Publication: 2FHL: The SECOND CATALOG of HARD FERMI-LAT SOURCES
dc.contributor.author | M. Ackermann | en_US |
dc.contributor.author | M. Ajello | en_US |
dc.contributor.author | W. B. Atwood | en_US |
dc.contributor.author | L. Baldini | en_US |
dc.contributor.author | J. Ballet | en_US |
dc.contributor.author | G. Barbiellini | en_US |
dc.contributor.author | D. Bastieri | en_US |
dc.contributor.author | J. Becerra Gonzalez | en_US |
dc.contributor.author | R. Bellazzini | en_US |
dc.contributor.author | E. Bissaldi | en_US |
dc.contributor.author | R. D. Blandford | en_US |
dc.contributor.author | E. D. Bloom | en_US |
dc.contributor.author | R. Bonino | en_US |
dc.contributor.author | E. Bottacini | en_US |
dc.contributor.author | T. J. Brandt | en_US |
dc.contributor.author | J. Bregeon | en_US |
dc.contributor.author | P. Bruel | en_US |
dc.contributor.author | R. Buehler | en_US |
dc.contributor.author | S. Buson | en_US |
dc.contributor.author | G. A. Caliandro | en_US |
dc.contributor.author | R. A. Cameron | en_US |
dc.contributor.author | R. Caputo | en_US |
dc.contributor.author | M. Caragiulo | en_US |
dc.contributor.author | P. A. Caraveo | en_US |
dc.contributor.author | E. Cavazzuti | en_US |
dc.contributor.author | C. Cecchi | en_US |
dc.contributor.author | E. Charles | en_US |
dc.contributor.author | A. Chekhtman | en_US |
dc.contributor.author | C. C. Cheung | en_US |
dc.contributor.author | J. Chiang | en_US |
dc.contributor.author | G. Chiaro | en_US |
dc.contributor.author | S. Ciprini | en_US |
dc.contributor.author | J. M. Cohen | en_US |
dc.contributor.author | J. Cohen-Tanugi | en_US |
dc.contributor.author | L. R. Cominsky | en_US |
dc.contributor.author | J. Conrad | en_US |
dc.contributor.author | A. Cuoco | en_US |
dc.contributor.author | S. Cutini | en_US |
dc.contributor.author | F. D'Ammando | en_US |
dc.contributor.author | A. De Angelis | en_US |
dc.contributor.author | F. De Palma | en_US |
dc.contributor.author | R. Desiante | en_US |
dc.contributor.author | M. Di Mauro | en_US |
dc.contributor.author | L. Di Venere | en_US |
dc.contributor.author | A. Domínguez | en_US |
dc.contributor.author | P. S. Drell | en_US |
dc.contributor.author | C. Favuzzi | en_US |
dc.contributor.author | S. J. Fegan | en_US |
dc.contributor.author | E. C. Ferrara | en_US |
dc.contributor.author | W. B. Focke | en_US |
dc.contributor.author | P. Fortin | en_US |
dc.contributor.author | A. Franckowiak | en_US |
dc.contributor.author | Y. Fukazawa | en_US |
dc.contributor.author | S. Funk | en_US |
dc.contributor.author | A. K. Furniss | en_US |
dc.contributor.author | P. Fusco | en_US |
dc.contributor.author | F. Gargano | en_US |
dc.contributor.author | D. Gasparrini | en_US |
dc.contributor.author | N. Giglietto | en_US |
dc.contributor.author | P. Giommi | en_US |
dc.contributor.author | F. Giordano | en_US |
dc.contributor.author | M. Giroletti | en_US |
dc.contributor.author | T. Glanzman | en_US |
dc.contributor.author | G. Godfrey | en_US |
dc.contributor.author | I. A. Grenier | en_US |
dc.contributor.author | M. H. Grondin | en_US |
dc.contributor.author | L. Guillemot | en_US |
dc.contributor.author | S. Guiriec | en_US |
dc.contributor.author | A. K. Harding | en_US |
dc.contributor.author | E. Hays | en_US |
dc.contributor.author | J. W. Hewitt | en_US |
dc.contributor.author | A. B. Hill | en_US |
dc.contributor.author | D. Horan | en_US |
dc.contributor.other | Deutsche Elektronen-Synchrotron | en_US |
dc.contributor.other | Clemson University | en_US |
dc.contributor.other | Santa Cruz Institute for Particle Physics | en_US |
dc.contributor.other | Istituto Nazionale Di Fisica Nucleare, Sezione di Pisa | en_US |
dc.contributor.other | Kavli Institute for Particle Astrophysics and Cosmology | en_US |
dc.contributor.other | Institut de Recherche sur les Lois Fondamentales de l'Univers | en_US |
dc.contributor.other | Istituto Nazionale di Fisica Nucleare, Roma | en_US |
dc.contributor.other | Universita degli Studi di Trieste | en_US |
dc.contributor.other | Istituto Nazionale Di Fisica Nucleare, Sezione di Padova | en_US |
dc.contributor.other | Università degli Studi di Padova | en_US |
dc.contributor.other | NASA Goddard Space Flight Center | en_US |
dc.contributor.other | University of Maryland | en_US |
dc.contributor.other | Università degli Studi di Torino | en_US |
dc.contributor.other | Laboratoire Univers et Particules de Montpellier | en_US |
dc.contributor.other | Laboratoire Leprince-Ringuet | en_US |
dc.contributor.other | University of Maryland, Baltimore County | en_US |
dc.contributor.other | Consorzio Interuniversitario per la Fisica Spaziale (CIFS) | en_US |
dc.contributor.other | Università degli Studi di Bari | en_US |
dc.contributor.other | INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan | en_US |
dc.contributor.other | Agenzia Spaziale Italiana | en_US |
dc.contributor.other | Universita degli Studi di Perugia | en_US |
dc.contributor.other | George Mason University, Fairfax Campus | en_US |
dc.contributor.other | Naval Research Laboratory | en_US |
dc.contributor.other | Sonoma State University | en_US |
dc.contributor.other | Stockholms universitet | en_US |
dc.contributor.other | Oskar Klein Centre for Cosmoparticle Physics | en_US |
dc.contributor.other | Osservatorio Astronomico di Roma | en_US |
dc.contributor.other | Istituto Di Radioastronomia, Bologna | en_US |
dc.contributor.other | Alma Mater Studiorum Università di Bologna | en_US |
dc.contributor.other | Università degli Studi di Napoli Federico II | en_US |
dc.contributor.other | Universita degli Studi di Udine | en_US |
dc.contributor.other | Harvard-Smithsonian Center for Astrophysics | en_US |
dc.contributor.other | Hiroshima University | en_US |
dc.contributor.other | Erlangen Centre for Astroparticle Physics | en_US |
dc.contributor.other | IN2P3 Institut National de Physique Nucleaire et de Physique des Particules | en_US |
dc.contributor.other | Universite d'Orleans | en_US |
dc.contributor.other | Institut National des Sciences de l'Univers | en_US |
dc.contributor.other | University of North Florida | en_US |
dc.contributor.other | University of Southampton | en_US |
dc.contributor.other | Osservatorio Astronomico di Trieste | en_US |
dc.contributor.other | University Science Institute Reykjavik | en_US |
dc.contributor.other | University of Tokyo | en_US |
dc.contributor.other | Waseda University | en_US |
dc.contributor.other | CNRS Centre National de la Recherche Scientifique | en_US |
dc.contributor.other | Universite de Toulouse | en_US |
dc.contributor.other | Medizinische Universitat Innsbruck | en_US |
dc.contributor.other | The Royal Institute of Technology (KTH) | en_US |
dc.contributor.other | Universitat Autònoma de Barcelona | en_US |
dc.date.accessioned | 2018-12-11T02:44:55Z | |
dc.date.accessioned | 2019-03-14T08:04:39Z | |
dc.date.available | 2018-12-11T02:44:55Z | |
dc.date.available | 2019-03-14T08:04:39Z | |
dc.date.issued | 2016-01-01 | en_US |
dc.description.abstract | © 2016. The American Astronomical Society. All rights reserved. We present a catalog of sources detected above 50 GeV by the Fermi-Large Area Telescope (LAT) in 80 months of data. The newly delivered Pass 8 event-level analysis allows the detection and characterization of sources in the 50 GeV-2 TeV energy range. In this energy band, Fermi-LAT has detected 360 sources, which constitute the second catalog of hard Fermi-LAT sources (2FHL). The improved angular resolution enables the precise localization of point sources (∼1.′7 radius at 68% C. L.) and the detection and characterization of spatially extended sources. We find that 86% of the sources can be associated with counterparts at other wavelengths, of which the majority (75%) are active galactic nuclei and the rest (11%) are Galactic sources. Only 25% of the 2FHL sources have been previously detected by Cherenkov telescopes, implying that the 2FHL provides a reservoir of candidates to be followed up at very high energies. This work closes the energy gap between the observations performed at GeV energies by Fermi-LAT on orbit and the observations performed at higher energies by Cherenkov telescopes from the ground. | en_US |
dc.identifier.citation | Astrophysical Journal, Supplement Series. Vol.222, No.1 (2016) | en_US |
dc.identifier.doi | 10.3847/0067-0049/222/1/5 | en_US |
dc.identifier.issn | 00670049 | en_US |
dc.identifier.other | 2-s2.0-84955482407 | en_US |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/43594 | |
dc.rights | Mahidol University | en_US |
dc.rights.holder | SCOPUS | en_US |
dc.source.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84955482407&origin=inward | en_US |
dc.subject | Earth and Planetary Sciences | en_US |
dc.title | 2FHL: The SECOND CATALOG of HARD FERMI-LAT SOURCES | en_US |
dc.type | Article | en_US |
dspace.entity.type | Publication | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84955482407&origin=inward | en_US |