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  <title>Fermi LAT High-Energy Source Catalog (1FHL)</title>
  <shortName>FERMILHESC</shortName>
  <identifier>ivo://nasa.heasarc/fermilhesc</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Ackermann et al.</name>
    </creator>
    <contributor/>
    <date>2026-10-09</date>
    <contact>
      <name>NASA/GSFC HEASARC help desk</name>
      <email>heasarc-vo at athena.gsfc.nasa.gov</email>
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    <subject>Survey Source</subject>
    <description>
      This table contains the catalog of gamma-ray sources at energies above 10 GeV based on data from the Large Area Telescope (LAT) accumulated during the first 3 years of the Fermi Gamma-ray Space Telescope mission. The first Fermi-LAT catalog of &amp;gt; 10 GeV sources (1FHL) has 514 sources. For each source, the authors present location, spectrum, a measure of variability,and associations with cataloged sources at other wavelengths. They found that 449 (87%) could be associated with known sources, of which 393 (76% of the 1FHL sources) are active galactic nuclei. Of the 27 sources associated with known pulsars, they find 20 (12) to have significant pulsations in the range &amp;gt; 10 GeV (&amp;gt; 25 GeV). In this work, the authors also report that, at energies above 10 GeV, unresolved sources account for 27% +/- 8% of the isotropic gamma-ray background, while the unresolved Galactic population contributes only at the few percent level to the Galactic diffuse background. The authors also highlight the subset of the 1FHL sources that are the best candidates for detection at energies above 50 - 100 GeV with current and future ground-based gamma-ray observatories. The time interval analyzed here is from the beginning of Fermi LAT science operations on 2008 August 4 (MET 239557447) to 2011 August 1 (MET 333849586), covering very nearly 3 years. In this work, the authors analyze gamma rays with energies in the range 10-500 GeV. To limit the contamination from gamma rays produced by cosmic-ray interactions in the upper atmosphere, gamma rays with zenith angles greater than 105 degrees were excluded. To further reduce the residual gamma rays from the upper atmosphere only data for time periods when the spacecraft rocking angle was less than 52 degrees were considered. See Section 2 of the reference paper for further explanations. This table was created by the HEASARC in April 2015 based on &amp;lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/ApJS/209/34/"&amp;gt;CDS Catalog J/ApJS/209/34/&amp;lt;/a&amp;gt; files table3.dat and table7.dat. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2013ApJS..209...34A
    </source>
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        <description>
          Fermi LAT High-Energy Source Catalog (1FHL)
        </description>
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          <name>name</name>
          <description>
            The 1FHL Catalog Source Identifier (1FHL JHHMM.s+DDMM)
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            meta.id;meta.main
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            The 10-500 GeV Photon Flux
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            The 1-Sigma Uncertainty in the 10-500 GeV Photon Flux
          </description>
          <unit>photon/cm^2/s</unit>
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          <name>flux</name>
          <description>
            Energy Flux from 10-500 GeV from Power-Law Spectral Fit
          </description>
          <unit>erg/s/cm^2</unit>
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            phot.flux;em.gamma.hard
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          <description>
            The 1-Sigma Uncertainty in the Energy Flux
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          <unit>erg/s/cm^2</unit>
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        <column>
          <name>assoc_name_1</name>
          <description>
            Primary Name of Associated Source
          </description>
          <ucd>
            meta.id.assoc
          </ucd>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
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        <column>
          <name>source_type_1</name>
          <description>
            Primary Astrophysical Class of Associated Source
          </description>
          <ucd>
            src.class
          </ucd>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
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        <column>
          <name>"__x_ra_dec"</name>
          <description>
            System unit vector column
          </description>
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            System unit vector column
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            System unit vector column
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            System index column
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        <column>
          <name>lii</name>
          <description>
            Galactic Longitude
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          <unit>degree</unit>
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            Primary SED Classification
          </description>
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          <dataType xsi:type="vs:VOTableType">char</dataType>
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          <ucd>
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          <name>agn_optical_class_2</name>
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            Secondary AGN Optical Classification
          </description>
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            src.class
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          <flag>
            nullable
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            Second Distinct Redshift Found in Literature
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            Secondary SED Classification
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            Primary AGN Optical Classification
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            src.class
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          <flag>
            nullable
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            Position Angle of Major Axis of 95% Confidence Ellipse from North through East
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          <unit>degree</unit>
          <ucd>
            pos.posAng
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            Photon Power-Law Index, Gamma
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        <column>
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            Galactic Latitude
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          <unit>degree</unit>
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            pos.galactic.lat
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          <dataType xsi:type="vs:VOTableType">double</dataType>
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        <column>
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          <description>
            Browse Object Classification
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          <flag>
            nullable
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        <column>
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            Number of Change Points in Bayesian Blocks Light Curve (1 for Non-Variable)
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            Secondary Name of Associated Source
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            meta.id.assoc
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            Source Significance
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            Association with Other Catalogs of GeV Gamma-Ray Sources, If Any
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