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hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorSMITH, D. A.
dc.date.issued2006-08
dc.date.conference2006-08-16
dc.description.abstractEnGeV measurements of pulsar light curves versus energy provide information on beam geometry, and spectral cut-offs give insights into the particle acceleration region(s) around the neutron star. The two together can help build a better picture of neutron star populations in the galaxy. We are on the verge of instrumental break-through that promise to increase the sample of measured objects by ~10. This talk describes instruments for multi-GeV pulsations for the next few years. We'll cover developments of ground-based atmospheric Cherenkov detectors, review AGILE's prospects, and then focus on the LAT (Large Area Telescope) on GLAST, including sensitivity estimations. Accurate radio ephemeredes can greatly enhance the gamma-ray pulsar science, and we will describe efforts to build a large ephemeredes database.
dc.language.isoen
dc.source.titleOn the Present and Future of Pulsar Astronomy, 26th meeting of the IAU
dc.title.enFuture Gamma-ray and TeV Observatories for Pulsar Searches
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
bordeaux.page62
bordeaux.volume2
bordeaux.countryCZ
bordeaux.title.proceedingOn the Present and Future of Pulsar Astronomy, 26th meeting of the IAU
bordeaux.conference.cityPrague
bordeaux.peerReviewedoui
hal.identifierin2p3-00411229
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2006-08-17
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00411229v1
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