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hal.structure.identifierFERMI
dc.contributor.authorHOU, X.
hal.structure.identifierFERMI
dc.contributor.authorSMITH, D.A.
hal.structure.identifierFERMI
dc.contributor.authorREPOSEUR, T.
hal.structure.identifierFERMI
dc.contributor.authorROUSSEAU, R.
dc.date.issued2014
dc.identifier.issn0004-6337
dc.description.abstractEnOver thirteen times more gamma-ray pulsars have now been studied with the Large Area Telescope on NASA's Fermi satellite than the ten seen with the Compton Gamma-Ray Observatory in the nineteen-nineties. The large sample is diverse, allowing better understanding both of the pulsars themselves and of their roles in various cosmic processes. Here we explore the prospects for even more gamma-ray pulsars as Fermi enters the 2nd half of its nominal ten-year mission. New pulsars will naturally tend to be fainter than the first ones discovered. Some of them will have unusual characteristics compared to the current population, which may help discriminate between models. We illustrate a vision of the future with a sample of six pulsars discovered after the 2nd Fermi Pulsar Catalog was written.
dc.language.isoen
dc.publisherWiley-VCH Verlag
dc.title.enBeyond the 2nd Fermi Pulsar Catalog
dc.typeArticle de revue
dc.identifier.doi10.1002/asna.201312042
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]
dc.identifier.arxiv1310.5481
bordeaux.journalAstronomical Notes / Astronomische Nachrichten
bordeaux.page334-339
bordeaux.volume335
bordeaux.peerReviewedoui
hal.identifierin2p3-00977416
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00977416v1
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