributor.author | A. ABDO, A. | |
dc.contributor.author | ACKERMANN, Markus | |
dc.contributor.author | AJELLO, Marco | |
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 | 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 | D. BLANDFORD, R. | |
dc.contributor.author | D. BLOOM, E. | |
dc.contributor.author | BONAMENTE, E. | |
dc.contributor.author | W. BORGLAND, A. | |
dc.contributor.author | BOUVIER, 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 | CAMILO, F. | |
dc.contributor.author | CARAVEO, P. A. | |
dc.contributor.author | M. CASANDJIAN, J. | |
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 et chimie de l'environnement [LPCE] | |
dc.contributor.author | COGNARD, Ismaël | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | COHEN-TANUGI, J. | |
dc.contributor.author | CONRAD, J. | |
dc.contributor.author | D. DERMER, C. | |
dc.contributor.author | DE ANGELIS, 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. | |
dc.contributor.author | EDMONDS, Y. | |
dc.contributor.author | ESPINOZA, C. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | FARNIER, C. | |
dc.contributor.author | FAVUZZI, C. | |
dc.contributor.author | B. FOCKE, W. | |
dc.contributor.author | FRAILIS, M. | |
dc.contributor.author | C. C. FREIRE, P. | |
dc.contributor.author | FUKAZAWA, Y. | |
dc.contributor.author | FUSCO, P. | |
dc.contributor.author | GARGANO, F. | |
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 | 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 | HANABATA, Y. | |
dc.contributor.author | K. HARDING, A. | |
dc.contributor.author | HAYASHIDA, M. | |
dc.contributor.author | HAYS, E. | |
dc.contributor.author | HOBBS, G. | |
dc.contributor.author | E. HUGHES, R. | |
dc.contributor.author | JOHANNESSON, G. | |
dc.contributor.author | S. JOHNSON, A. | |
dc.contributor.author | P. JOHNSON, R. | |
dc.contributor.author | J. JOHNSON, T. | |
dc.contributor.author | N. JOHNSON, W. | |
dc.contributor.author | JOHNSTON, S. | |
dc.contributor.author | KAMAE, T. | |
dc.contributor.author | M. KASPI, V. | |
dc.contributor.author | KATAGIRI, H. | |
dc.contributor.author | KATAOKA, J. | |
dc.contributor.author | KAWAI, N. | |
dc.contributor.author | KEITH, M. | |
dc.contributor.author | KERR, M. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | KNÖDLSEDER, Jürgen | |
dc.contributor.author | KRAMER, M. | |
dc.contributor.author | KUEHN, F. | |
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 | LIVINGSTONE, 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 | G. LYNE, A. | |
dc.contributor.author | MAKEEV, A. | |
dc.contributor.author | N. MANCHESTER, R. | |
dc.contributor.author | MARELLI, M. | |
dc.contributor.author | N. MAZZIOTTA, M. | |
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 | 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 | L. NOLAN, P. | |
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. | |
dc.contributor.author | H. PANETTA, J. | |
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 | RAINO, S. | |
dc.contributor.author | RANDO, R. | |
dc.contributor.author | M. RANSOM, S. | |
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 | 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 | 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. | |
dc.contributor.author | W. STAPPERS, B. | |
dc.contributor.author | STRIANI, E. | |
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 | TANAKA, T. | |
dc.contributor.author | B. THAYER, J. | |
dc.contributor.author | G. THAYER, J. | |
hal.structure.identifier | Laboratoire de physique et chimie de l'environnement [LPCE] | |
dc.contributor.author | THEUREAU, G. | |
dc.contributor.author | J. THOMPSON, D. | |
dc.contributor.author | E. THORSETT, S. | |
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 | 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 | WELTEVREDE, P. | |
dc.contributor.author | L. WINER, B. | |
dc.contributor.author | S. WOOD, K. | |
dc.contributor.author | YLINEN, T. | |
dc.contributor.author | ZIEGLER, M. | |
dc.date.issued | 2009-07-10 | |
dc.identifier.issn | 2041-8205 | |
dc.description.abstractEn | We report the discovery of γ-ray pulsations (≥0.1 GeV) from the young radio and X-ray pulsar PSR J0205 + 6449 located in the Galactic supernova remnant 3C 58. Data in the γ-ray band were acquired by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope (formerly GLAST), while the radio rotational ephemeris used to fold γ-rays was obtained using both the Green Bank Telescope and the Lovell telescope at Jodrell Bank. The light curve consists of two peaks separated by 0.49 ± 0.01 ± 0.01 cycles which are aligned with the X-ray peaks. The first γ-ray peak trails the radio pulse by 0.08 ± 0.01 ± 0.01, while its amplitude decreases with increasing energy as for the other γ-ray pulsars. Spectral analysis of the pulsed γ-ray emission suggests a simple power law of index –2.1 ± 0.1 ± 0.2 with an exponential cutoff at 3.0+1.1 –0.7 ± 0.4 GeV. The first uncertainty is statistical and the second is systematic. The integral γ-ray photon flux above 0.1 GeV is (13.7 ± 1.4 ± 3.0) × 10–8 cm–2 s–1, which implies for a distance of 3.2 kpc and assuming a broad fan-like beam a luminosity of 8.3 × 1034 erg s–1 and an efficiency η of 0.3%. Finally, we report a 95% upper limit on the flux of 1.7 × 10–8 cm–2 s–1 for off-pulse emission from the object. | |
dc.language.iso | en | |
dc.publisher | Bristol : IOP Publishing | |
dc.title.en | Discovery of Pulsations from the pulsars J0205+6449 in SNR 3C 58 with the Fermi Gammay-ray Space Telescope | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1088/0004-637X/699/2/L102 | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.identifier.arxiv | 0906.1217 | |
bordeaux.journal | The Astrophysical journal letters | |
bordeaux.page | L102-L107 | |
bordeaux.volume | 699 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00410517 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00410517v1 | |
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