Search for Extended Sources in the Galactic Plane Using Six Years of Fermi-Large Area Telescope Pass 8 Data above 10 GeV
- Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany)
- Clemson Univ., Clemson, SC (United States)
- Univ. di Pisa and Istituto Nazionale di Fisica Nucleare, Pisa (Italy)
- Univ. Paris Diderot, Gif sur Yvette (France)
- Istituto Nazionale di Fisica Nucleare, Trieste (Italy); Univ. di Trieste, Trieste (Italy)
- Istituto Nazionale di Fisica Nucleare, Padova (Italy); Univ. di Padova, Padova (Italy)
- Istituto Nazionale de Fisica Nucleare, Pisa (Italy)
- Istituto Nazionale de Fisica Nucleare, Bari (Italy)
- Stanford Univ., Stanford, CA (United States)
- Istituto Nazionale di Fisica Nucleare, Torino (Italy); Univ. degli Studi di Torino, Torino (Italy)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Univ. Montpellier, Montpellier (France)
- Ecole Polytechnique, Palaiseau (France)
- Istituto Nazionale di Fisica Nucleare, Bari (Italy); "M. Merlin" dell'Univ. e del Politecnico di Bari, Bari (Italy)
- INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano, Milano (Italy)
- Agenzia Spaziale Italiana (ASI) Science Data Center, Roma (Italy)
- Istituto Nazionale di Fisica Nucleare, Perugia (Italy); Univ. degli Studi di Perugia, Perugia (Italy)
- George Mason Univ., Fairfax, VA (United States)
- Naval Research Lab., Washington, D.C. (United States)
- Univ. di Padova, Padova (Italy)
- Agenzia Spaziale Italiana (ASI) Science Data Center, Roma (Italy); Istituto Nazionale di Fisica Nucleare, Perugia (Italy)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland, College Park, MD (United States)
- Istituto Nazionale di Fisica Nucleare, Bari (Italy)
- INAF Istituto di Radioastronomia, Bologna (Italy); Univ. di Bologna, Bologna (Italy)
- Istituto Nazionale di Fisica Nucleare, Bari (Italy); Univ. Telematica Pegaso, Napoli (Italy)
- Istituto Nazionale di Fisica Nucleare, Torino (Italy); Univ. di Udine, Udine (Italy)
- Ecole polytechnique, Palaiseau (France)
- Hiroshima Univ., Hiroshima (Japan)
- Erlangen Centre for Astroparticle Physics, Erlangen (Germany)
- INAF Istituto di Radioastronomia, Bologna (Italy)
- Univ. Bordeaux, Gradignan Cedex (France)
- Univ. d'Orleans, Orleans Cedex (France); Observatoire de Paris, Nancay (France)
- Univ. of North Florida, Jacksonville, FL (United States)
- Chinese Academy of Sciences, Kunming (China); Chinese Academy of Sciences, Beijing (China)
- Univ. of Iceland, Reykjavik (Iceland); Nordita, Stockholm (Sweden)
- Univ. of Tokyo, Tokyo (Japan)
- Istituto Nazionale di Fisica Nucleare, Pisa (Italy)
- KTH Royal Institute of Technology, Stockholm (Sweden); The Oskar Klein Centre for Cosmoparticle Physics, Stockholm (Sweden)
- Institute of Space Sciences (IEEC-CSIC), Barcelona (Spain)
- Istituto Nazionale di Fisica Nucleare, Perugia (Italy)
- Univ. of Maryland, College Park, MD (United States)
- Istituto Nazionale di Fisica Nucleare, Torino (Italy)
- Mahidol Univ., Bangkok (Thailand)
- Istituto Nazionale di Fisica Nucleare, Roma (Italy)
- Univ. of Denver, Denver, CO (United States)
- Max-Planck-Institut fur Physik, Munchen (Germany)
- Istituto Nazionale di Fisica Nucleare, Trieste (Italy)
- Istituto Nazionale di Fisica Nucleare, Pisa (Italy);
- Univ. of Johannesburg, Auckland Park (South Africa)
- Leopold-Franzens-Univ. Innsbruck, Innsbruck (Austria); Stanford Univ., Stanford, CA (United States)
- NYCB Real-Time Computing Inc., Lattingtown, NY (United States)
- Purdue Univ. Calumet, Hammond, IN (United States)
- Institute of Space Sciences (IEEC-CSIC), Barcelona (Spain); Institucio Catalana de Recerca i Estudis Acancats (ICREA), Barcelona (Spain)
- Istituto Nazionale di Fisica Nucleare, Perugia (Italy); Univ. degli Studi di Perugia, Periugia (Italy)
- Praxis Inc., Alexandria, VA (United States)
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. As a result, 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.
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1374391
- Journal Information:
- The Astrophysical Journal (Online), Vol. 843, Issue 2; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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