Publication:
Catalog of Long-term Transient Sources in the First 10 yr of Fermi-LAT Data

dc.contributor.authorThe Fermi-Lat Collaborationen_US
dc.contributor.authorL. Baldinien_US
dc.contributor.authorJ. Balleten_US
dc.contributor.authorD. Bastierien_US
dc.contributor.authorJ. Becerra Gonzalezen_US
dc.contributor.authorR. Bellazzinien_US
dc.contributor.authorA. Berrettaen_US
dc.contributor.authorE. Bissaldien_US
dc.contributor.authorR. D. Blandforden_US
dc.contributor.authorE. D. Bloomen_US
dc.contributor.authorR. Boninoen_US
dc.contributor.authorE. Bottacinien_US
dc.contributor.authorP. Bruelen_US
dc.contributor.authorS. Busonen_US
dc.contributor.authorR. A. Cameronen_US
dc.contributor.authorP. A. Caraveoen_US
dc.contributor.authorE. Cavazzutien_US
dc.contributor.authorS. Chenen_US
dc.contributor.authorG. Chiaroen_US
dc.contributor.authorD. Ciangottinien_US
dc.contributor.authorN. Cibarioen_US
dc.contributor.authorS. Ciprinien_US
dc.contributor.authorP. Cristarella Orestanoen_US
dc.contributor.authorM. Crnogorcevicen_US
dc.contributor.authorS. Cutinien_US
dc.contributor.authorF. D'Ammandoen_US
dc.contributor.authorP. De La Torre Luqueen_US
dc.contributor.authorF. De Palmaen_US
dc.contributor.authorS. W. Digelen_US
dc.contributor.authorN. Di Lallaen_US
dc.contributor.authorF. Dirirsaen_US
dc.contributor.authorL. Di Venereen_US
dc.contributor.authorA. Domínguezen_US
dc.contributor.authorA. Fiorien_US
dc.contributor.authorH. Fleischhacken_US
dc.contributor.authorA. Franckowiaken_US
dc.contributor.authorY. Fukazawaen_US
dc.contributor.authorS. Funken_US
dc.contributor.authorP. Fuscoen_US
dc.contributor.authorF. Garganoen_US
dc.contributor.authorD. Gasparrinien_US
dc.contributor.authorS. Germanien_US
dc.contributor.authorN. Gigliettoen_US
dc.contributor.authorF. Giordanoen_US
dc.contributor.authorM. Girolettien_US
dc.contributor.authorD. Greenen_US
dc.contributor.authorI. A. Grenieren_US
dc.contributor.authorS. Griffinen_US
dc.contributor.authorS. Guiriecen_US
dc.contributor.authorM. Gustafssonen_US
dc.contributor.authorJ. W. Hewitten_US
dc.contributor.authorD. Horanen_US
dc.contributor.authorR. Imazawaen_US
dc.contributor.authorG. Jóhannessonen_US
dc.contributor.authorM. Kerren_US
dc.contributor.authorD. Kocevskien_US
dc.contributor.authorM. Kussen_US
dc.contributor.authorS. Larssonen_US
dc.contributor.authorL. Latronicoen_US
dc.contributor.authorJ. Lien_US
dc.contributor.authorI. Liodakisen_US
dc.contributor.authorF. Longoen_US
dc.contributor.authorF. Loparcoen_US
dc.contributor.authorM. N. Lovelletteen_US
dc.contributor.authorP. Lubranoen_US
dc.contributor.authorS. Malderaen_US
dc.contributor.authorA. Manfredaen_US
dc.contributor.authorG. Martí-Devesaen_US
dc.contributor.authorH. Matakeen_US
dc.contributor.authorM. N. Mazziottaen_US
dc.contributor.authorI. Mereuen_US
dc.contributor.authorM. Meyeren_US
dc.contributor.authorN. Mirabalen_US
dc.contributor.authorW. Mitthumsirien_US
dc.contributor.authorT. Mizunoen_US
dc.contributor.authorM. E. Monzanien_US
dc.contributor.authorA. Morsellien_US
dc.contributor.authorI. V. Moskalenkoen_US
dc.contributor.authorS. Nagasawaen_US
dc.contributor.authorM. Negroen_US
dc.contributor.authorR. Ojhaen_US
dc.contributor.authorM. Orientien_US
dc.contributor.authorE. Orlandoen_US
dc.contributor.authorM. Palatielloen_US
dc.contributor.authorV. Paliyaen_US
dc.contributor.authorD. Panequeen_US
dc.contributor.authorZ. Peien_US
dc.contributor.authorM. Persicen_US
dc.contributor.authorM. Pesce-Rollinsen_US
dc.contributor.authorV. Petrosianen_US
dc.contributor.authorH. Poonen_US
dc.contributor.authorT. A. Porteren_US
dc.contributor.authorG. Principeen_US
dc.contributor.authorJ. L. Racusinen_US
dc.contributor.authorS. Rainen_US
dc.contributor.authorR. Randoen_US
dc.contributor.authorB. Ranien_US
dc.contributor.authorM. Razzanoen_US
dc.contributor.authorS. Razzaqueen_US
dc.contributor.authorA. Reimeren_US
dc.contributor.otherOskar Klein Centreen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Triesteen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Perugiaen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Lecceen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Barien_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergataen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Torinoen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Pisaen_US
dc.contributor.otherIstituto Nazionale Di Fisica Nucleare, Sezione di Padovaen_US
dc.contributor.otherUniversite Paris-Saclayen_US
dc.contributor.otherAryabhatta Research Institute of Observational Sciencesen_US
dc.contributor.otherINAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milanen_US
dc.contributor.otherKorea Astronomy and Space Science Instituteen_US
dc.contributor.otherRaunvísindastofnun Háskólansen_US
dc.contributor.otherAgenzia Spaziale Italianaen_US
dc.contributor.otherGeorg-August-Universität Göttingenen_US
dc.contributor.otherHiroshima Universityen_US
dc.contributor.otherDeutsches Elektronen-Synchrotron (DESY)en_US
dc.contributor.otherOsservatorio Astronomico di Triesteen_US
dc.contributor.otherUniversità di Pisaen_US
dc.contributor.otherPolitecnico di Barien_US
dc.contributor.otherUniversidad Complutense de Madriden_US
dc.contributor.otherNaval Research Laboratoryen_US
dc.contributor.otherUniversità degli Studi di Udineen_US
dc.contributor.otherSLAC National Accelerator Laboratoryen_US
dc.contributor.otherThe University of Tokyoen_US
dc.contributor.otherUniversity of Maryland, Baltimore County (UMBC)en_US
dc.contributor.otherUniversita del Salentoen_US
dc.contributor.otherCatholic University of Americaen_US
dc.contributor.otherAmerican Universityen_US
dc.contributor.otherUniversity of Maryland, College Parken_US
dc.contributor.otherUniversité Savoie Mont Blancen_US
dc.contributor.otherUniversità degli Studi di Triesteen_US
dc.contributor.otherHögskolan Dalarnaen_US
dc.contributor.otherÉcole polytechniqueen_US
dc.contributor.otherMahidol Universityen_US
dc.contributor.otherJulius-Maximilians-Universität Würzburgen_US
dc.contributor.otherIstituto Di Radioastronomia, Bolognaen_US
dc.contributor.otherUniversità degli Studi di Torinoen_US
dc.contributor.otherNASA Marshall Space Flight Centeren_US
dc.contributor.otherInstituto Astrofisico de Canariasen_US
dc.contributor.otherUniversität Innsbrucken_US
dc.contributor.otherMax Planck Institute for Physics (Werner Heisenberg Institute)en_US
dc.contributor.otherTurun yliopistoen_US
dc.contributor.otherNASA Goddard Space Flight Centeren_US
dc.contributor.otherRuhr-Universitat Bochumen_US
dc.contributor.otherThe George Washington Universityen_US
dc.contributor.otherUniversità degli Studi di Perugiaen_US
dc.contributor.otherThe Royal Institute of Technology (KTH)en_US
dc.contributor.otherFriedrich-Alexander-Universität Erlangen-Nürnbergen_US
dc.contributor.otherUniversity of Johannesburgen_US
dc.contributor.otherUniversità degli Studi di Padovaen_US
dc.contributor.otherUniversity of North Floridaen_US
dc.date.accessioned2022-08-04T08:31:58Z
dc.date.available2022-08-04T08:31:58Z
dc.date.issued2021-09-01en_US
dc.description.abstractWe present the first Fermi Large Area Telescope (LAT) catalog of long-term γ-ray transient sources (1FLT). This comprises sources that were detected on monthly time intervals during the first decade of Fermi-LAT operations. The monthly timescale allows us to identify transient and variable sources that were not yet reported in other Fermi-LAT catalogs. The monthly data sets were analyzed using a wavelet-based source detection algorithm that provided the candidate new transient sources. The search was limited to the extragalactic regions of the sky to avoid the dominance of the Galactic diffuse emission at low Galactic latitudes. The transient candidates were then analyzed using the standard Fermi-LAT maximum likelihood analysis method. All sources detected with a statistical significance above 4σ in at least one monthly bin were listed in the final catalog. The 1FLT catalog contains 142 transient γ-ray sources that are not included in the 4FGL-DR2 catalog. Many of these sources (102) have been confidently associated with active galactic nuclei (AGNs): 24 are associated with flat-spectrum radio quasars, 1 with a BL Lac object, 70 with blazars of uncertain type, 3 with radio galaxies, 1 with a compact steep-spectrum radio source, 1 with a steep-spectrum radio quasar, and 2 with AGNs of other types. The remaining 40 sources have no candidate counterparts at other wavelengths. The median γ-ray spectral index of the 1FLT-AGN sources is softer than that reported in the latest Fermi-LAT AGN general catalog. This result is consistent with the hypothesis that detection of the softest γ-ray emitters is less efficient when the data are integrated over year-long intervals.en_US
dc.identifier.citationAstrophysical Journal, Supplement Series. Vol.256, No.1 (2021)en_US
dc.identifier.doi10.3847/1538-4365/ac072aen_US
dc.identifier.issn00670049en_US
dc.identifier.other2-s2.0-85115816543en_US
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/76850
dc.rightsMahidol Universityen_US
dc.rights.holderSCOPUSen_US
dc.source.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85115816543&origin=inwarden_US
dc.subjectEarth and Planetary Sciencesen_US
dc.subjectPhysics and Astronomyen_US
dc.titleCatalog of Long-term Transient Sources in the First 10 yr of Fermi-LAT Dataen_US
dc.typeArticleen_US
dspace.entity.typePublication
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85115816543&origin=inwarden_US

Files

Collections