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 RD
dc.contributor.authorBloom E
dc.contributor.authorBonino R
dc.contributor.authorBrill A
dc.contributor.authorBritto RJ
dc.contributor.authorBruel P
dc.contributor.authorBurnett TH
dc.contributor.authorBuson S
dc.contributor.authorCameron RA
dc.contributor.authorCaputo R
dc.contributor.authorCaraveo PA
dc.contributor.authorCastro D
dc.contributor.authorChaty S
dc.contributor.authorCheung CC
dc.contributor.authorChiaro G
dc.contributor.authorCibrario N
dc.contributor.authorCiprini S
dc.contributor.authorCoronado-Blazquez J
dc.contributor.authorCrnogorcevic M
dc.contributor.authorCutini S
dc.contributor.authorD'Ammando F
dc.contributor.authorDe Gaetano S
dc.contributor.authorDigel SW
dc.contributor.authorDi Lalla N
dc.contributor.authorDirirsa F
dc.contributor.authorDi Venere L
dc.contributor.authorDominguez A
dc.contributor.authorRamazani VF
dc.contributor.authorFegan SJ
dc.contributor.authorFerrara EC
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 IA
dc.contributor.authorGrondin MH
dc.contributor.authorGuillemot L
dc.contributor.authorGuiriec S
dc.contributor.authorGustafsson M
dc.contributor.authorHarding AK
dc.contributor.authorHays E
dc.contributor.authorHewitt JW
dc.contributor.authorHoran D
dc.contributor.authorHou X
dc.contributor.authorJohannesson 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.authorMarti-Devesa G
dc.contributor.authorMazziotta MN
dc.contributor.authorMereu I
dc.contributor.authorMeyer M
dc.contributor.authorMichelson PF
dc.contributor.authorMirabal N
dc.contributor.authorMitthumsiri W
dc.contributor.authorMizuno T
dc.contributor.authorMoiseev AA
dc.contributor.authorMonzani ME
dc.contributor.authorMorselli A
dc.contributor.authorMoskalenko IV
dc.contributor.authorNegro M
dc.contributor.authorNuss E
dc.contributor.authorOmodei N
dc.contributor.authorOrienti M
dc.contributor.authorOrlando E
dc.contributor.authorPaneque D
dc.contributor.authorPei Z
dc.contributor.authorPerkins JS
dc.contributor.authorPersic M
dc.contributor.authorPesce-Rollins M
dc.contributor.authorPetrosian V
dc.contributor.authorPillera R
dc.contributor.authorPoon H
dc.contributor.authorPorter TA
dc.contributor.authorPrincipe G
dc.contributor.authorRaino S
dc.contributor.authorRando R
dc.contributor.authorRani B
dc.contributor.authorRazzano M
dc.contributor.authorRazzaque S
dc.contributor.authorReimer A
dc.contributor.authorReimer O
dc.contributor.authorReposeur T
dc.contributor.authorSanchez-Conde M
dc.contributor.authorParkinson PMS
dc.contributor.authorScotton L
dc.contributor.authorSerini D
dc.contributor.authorSgro C
dc.contributor.authorSiskind EJ
dc.contributor.authorSmith DA
dc.contributor.authorSpandre G
dc.contributor.authorSpinelli P
dc.contributor.authorSueoka K
dc.contributor.authorSuson DJ
dc.contributor.authorTajima H
dc.contributor.authorTak D
dc.contributor.authorThayer JB
dc.contributor.authorThompson DJ
dc.contributor.authorTorres DF
dc.contributor.authorTroja E
dc.contributor.authorValverde J
dc.contributor.authorWood K
dc.contributor.authorZaharijas G
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.converis.publication-id175935529
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/175935529
dc.date.accessioned2022-10-27T12:12:44Z
dc.date.available2022-10-27T12:12:44Z
dc.description.abstractWe present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi Large Area Telescope (LAT) catalog of gamma-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.jour-issn0067-0049
dc.identifier.olddbid173952
dc.identifier.oldhandle10024/157046
dc.identifier.urihttps://www.utupub.fi/handle/11111/33306
dc.identifier.urlhttps://iopscience.iop.org/article/10.3847/1538-4365/ac6751
dc.identifier.urnURN:NBN:fi-fe2022091258468
dc.language.isoen
dc.okm.affiliatedauthorLiodakis, Yannis
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherIOP Publishing Ltd
dc.publisher.countryUnited Kingdomen_GB
dc.publisher.countryBritanniafi_FI
dc.publisher.country-codeGB
dc.relation.articlenumber53
dc.relation.doi10.3847/1538-4365/ac6751
dc.relation.ispartofjournalAstrophysical Journal Supplement
dc.relation.issue2
dc.relation.volume260
dc.source.identifierhttps://www.utupub.fi/handle/10024/157046
dc.titleIncremental Fermi Large Area Telescope Fourth Source Catalog
dc.year.issued2022

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