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  • 1. Abdollahi, S.
    et al.
    Acero, F.
    Ackermann, M.
    Ajello, M.
    Atwood, W. B.
    Axelsson, M.
    Baldini, L.
    Ballet, J.
    Larsson, Stefan
    Dalarna University, School of Education, Health and Social Studies, Natural Science. KTH Royal Inst Technol / AlbaNova, Oskar Klein Ctr Cosmoparticle Phys.
    Zaharijas, G.
    Fermi Large Area Telescope Fourth Source Catalog2020In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 247, no 1, article id 33Article in journal (Refereed)
    Abstract [en]

    We present the fourth Fermi Large Area Telescope catalog (4FGL) of gamma-ray sources. Based on the first eight years of science data from the Fermi Gamma-ray Space Telescope mission in the energy range from 50 MeV to 1 TeV, it is the deepest yet in this energy range. Relative to the 3FGL catalog, the 4FGL catalog has twice as much exposure as well as a number of analysis improvements, including an updated model for the Galactic diffuse gamma-ray emission, and two sets of light curves (one-year and two-month intervals). The 4FGL catalog includes 5064 sources above 4 sigma significance, for which we provide localization and spectral properties. Seventy-five sources are modeled explicitly as spatially extended, and overall, 358 sources are considered as identified based on angular extent, periodicity, or correlated variability observed at other wavelengths. For 1336 sources, we have not found plausible counterparts at other wavelengths. More than 3130 of the identified or associated sources are active galaxies of the blazar class, and 239 are pulsars.

  • 2. Abdollahi, S.
    et al.
    Acero, F.
    Baldini, L.
    Ballet, J.
    Bastieri, D.
    Bellazzini, R.
    Berenji, B.
    Berretta, A.
    Larsson, Stefan
    Dalarna University, School of Teacher Education, Natural Science.
    Zaharijas, G.
    Incremental Fermi Large Area Telescope Fourth Source Catalog2022In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 260, no 2, article id 53Article in journal (Refereed)
    Abstract [en]

    We present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi Large Area Telescope (LAT) catalog of 3-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. © 2022. The Author(s). Published by the American Astronomical Society.

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  • 3. Ajello, M
    et al.
    Atwood, W B
    Axelsson, M
    Bagagli, R
    Bagni, M
    Baldini, L
    Bastieri, D
    Bellardi, F
    Larsson, Stefan
    Dalarna University, School of Teacher Education, Natural Science.
    Zaharijas, G.
    Fermi Large Area Telescope Performance after 10 Years of Operation2021In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 256, no 1, article id 12Article in journal (Refereed)
    Abstract [en]

    The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from 30 MeV to more than 300 GeV. We describe the performance of the instrument at the 10 yr milestone. LAT performance remains well within the specifications defined during the planning phase, validating the design choices and supporting the compelling case to extend the duration of the Fermi mission. The details provided here will be useful when designing the next generation of high-energy gamma-ray observatories.

  • 4. Ajello, M.
    et al.
    Baldini, L.
    Bastieri, D.
    Bellazzini, R.
    Berretta, A.
    Bissaldi, E.
    Blandford, R. D.
    Bonino, R.
    Larsson, Stefan
    Dalarna University, School of Teacher Education, Natural Science. KTH Royal Institute of Technology, AlbaNova, Stockholm; The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, Stockholm.
    Zaharijas, G.
    First fermi-LAT solar flare catalog2021In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 252, no 2, article id abd32eArticle in journal (Refereed)
  • 5. Fermi-Lat Collaboration, T.
    et al.
    Baldini, L.
    Ballet, J.
    Bastieri, D.
    Becerra Gonzalez, J.
    Bellazzini, R.
    Berretta, A.
    Bissaldi, E.
    Larsson, Stefan
    Dalarna University, School of Teacher Education, Natural Science. KTH Royal Institute of Technology, Stockholm; The Oskar Klein Centre for Cosmoparticle Physics, Stockholm.
    Cavazzuti, E.
    Catalog of Long-term Transient Sources in the First 10 yr of Fermi-LAT Data2021In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 256, no 1, article id 13Article in journal (Refereed)
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