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The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

hal.structure.identifierLaboratoire de Physique des Deux Infinis Bordeaux [LP2I - Bordeaux]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorSMITH, D.A
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorABDOLLAHI, S
dc.contributor.authorAJELLO, M
dc.contributor.authorBAILES, M
dc.contributor.authorBALDINI, L
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorBALLET, J
dc.contributor.authorBARING, M.G
dc.contributor.authorBASSA, C
dc.contributor.authorGONZALEZ, J. Becerra
dc.contributor.authorBELLAZZINI, R
dc.contributor.authorBERRETTA, A
dc.contributor.authorBHATTACHARYYA, B
dc.contributor.authorBISSALDI, E
dc.contributor.authorBONINO, R
dc.contributor.authorBOTTACINI, E
hal.structure.identifierLaboratoire de Physique Subatomique et de Cosmologie [LPSC]
dc.contributor.authorBREGEON, J
hal.structure.identifierLaboratoire Leprince-Ringuet [LLR]
dc.contributor.authorBRUEL, P
dc.contributor.authorBURGAY, M
dc.contributor.authorBURNETT, T.H
dc.contributor.authorCAMERON, R.A
dc.contributor.authorCAMILO, F
dc.contributor.authorCAPUTO, R
dc.contributor.authorCARAVEO, P.A
dc.contributor.authorCAVAZZUTI, E
dc.contributor.authorCHIARO, G
dc.contributor.authorCIPRINI, S
dc.contributor.authorCLARK, C.J
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
dc.contributor.authorCOGNARD, I
dc.contributor.authorCORONGIU, A
dc.contributor.authorORESTANO, P. Cristarella
dc.contributor.authorCRNOGORCEVIC, M
dc.contributor.authorCUOCO, A
dc.contributor.authorCUTINI, S
dc.contributor.authorD'AMMANDO, F
dc.contributor.authorDE ANGELIS, A
dc.contributor.authorDECESAR, M.E
dc.contributor.authorDE GAETANO, S
dc.contributor.authorDE MENEZES, R
dc.contributor.authorDENEVA, J
dc.contributor.authorDE PALMA, F
dc.contributor.authorDI LALLA, N
dc.contributor.authorDIRIRSA, F
dc.contributor.authorDI VENERE, L
dc.contributor.authorDOMÍNGUEZ, A
hal.structure.identifierLaboratoire de Physique des Deux Infinis Bordeaux [LP2I - Bordeaux]
dc.contributor.authorDUMORA, D
hal.structure.identifierLaboratoire Leprince-Ringuet [LLR]
dc.contributor.authorFEGAN, S.J
dc.contributor.authorFERRARA, E.C
dc.contributor.authorFIORI, A
dc.contributor.authorFLEISCHHACK, H
dc.contributor.authorFLYNN, C
dc.contributor.authorFRANCKOWIAK, A
dc.contributor.authorFREIRE, P.C.C
dc.contributor.authorFUKAZAWA, Y
dc.contributor.authorFUSCO, P
dc.contributor.authorGALANTI, G
dc.contributor.authorGAMMALDI, V
dc.contributor.authorGARGANO, F
dc.contributor.authorGASPARRINI, D
dc.contributor.authorGIACCHINO, F
dc.contributor.authorGIGLIETTO, N
dc.contributor.authorGIORDANO, F
dc.contributor.authorGIROLETTI, M
dc.contributor.authorGREEN, D
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorGRENIER, I.A
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
dc.contributor.authorGUILLEMOT, L
dc.contributor.authorGUIRIEC, S
dc.contributor.authorGUSTAFSSON, M
dc.contributor.authorHARDING, A.K
dc.contributor.authorHAYS, E
dc.contributor.authorHEWITT, J.W
hal.structure.identifierLaboratoire Leprince-Ringuet [LLR]
dc.contributor.authorHORAN, D
dc.contributor.authorHOU, X
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
dc.contributor.authorJANKOWSKI, F
dc.contributor.authorJOHNSON, R.P
dc.contributor.authorJOHNSON, T.J
dc.contributor.authorJOHNSTON, S
dc.contributor.authorKATAOKA, J
dc.contributor.authorKEITH, M.J
dc.contributor.authorKERR, M
dc.contributor.authorKRAMER, M
dc.contributor.authorKUSS, M
dc.contributor.authorLATRONICO, L
dc.contributor.authorLEE, S.-H
dc.contributor.authorLI, D
dc.contributor.authorLI, J
dc.contributor.authorLIMYANSKY, B
dc.contributor.authorLONGO, F
dc.contributor.authorLOPARCO, F
dc.contributor.authorLORUSSO, L
dc.contributor.authorLOVELLETTE, M.N
dc.contributor.authorLOWER, M
dc.contributor.authorLUBRANO, P
dc.contributor.authorLYNE, A.G
dc.contributor.authorMAAN, Y
dc.contributor.authorMALDERA, S
dc.contributor.authorMANCHESTER, R.N
dc.contributor.authorMANFREDA, A
dc.contributor.authorMARELLI, M
dc.contributor.authorMARTÍ-DEVESA, G
dc.contributor.authorMAZZIOTTA, M.N
dc.contributor.authorMCENERY, J.E
dc.contributor.authorMEREU, I
dc.contributor.authorMICHELSON, P.F
dc.contributor.authorMICKALIGER, M
dc.contributor.authorMITTHUMSIRI, W
dc.contributor.authorMIZUNO, T
dc.contributor.authorMOISEEV, A.A
dc.contributor.authorMONZANI, M.E
dc.contributor.authorMORSELLI, A
dc.contributor.authorNEGRO, M
dc.contributor.authorNEMMEN, R
dc.contributor.authorNIEDER, L
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorNUSS, E
dc.contributor.authorOMODEI, N
dc.contributor.authorORIENTI, M
dc.contributor.authorORLANDO, E
dc.contributor.authorORMES, J.F
dc.contributor.authorPALATIELLO, M
dc.contributor.authorPANEQUE, D
dc.contributor.authorPANZARINI, G
dc.contributor.authorPARTHASARATHY, A
dc.contributor.authorPERSIC, M
dc.contributor.authorPESCE-ROLLINS, M
dc.contributor.authorPILLERA, R
dc.contributor.authorPOON, H
dc.contributor.authorPORTER, T.A
dc.contributor.authorPOSSENTI, A
dc.contributor.authorPRINCIPE, G
dc.contributor.authorRAINO, S
dc.contributor.authorRANDO, R
dc.contributor.authorRANSOM, S.M
dc.contributor.authorRAY, P.S
dc.contributor.authorRAZZANO, M
dc.contributor.authorRAZZAQUE, S
dc.contributor.authorREIMER, A
dc.contributor.authorREIMER, O
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorRENAULT-TINACCI, N
dc.contributor.authorROMANI, R.W
dc.contributor.authorSANCHEZ-CONDE, M
dc.contributor.authorPARKINSON, P.M. Saz
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorSCOTTON, L
dc.contributor.authorSERINI, D
dc.contributor.authorSGRO, C
dc.contributor.authorSHANNON, R
dc.contributor.authorSHARMA, V
dc.contributor.authorSHEN, Z
dc.contributor.authorSISKIND, E.J
dc.contributor.authorSPANDRE, G
dc.contributor.authorSPINELLI, P
dc.contributor.authorSTAPPERS, B.W
dc.contributor.authorSTEPHENS, T.E
dc.contributor.authorSUSON, D.J
dc.contributor.authorTABASSUM, S
dc.contributor.authorTAJIMA, H
dc.contributor.authorTAK, D
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
dc.contributor.authorTHEUREAU, G
dc.contributor.authorTHOMPSON, D.J
dc.contributor.authorTIBOLLA, O
dc.contributor.authorTORRES, D.F
dc.contributor.authorVALVERDE, J
dc.contributor.authorVENTER, C
dc.contributor.authorWADIASINGH, Z
dc.contributor.authorWANG, N
dc.contributor.authorWANG, P
dc.contributor.authorWELTEVREDE, P
dc.contributor.authorWOOD, K
dc.contributor.authorYAN, J
dc.contributor.authorZAHARIJAS, G
dc.contributor.authorZHANG, C
dc.contributor.authorZHU, W
dc.date.issued2023
dc.description.abstractEnWe 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.isoen
dc.subject.enX-ray: binary
dc.subject.engamma ray
dc.subject.enpulsar
dc.subject.enenergy spectrum
dc.subject.enGeV
dc.subject.ensynchrotron radiation
dc.subject.ensensitivity
dc.subject.enpole
dc.subject.enspectral energy distribution
dc.subject.enGLAST
dc.subject.enelectron
dc.subject.enoptical
dc.subject.encrossing
dc.subject.enrotation
dc.subject.engalaxy
dc.title.enThe Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
dc.typeArticle de revue
dc.identifier.doi10.3847/1538-4357/acee67
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv2307.11132
bordeaux.journalAstrophys.J
bordeaux.page191
bordeaux.volume958
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-04179157
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04179157v1
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