Multi-wavelength pulsars study : Long-term timing of XMM, HESS and GLAST sources with the Nancay radiotelescope
hal.structure.identifier | Galaxies, Etoiles, Physique, Instrumentation [GEPI] | |
hal.structure.identifier | Laboratoire de physique et chimie de l'environnement [LPCE] | |
dc.contributor.author | THEUREAU, Gilles | |
hal.structure.identifier | Laboratoire de physique et chimie de l'environnement [LPCE] | |
dc.contributor.author | COGNARD, Ismaël | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | SMITH, D. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | WEBB, N. | |
hal.structure.identifier | Laboratoire de Physique Théorique et Astroparticules [LPTA] | |
dc.contributor.author | GALLANT, Y. | |
dc.contributor.editor | D. Barret | |
dc.contributor.editor | F. Casoli | |
dc.contributor.editor | G. Lagache | |
dc.contributor.editor | A. Lecavelier | |
dc.contributor.editor | L. Pagani | |
dc.date.issued | 2006 | |
dc.date.conference | 2006-06-26 | |
dc.description.abstractEn | We present here the current Nançay observing program gathering the pulsar french community around the radio follow-up of X- and gamma-ray pulsars for the building of a complete multi-wavelength sample. The goal of this project is double : 1) provide strong constraints on the physics and emission mechanisms of pulsars , 2) guarantee the success of pulsar harvest at high energy by providing good and contemporaneous ephemerides for folding the few gamma and X-ray photons . The community is well involved in the last generation of gamma-ray and X-ray detectors and the availability of the NRT and its dedicated backend BON represents a very good opportunity for acquiring the necessary and complementary radio data. | |
dc.language.iso | en | |
dc.publisher | Société Française d'Astronomie et d'Astrophysique | |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/ | |
dc.title.en | Multi-wavelength pulsars study : Long-term timing of XMM, HESS and GLAST sources with the Nancay radiotelescope | |
dc.type | Communication dans un congrès | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
bordeaux.page | 197-200 | |
bordeaux.country | FR | |
bordeaux.conference.city | Paris | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00135989 | |
hal.version | 1 | |
hal.invited | non | |
hal.proceedings | oui | |
hal.conference.end | 2006-06-30 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00135989v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2006&rft.spage=197-200&rft.epage=197-200&rft.au=THEUREAU,%20Gilles&COGNARD,%20Isma%C3%ABl&SMITH,%20D.&WEBB,%20N.&GALLANT,%20Y.&rft.genre=unknown |
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