Incremental Fermi Large Area Telescope Fourth Source Catalog

dc.contributor.authorAbdollahi S.
dc.contributor.authorAcero F.
dc.contributor.authorBaldini L.
dc.contributor.authorBallet J.
dc.contributor.authorBastieri D.
dc.contributor.authorBellazzini R.
dc.contributor.authorBerenji B.
dc.contributor.authorBerretta A.
dc.contributor.authorBissaldi E.
dc.contributor.authorBlandford R.D.
dc.contributor.authorBloom E.
dc.contributor.authorBonino R.
dc.contributor.authorBrill A.
dc.contributor.authorBritto R.J.
dc.contributor.authorBruel P.
dc.contributor.authorBurnett T.H.
dc.contributor.authorBuson S.
dc.contributor.authorCameron R.A.
dc.contributor.authorCaputo R.
dc.contributor.authorCaraveo P.A.
dc.contributor.authorCastro D.
dc.contributor.authorChaty S.
dc.contributor.authorCheung C.C.
dc.contributor.authorChiaro G.
dc.contributor.authorCibrario N.
dc.contributor.authorCiprini S.
dc.contributor.authorCoronado-Blázquez J.
dc.contributor.authorCrnogorcevic M.
dc.contributor.authorCutini S.
dc.contributor.authorD'Ammando F.
dc.contributor.authorDe Gaetano S.
dc.contributor.authorDigel S.W.
dc.contributor.authorDi Lalla N.
dc.contributor.authorDirirsa F.
dc.contributor.authorDi Venere L.
dc.contributor.authorDomínguez A.
dc.contributor.authorFallah Ramazani V.
dc.contributor.authorFegan S.J.
dc.contributor.authorFerrara E.C.
dc.contributor.authorFiori A.
dc.contributor.authorFleischhack H.
dc.contributor.authorFranckowiak A.
dc.contributor.authorFukazawa Y.
dc.contributor.authorFunk S.
dc.contributor.authorFusco P.
dc.contributor.authorGalanti G.
dc.contributor.authorGammaldi V.
dc.contributor.authorGargano F.
dc.contributor.authorGarrappa S.
dc.contributor.authorGasparrini D.
dc.contributor.authorGiacchino F.
dc.contributor.authorGiglietto N.
dc.contributor.authorGiordano F.
dc.contributor.authorGiroletti M.
dc.contributor.authorGlanzman T.
dc.contributor.authorGreen D.
dc.contributor.authorGrenier I.A.
dc.contributor.authorGrondin M.H.
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.
dc.contributor.authorHoran D.
dc.contributor.authorHou X.
dc.contributor.authorJóhannesson G.
dc.contributor.authorKarwin C.
dc.contributor.authorKayanoki T.
dc.contributor.authorKerr M.
dc.contributor.authorKuss M.
dc.contributor.authorLandriu D.
dc.contributor.authorLarsson S.
dc.contributor.authorLatronico L.
dc.contributor.authorLemoine-Goumard M.
dc.contributor.authorLi J.
dc.contributor.authorLiodakis I.
dc.contributor.authorLongo F.
dc.contributor.authorLoparco F.
dc.contributor.authorLott B.
dc.contributor.authorLubrano P.
dc.contributor.authorMaldera S.
dc.contributor.authorMalyshev D.
dc.contributor.authorManfreda A.
dc.contributor.authorMartí-Devesa G.
dc.contributor.authorMazziotta M.N.
dc.contributor.authorMereu I.
dc.contributor.authorMeyer M.
dc.contributor.authorMichelson P.F.
dc.contributor.authorMirabal N.
dc.contributor.authorMitthumsiri W.
dc.contributor.authorMizuno T.
dc.contributor.authorMoiseev A.A.
dc.contributor.authorMonzani M.E.
dc.contributor.authorMorselli A.
dc.contributor.authorMoskalenko I.V.
dc.contributor.authorNegro M.
dc.contributor.authorNuss E.
dc.contributor.authorOmodei N.
dc.contributor.authorOrienti M.
dc.contributor.otherMahidol University
dc.date.accessioned2023-06-18T17:07:20Z
dc.date.available2023-06-18T17:07:20Z
dc.date.issued2022-06-01
dc.description.abstractWe present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi Large Area Telescope (LAT) catalog of 3-ray sources. Based on the first 12 years of science data in the energy range from 50 MeV to 1 TeV, it contains 6658 sources. The analysis improves on that used for the 4FGL catalog over eight years of data: more sources are fit with curved spectra, we introduce a more robust spectral parameterization for pulsars, and we extend the spectral points to 1 TeV. The spectral parameters, spectral energy distributions, and associations are updated for all sources. Light curves are rebuilt for all sources with 1 yr intervals (not 2 month intervals). Among the 5064 original 4FGL sources, 16 were deleted, 112 are formally below the detection threshold over 12 yr (but are kept in the list), while 74 are newly associated, 10 have an improved association, and seven associations were withdrawn. Pulsars are split explicitly between young and millisecond pulsars. Pulsars and binaries newly detected in LAT sources, as well as more than 100 newly classified blazars, are reported. We add three extended sources and 1607 new point sources, mostly just above the detection threshold, among which eight are considered identified, and 699 have a plausible counterpart at other wavelengths. We discuss the degree-scale residuals to the global sky model and clusters of soft unassociated point sources close to the Galactic plane, which are possibly related to limitations of the interstellar emission model and missing extended sources.
dc.identifier.citationAstrophysical Journal, Supplement Series Vol.260 No.2 (2022)
dc.identifier.doi10.3847/1538-4365/ac6751
dc.identifier.issn00670049
dc.identifier.scopus2-s2.0-85134542146
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/84499
dc.rights.holderSCOPUS
dc.subjectEarth and Planetary Sciences
dc.titleIncremental Fermi Large Area Telescope Fourth Source Catalog
dc.typeArticle
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85134542146&origin=inward
oaire.citation.issue2
oaire.citation.titleAstrophysical Journal, Supplement Series
oaire.citation.volume260
oairecerif.author.affiliationOskar Klein Centre
oairecerif.author.affiliationYunnan Observatories
oairecerif.author.affiliationIstituto Nazionale di Fisica Nucleare, Sezione di Trieste
oairecerif.author.affiliationIstituto Nazionale di Fisica Nucleare, Sezione di Perugia
oairecerif.author.affiliationIstituto Nazionale di Fisica Nucleare, Sezione di Bari
oairecerif.author.affiliationIstituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata
oairecerif.author.affiliationIstituto Nazionale di Fisica Nucleare, Sezione di Torino
oairecerif.author.affiliationIstituto Nazionale di Fisica Nucleare, Sezione di Pisa
oairecerif.author.affiliationIstituto Nazionale Di Fisica Nucleare, Sezione di Padova
oairecerif.author.affiliationLaboratoire Univers et Particules de Montpellier
oairecerif.author.affiliationUniversité Paris-Saclay
oairecerif.author.affiliationUniversité de Bordeaux
oairecerif.author.affiliationINAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
oairecerif.author.affiliationRaunvísindastofnun Háskólans
oairecerif.author.affiliationAgenzia Spaziale Italiana
oairecerif.author.affiliationGeorg-August-Universität Göttingen
oairecerif.author.affiliationHiroshima University
oairecerif.author.affiliationCalifornia State University, Los Angeles
oairecerif.author.affiliationDeutsches Elektronen-Synchrotron (DESY)
oairecerif.author.affiliationUniversité d'Orléans
oairecerif.author.affiliationUniversità di Pisa
oairecerif.author.affiliationStockholms universitet
oairecerif.author.affiliationPolitecnico di Bari
oairecerif.author.affiliationUniversidad Complutense de Madrid
oairecerif.author.affiliationNaval Research Laboratory
oairecerif.author.affiliationUniversité Toulouse III - Paul Sabatier
oairecerif.author.affiliationUniversidad Autónoma de Madrid
oairecerif.author.affiliationClemson University
oairecerif.author.affiliationSLAC National Accelerator Laboratory
oairecerif.author.affiliationUniversity of Maryland, Baltimore County (UMBC)
oairecerif.author.affiliationHarvard-Smithsonian Center for Astrophysics
oairecerif.author.affiliationCatholic University of America
oairecerif.author.affiliationUniversity of Maryland, College Park
oairecerif.author.affiliationChinese Academy of Sciences
oairecerif.author.affiliationUniversity of Science and Technology of China
oairecerif.author.affiliationUniversità degli Studi di Trieste
oairecerif.author.affiliationUniversity of the Free State
oairecerif.author.affiliationUniversity of Washington
oairecerif.author.affiliationHögskolan Dalarna
oairecerif.author.affiliationÉcole polytechnique
oairecerif.author.affiliationMahidol University
oairecerif.author.affiliationJulius-Maximilians-Universität Würzburg
oairecerif.author.affiliationIstituto Di Radioastronomia, Bologna
oairecerif.author.affiliationUniversità degli Studi di Torino
oairecerif.author.affiliationUniversität Innsbruck
oairecerif.author.affiliationMax Planck Institute for Physics (Werner Heisenberg Institute)
oairecerif.author.affiliationCNRS Centre National de la Recherche Scientifique
oairecerif.author.affiliationTurun yliopisto
oairecerif.author.affiliationNASA Goddard Space Flight Center
oairecerif.author.affiliationLos Alamos National Laboratory
oairecerif.author.affiliationRuhr-Universitat Bochum
oairecerif.author.affiliationThe George Washington University
oairecerif.author.affiliationUniversità degli Studi di Perugia
oairecerif.author.affiliationThe Royal Institute of Technology (KTH)
oairecerif.author.affiliationFriedrich-Alexander-Universität Erlangen-Nürnberg
oairecerif.author.affiliationUniversità degli Studi di Padova
oairecerif.author.affiliationUniversity of North Florida
oairecerif.author.affiliationEthiopian Space Science and Technology Institute

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