Publication:
Search for Extended Sources in the Galactic Plane Using Six Years of Fermi-Large Area Telescope Pass 8 Data above 10 GeV

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dc.contributor.authorM. Ackermannen_US
dc.contributor.authorM. Ajelloen_US
dc.contributor.authorL. Baldinien_US
dc.contributor.authorJ. Balleten_US
dc.contributor.authorG. Barbiellinien_US
dc.contributor.authorD. Bastierien_US
dc.contributor.authorR. Bellazzinien_US
dc.contributor.authorE. Bissaldien_US
dc.contributor.authorE. D. Bloomen_US
dc.contributor.authorR. Boninoen_US
dc.contributor.authorE. Bottacinien_US
dc.contributor.authorT. J. Brandten_US
dc.contributor.authorJ. Bregeonen_US
dc.contributor.authorP. Bruelen_US
dc.contributor.authorR. Buehleren_US
dc.contributor.authorR. A. Cameronen_US
dc.contributor.authorM. Caragiuloen_US
dc.contributor.authorP. A. Caraveoen_US
dc.contributor.authorD. Castroen_US
dc.contributor.authorE. Cavazzutien_US
dc.contributor.authorC. Cecchien_US
dc.contributor.authorE. Charlesen_US
dc.contributor.authorA. Chekhtmanen_US
dc.contributor.authorC. C. Cheungen_US
dc.contributor.authorG. Chiaroen_US
dc.contributor.authorS. Ciprinien_US
dc.contributor.authorJ. M. Cohenen_US
dc.contributor.authorD. Costantinen_US
dc.contributor.authorF. Costanzaen_US
dc.contributor.authorS. Cutinien_US
dc.contributor.authorF. D'Ammandoen_US
dc.contributor.authorF. De Palmaen_US
dc.contributor.authorR. Desianteen_US
dc.contributor.authorS. W. Digelen_US
dc.contributor.authorN. Di Lallaen_US
dc.contributor.authorM. Di Mauroen_US
dc.contributor.authorL. Di Venereen_US
dc.contributor.authorC. Favuzzien_US
dc.contributor.authorS. J. Feganen_US
dc.contributor.authorE. C. Ferraraen_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.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.authorM. H. Grondinen_US
dc.contributor.authorL. Guillemoten_US
dc.contributor.authorS. Guiriecen_US
dc.contributor.authorA. K. Hardingen_US
dc.contributor.authorE. Haysen_US
dc.contributor.authorJ. W. Hewitten_US
dc.contributor.authorD. Horanen_US
dc.contributor.authorX. Houen_US
dc.contributor.authorG. Jóhannessonen_US
dc.contributor.authorT. Kamaeen_US
dc.contributor.authorM. Kussen_US
dc.contributor.authorG. La Muraen_US
dc.contributor.authorS. Larssonen_US
dc.contributor.authorM. Lemoine-Goumarden_US
dc.contributor.authorJ. Lien_US
dc.contributor.authorF. Longoen_US
dc.contributor.authorF. Loparcoen_US
dc.contributor.authorP. Lubranoen_US
dc.contributor.authorJ. D. Magillen_US
dc.contributor.authorS. Malderaen_US
dc.contributor.authorD. Malysheven_US
dc.contributor.authorA. Manfredaen_US
dc.contributor.authorM. N. Mazziottaen_US
dc.contributor.authorP. F. Michelsonen_US
dc.contributor.otherDeutsche Elektronen-Synchrotronen_US
dc.contributor.otherClemson Universityen_US
dc.contributor.otherUniversità di Pisaen_US
dc.contributor.otherUniversite Paris 7- Denis Dideroten_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Romaen_US
dc.contributor.otherUniversità degli Studi di Triesteen_US
dc.contributor.otherIstituto Nazionale Di Fisica Nucleare, Sezione di Padovaen_US
dc.contributor.otherUniversità degli Studi di Padovaen_US
dc.contributor.otherIstituto Nazionale Di Fisica Nucleare, Sezione di Pisaen_US
dc.contributor.otherKavli Institute for Particle Astrophysics and Cosmologyen_US
dc.contributor.otherUniversità degli Studi di Torinoen_US
dc.contributor.otherNASA Goddard Space Flight Centeren_US
dc.contributor.otherLaboratoire Univers et Particules de Montpellieren_US
dc.contributor.otherLaboratoire Leprince-Ringueten_US
dc.contributor.otherUniversità degli Studi di Barien_US
dc.contributor.otherINAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milanen_US
dc.contributor.otherAgenzia Spaziale Italianaen_US
dc.contributor.otherUniversità degli Studi di Perugiaen_US
dc.contributor.otherGeorge Mason University, Fairfax Campusen_US
dc.contributor.otherNaval Research Laboratoryen_US
dc.contributor.otherUniversity of Marylanden_US
dc.contributor.otherIstituto Di Radioastronomia, Bolognaen_US
dc.contributor.otherAlma Mater Studiorum Università di Bolognaen_US
dc.contributor.otherUniversità degli Studi di Napoli Federico IIen_US
dc.contributor.otherUniversità degli Studi di Udineen_US
dc.contributor.otherHiroshima Universityen_US
dc.contributor.otherErlangen Centre for Astroparticle Physicsen_US
dc.contributor.otherIN2P3 Institut National de Physique Nucleaire et de Physique des Particulesen_US
dc.contributor.otherUniversite d'Orleansen_US
dc.contributor.otherInstitut National des Sciences de l'Universen_US
dc.contributor.otherUniversity of North Floridaen_US
dc.contributor.otherChinese Academy of Sciencesen_US
dc.contributor.otherUniversity Science Institute Reykjaviken_US
dc.contributor.otherNordisk Institut for Teoretisk Atomtysiken_US
dc.contributor.otherUniversity of Tokyoen_US
dc.contributor.otherThe Royal Institute of Technology (KTH)en_US
dc.contributor.otherOskar Klein Centre for Cosmoparticle Physicsen_US
dc.contributor.otherUniversitat Autònoma de Barcelonaen_US
dc.contributor.otherMahidol Universityen_US
dc.contributor.otherUniversity of Denveren_US
dc.contributor.otherMax Planck Institut für Physik (Werner-Heisenberg-Institut)en_US
dc.contributor.otherOsservatorio Astronomico di Triesteen_US
dc.contributor.otherUniversity of Johannesburgen_US
dc.date.accessioned2018-12-21T07:27:03Z
dc.date.accessioned2019-03-14T08:03:32Z
dc.date.available2018-12-21T07:27:03Z
dc.date.available2019-03-14T08:03:32Z
dc.date.issued2017-07-10en_US
dc.description.abstract© 2017. The American Astronomical Society. All rights reserved.. The spatial extension of a γ-ray source is an essential ingredient to determine its spectral properties, as well as its potential multiwavelength counterpart. The capability to spatially resolve γ-ray sources is greatly improved by the newly delivered Fermi-Large Area Telescope (LAT) Pass 8 event-level analysis, which provides a greater acceptance and an improved point-spread function, two crucial factors for the detection of extended sources. Here, we present a complete search for extended sources located within 7° from the Galactic plane, using 6 yr of Fermi-LAT data above 10 GeV. We find 46 extended sources and provide their morphological and spectral characteristics. This constitutes the first catalog of hard Fermi-LAT extended sources, named the Fermi Galactic Extended Source Catalog, which allows a thorough study of the properties of the Galactic plane in the sub-TeV domain.en_US
dc.identifier.citationAstrophysical Journal. Vol.843, No.2 (2017)en_US
dc.identifier.doi10.3847/1538-4357/aa775aen_US
dc.identifier.issn15384357en_US
dc.identifier.issn0004637Xen_US
dc.identifier.other2-s2.0-85025111888en_US
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/123456789/42491
dc.rightsMahidol Universityen_US
dc.rights.holderSCOPUSen_US
dc.source.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85025111888&origin=inwarden_US
dc.subjectEarth and Planetary Sciencesen_US
dc.titleSearch for Extended Sources in the Galactic Plane Using Six Years of Fermi-Large Area Telescope Pass 8 Data above 10 GeVen_US
dc.typeArticleen_US
dspace.entity.typePublication
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85025111888&origin=inwarden_US

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