The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
hal.structure.identifier | Laboratoire de Physique des Deux Infinis Bordeaux [LP2I - Bordeaux] | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
dc.contributor.author | SMITH, D.A | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | ABDOLLAHI, S | |
dc.contributor.author | AJELLO, M | |
dc.contributor.author | BAILES, M | |
dc.contributor.author | BALDINI, L | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | BALLET, J | |
dc.contributor.author | BARING, M.G | |
dc.contributor.author | BASSA, C | |
dc.contributor.author | GONZALEZ, J. Becerra | |
dc.contributor.author | BELLAZZINI, R | |
dc.contributor.author | BERRETTA, A | |
dc.contributor.author | BHATTACHARYYA, B | |
dc.contributor.author | BISSALDI, E | |
dc.contributor.author | BONINO, R | |
dc.contributor.author | BOTTACINI, E | |
hal.structure.identifier | Laboratoire de Physique Subatomique et de Cosmologie [LPSC] | |
dc.contributor.author | BREGEON, J | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | BRUEL, P | |
dc.contributor.author | BURGAY, M | |
dc.contributor.author | BURNETT, T.H | |
dc.contributor.author | CAMERON, R.A | |
dc.contributor.author | CAMILO, F | |
dc.contributor.author | CAPUTO, R | |
dc.contributor.author | CARAVEO, P.A | |
dc.contributor.author | CAVAZZUTI, E | |
dc.contributor.author | CHIARO, G | |
dc.contributor.author | CIPRINI, S | |
dc.contributor.author | CLARK, C.J | |
hal.structure.identifier | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E] | |
hal.structure.identifier | Unité Scientifique de la Station de Nançay [USN] | |
dc.contributor.author | COGNARD, I | |
dc.contributor.author | CORONGIU, A | |
dc.contributor.author | ORESTANO, P. Cristarella | |
dc.contributor.author | CRNOGORCEVIC, M | |
dc.contributor.author | CUOCO, A | |
dc.contributor.author | CUTINI, S | |
dc.contributor.author | D'AMMANDO, F | |
dc.contributor.author | DE ANGELIS, A | |
dc.contributor.author | DECESAR, M.E | |
dc.contributor.author | DE GAETANO, S | |
dc.contributor.author | DE MENEZES, R | |
dc.contributor.author | DENEVA, J | |
dc.contributor.author | DE PALMA, F | |
dc.contributor.author | DI LALLA, N | |
dc.contributor.author | DIRIRSA, F | |
dc.contributor.author | DI VENERE, L | |
dc.contributor.author | DOMÍNGUEZ, A | |
hal.structure.identifier | Laboratoire de Physique des Deux Infinis Bordeaux [LP2I - Bordeaux] | |
dc.contributor.author | DUMORA, D | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | FEGAN, S.J | |
dc.contributor.author | FERRARA, E.C | |
dc.contributor.author | FIORI, A | |
dc.contributor.author | FLEISCHHACK, H | |
dc.contributor.author | FLYNN, C | |
dc.contributor.author | FRANCKOWIAK, A | |
dc.contributor.author | FREIRE, P.C.C | |
dc.contributor.author | FUKAZAWA, Y | |
dc.contributor.author | FUSCO, P | |
dc.contributor.author | GALANTI, G | |
dc.contributor.author | GAMMALDI, V | |
dc.contributor.author | GARGANO, F | |
dc.contributor.author | GASPARRINI, D | |
dc.contributor.author | GIACCHINO, F | |
dc.contributor.author | GIGLIETTO, N | |
dc.contributor.author | GIORDANO, F | |
dc.contributor.author | GIROLETTI, M | |
dc.contributor.author | GREEN, D | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | GRENIER, I.A | |
hal.structure.identifier | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E] | |
hal.structure.identifier | Unité Scientifique de la Station de Nançay [USN] | |
dc.contributor.author | GUILLEMOT, L | |
dc.contributor.author | GUIRIEC, S | |
dc.contributor.author | GUSTAFSSON, M | |
dc.contributor.author | HARDING, A.K | |
dc.contributor.author | HAYS, E | |
dc.contributor.author | HEWITT, J.W | |
hal.structure.identifier | Laboratoire Leprince-Ringuet [LLR] | |
dc.contributor.author | HORAN, D | |
dc.contributor.author | HOU, X | |
hal.structure.identifier | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E] | |
dc.contributor.author | JANKOWSKI, F | |
dc.contributor.author | JOHNSON, R.P | |
dc.contributor.author | JOHNSON, T.J | |
dc.contributor.author | JOHNSTON, S | |
dc.contributor.author | KATAOKA, J | |
dc.contributor.author | KEITH, M.J | |
dc.contributor.author | KERR, M | |
dc.contributor.author | KRAMER, M | |
dc.contributor.author | KUSS, M | |
dc.contributor.author | LATRONICO, L | |
dc.contributor.author | LEE, S.-H | |
dc.contributor.author | LI, D | |
dc.contributor.author | LI, J | |
dc.contributor.author | LIMYANSKY, B | |
dc.contributor.author | LONGO, F | |
dc.contributor.author | LOPARCO, F | |
dc.contributor.author | LORUSSO, L | |
dc.contributor.author | LOVELLETTE, M.N | |
dc.contributor.author | LOWER, M | |
dc.contributor.author | LUBRANO, P | |
dc.contributor.author | LYNE, A.G | |
dc.contributor.author | MAAN, Y | |
dc.contributor.author | MALDERA, S | |
dc.contributor.author | MANCHESTER, R.N | |
dc.contributor.author | MANFREDA, A | |
dc.contributor.author | MARELLI, M | |
dc.contributor.author | MARTÍ-DEVESA, G | |
dc.contributor.author | MAZZIOTTA, M.N | |
dc.contributor.author | MCENERY, J.E | |
dc.contributor.author | MEREU, I | |
dc.contributor.author | MICHELSON, P.F | |
dc.contributor.author | MICKALIGER, M | |
dc.contributor.author | MITTHUMSIRI, W | |
dc.contributor.author | MIZUNO, T | |
dc.contributor.author | MOISEEV, A.A | |
dc.contributor.author | MONZANI, M.E | |
dc.contributor.author | MORSELLI, A | |
dc.contributor.author | NEGRO, M | |
dc.contributor.author | NEMMEN, R | |
dc.contributor.author | NIEDER, L | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | NUSS, E | |
dc.contributor.author | OMODEI, N | |
dc.contributor.author | ORIENTI, M | |
dc.contributor.author | ORLANDO, E | |
dc.contributor.author | ORMES, J.F | |
dc.contributor.author | PALATIELLO, M | |
dc.contributor.author | PANEQUE, D | |
dc.contributor.author | PANZARINI, G | |
dc.contributor.author | PARTHASARATHY, A | |
dc.contributor.author | PERSIC, M | |
dc.contributor.author | PESCE-ROLLINS, M | |
dc.contributor.author | PILLERA, R | |
dc.contributor.author | POON, H | |
dc.contributor.author | PORTER, T.A | |
dc.contributor.author | POSSENTI, A | |
dc.contributor.author | PRINCIPE, G | |
dc.contributor.author | RAINO, S | |
dc.contributor.author | RANDO, R | |
dc.contributor.author | RANSOM, S.M | |
dc.contributor.author | RAY, P.S | |
dc.contributor.author | RAZZANO, M | |
dc.contributor.author | RAZZAQUE, S | |
dc.contributor.author | REIMER, A | |
dc.contributor.author | REIMER, O | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | RENAULT-TINACCI, N | |
dc.contributor.author | ROMANI, R.W | |
dc.contributor.author | SANCHEZ-CONDE, M | |
dc.contributor.author | PARKINSON, P.M. Saz | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | SCOTTON, L | |
dc.contributor.author | SERINI, D | |
dc.contributor.author | SGRO, C | |
dc.contributor.author | SHANNON, R | |
dc.contributor.author | SHARMA, V | |
dc.contributor.author | SHEN, Z | |
dc.contributor.author | SISKIND, E.J | |
dc.contributor.author | SPANDRE, G | |
dc.contributor.author | SPINELLI, P | |
dc.contributor.author | STAPPERS, B.W | |
dc.contributor.author | STEPHENS, T.E | |
dc.contributor.author | SUSON, D.J | |
dc.contributor.author | TABASSUM, S | |
dc.contributor.author | TAJIMA, H | |
dc.contributor.author | TAK, D | |
hal.structure.identifier | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E] | |
hal.structure.identifier | Unité Scientifique de la Station de Nançay [USN] | |
dc.contributor.author | THEUREAU, G | |
dc.contributor.author | THOMPSON, D.J | |
dc.contributor.author | TIBOLLA, O | |
dc.contributor.author | TORRES, D.F | |
dc.contributor.author | VALVERDE, J | |
dc.contributor.author | VENTER, C | |
dc.contributor.author | WADIASINGH, Z | |
dc.contributor.author | WANG, N | |
dc.contributor.author | WANG, P | |
dc.contributor.author | WELTEVREDE, P | |
dc.contributor.author | WOOD, K | |
dc.contributor.author | YAN, J | |
dc.contributor.author | ZAHARIJAS, G | |
dc.contributor.author | ZHANG, C | |
dc.contributor.author | ZHU, W | |
dc.date.issued | 2023 | |
dc.identifier.issn | 0004-637X | |
dc.description.abstractEn | We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected rotation ephemerides are achieved. A further dozen optical and/or X-ray binary systems co-located with LAT sources also likely harbor gamma-ray MSPs. This catalog thus reports roughly 340 gamma-ray pulsars and candidates, 10% of all known pulsars, compared to $\leq 11$ known before Fermi. Half of the gamma-ray pulsars are young. Of these, the half that are undetected in radio have a broader Galactic latitude distribution than the young radio-loud pulsars. The others are MSPs, with 6 undetected in radio. Overall, >235 are bright enough above 50 MeV to fit the pulse profile, the energy spectrum, or both. For the common two-peaked profiles, the gamma-ray peak closest to the magnetic pole crossing generally has a softer spectrum. The spectral energy distributions tend to narrow as the spindown power $\dot E$ decreases to its observed minimum near $10^{33}$ erg s$^{-1}$, approaching the shape for synchrotron radiation from monoenergetic electrons. We calculate gamma-ray luminosities when distances are available. Our all-sky gamma-ray sensitivity map is useful for population syntheses. The electronic catalog version provides gamma-ray pulsar ephemerides, properties and fit results to guide and be compared with modeling results. | |
dc.language.iso | en | |
dc.publisher | American Astronomical Society | |
dc.subject.en | X-ray: binary | |
dc.subject.en | gamma ray | |
dc.subject.en | pulsar | |
dc.subject.en | energy spectrum | |
dc.subject.en | GeV | |
dc.subject.en | synchrotron radiation | |
dc.subject.en | sensitivity | |
dc.subject.en | pole | |
dc.subject.en | spectral energy distribution | |
dc.subject.en | GLAST | |
dc.subject.en | electron | |
dc.subject.en | optical | |
dc.subject.en | crossing | |
dc.subject.en | rotation | |
dc.subject.en | galaxy | |
dc.title.en | The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars | |
dc.type | Article de revue | |
dc.identifier.doi | 10.3847/1538-4357/acee67 | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph] | |
dc.identifier.arxiv | 2307.11132 | |
bordeaux.journal | The Astrophysical Journal | |
bordeaux.page | 191 | |
bordeaux.volume | 958 | |
bordeaux.issue | 2 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-04179157 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-04179157v1 | |
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