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<ri:Resource created="2016-04-20T15:36:02Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>The second Fermi-LAT &gt;50GeV catalog (2FHL)</title><shortName>J/ApJS/222/5</shortName><identifier>ivo://CDS.VizieR/J/ApJS/222/5</identifier><altIdentifier>doi:10.26093/cds/vizier.22220005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ackermann M.</name></creator><creator><name>Ajello M.</name></creator><creator><name>Atwood W.B.</name></creator><creator><name>Baldini L.</name></creator><creator><name>Ballet J.,Barbiellini G.</name></creator><creator><name>Bastieri D.</name></creator><creator><name>Becerra Gonzalez J.</name></creator><creator><name>Bellazzini R.,Bissaldi E.</name></creator><creator><name>Blandford R.D.</name></creator><creator><name>Bloom E.D.</name></creator><creator><name>Bonino R.</name></creator><creator><name>Bottacini E.,Brandt T.J.</name></creator><creator><name>Bregeon J.</name></creator><creator><name>Bruel P.</name></creator><creator><name>Buehler R.</name></creator><creator><name>Buson S.</name></creator><creator><name>Caliandro G.A.,Cameron R.A.</name></creator><creator><name>Caputo R.</name></creator><creator><name>Caragiulo M.</name></creator><creator><name>Caraveo P.A.</name></creator><creator><name>Cavazzuti E.,Cecchi C.</name></creator><creator><name>Charles E.</name></creator><creator><name>Chekhtman A.</name></creator><creator><name>Cheung C.C.</name></creator><creator><name>Chiang J.</name></creator><creator><name>Chiaro G.,Ciprini S.</name></creator><creator><name>Cohen J.M.</name></creator><creator><name>Cohen-Tanugi J.</name></creator><creator><name>Cominsky L.R.</name></creator><creator><name>Conrad J.,Cuoco A.</name></creator><creator><name>Cutini S.</name></creator><creator><name>D'Ammando F.</name></creator><creator><name>de Angelis A.</name></creator><creator><name>de Palma F.</name></creator><creator><name>Desiante R.,Di Mauro M.</name></creator><creator><name>Di Venere L.</name></creator><creator><name>Dominguez A.</name></creator><creator><name>Drell P.S.</name></creator><creator><name>Favuzzi C.,Fegan S.J.</name></creator><creator><name>Ferrara E.C.</name></creator><creator><name>Focke W.B.</name></creator><creator><name>Fortin P.</name></creator><creator><name>Franckowiak A.,Fukazawa Y.</name></creator><creator><name>Funk S.</name></creator><creator><name>Furniss A.K.</name></creator><creator><name>Fusco P.</name></creator><creator><name>Gargano F.</name></creator><creator><name>Gasparrini D.,Giglietto N.</name></creator><creator><name>Giommi P.</name></creator><creator><name>Giordano F.</name></creator><creator><name>Giroletti M.</name></creator><creator><name>Glanzman T.,Godfrey G.</name></creator><creator><name>Grenier I.A.</name></creator><creator><name>Grondin M.-H.</name></creator><creator><name>Guillemot L.</name></creator><creator><name>Guiriec S.,Harding A.K.</name></creator><creator><name>Hays E.</name></creator><creator><name>Hewitt J.W.</name></creator><creator><name>Hill A.B.</name></creator><creator><name>Horan D.</name></creator><creator><name>Iafrate G.,Hartmann D.</name></creator><creator><name>Jogler T.</name></creator><creator><name>Johannesson G.</name></creator><creator><name>Johnson A.S.</name></creator><creator><name>Kamae T.</name></creator><creator><name>Kataoka J.,Knodlseder J.</name></creator><creator><name>Kuss M.</name></creator><creator><name>La Mura G.</name></creator><creator><name>Larsson S.</name></creator><creator><name>Latronico L.,Lemoine-Goumard M.</name></creator><creator><name>Li J.</name></creator><creator><name>Li L.</name></creator><creator><name>Longo F.</name></creator><creator><name>Loparco F.</name></creator><creator><name>Lott B.,Lovellette M.N.</name></creator><creator><name>Lubrano P.</name></creator><creator><name>Madejski G.M.</name></creator><creator><name>Maldera S.</name></creator><creator><name>Manfreda A.,Mayer M.</name></creator><creator><name>Mazziotta M.N.</name></creator><creator><name>Michelson P.F.</name></creator><creator><name>Mirabal N.</name></creator><creator><name>Mitthumsiri W.,Mizuno T.</name></creator><creator><name>Moiseev A.A.</name></creator><creator><name>Monzani M.E.</name></creator><creator><name>Morselli A.</name></creator><creator><name>Moskalenko I.V.,Murgia S.</name></creator><creator><name>Nuss E.</name></creator><creator><name>Ohsugi T.</name></creator><creator><name>Omodei N.</name></creator><creator><name>Orienti M.</name></creator><creator><name>Orlando E.,Ormes J.F.</name></creator><creator><name>Paneque D.</name></creator><creator><name>Perkins J.S.</name></creator><creator><name>Pesce-Rollins M.</name></creator><creator><name>Petrosian V.,Piron F.</name></creator><creator><name>Pivato G.</name></creator><creator><name>Porter T.A.</name></creator><creator><name>Raino S.</name></creator><creator><name>Rando R.</name></creator><creator><name>Razzano M.,Razzaque S.</name></creator><creator><name>Reimer A.</name></creator><creator><name>Reimer O.</name></creator><creator><name>Reposeur T.</name></creator><creator><name>Romani R.W.,Sanchez-Conde M.</name></creator><creator><name>Parkinson P.M.S.</name></creator><creator><name>Schmid J.</name></creator><creator><name>Schulz A.</name></creator><creator><name>Sgro C.,Siskind E.J.</name></creator><creator><name>Spada F.</name></creator><creator><name>Spandre G.</name></creator><creator><name>Spinelli P.</name></creator><creator><name>Suson D.J.</name></creator><creator><name>Tajima H.,Takahashi H.</name></creator><creator><name>Takahashi M.</name></creator><creator><name>Takahashi T.</name></creator><creator><name>Thayer J.B.</name></creator><creator><name>Thompson D.J.,Tibaldo L.</name></creator><creator><name>Torres D.F.</name></creator><creator><name>Tosti G.</name></creator><creator><name>Troja E.</name></creator><creator><name>Vianello G.</name></creator><creator><name>Wood K.S.,Wood M.</name></creator><creator><name>Yassine M.</name></creator><creator><name>Zaharijas G.</name></creator><creator><name>Zimmer S.</name></creator><date role="Updated">2017-09-06T06:23:36Z</date><date role="Created">2016-04-20T15:36:02Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>gamma-ray-astronomy</subject><subject>bl-lacertae-objects</subject><subject>redshifted</subject><description>We present a catalog of sources detected above 50GeV 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 50GeV-2TeV 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.</description><source format="bibcode">2016ApJS..222....5A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/222/5</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/274">VII/274 : The Roma BZCAT - 5th edition (Massaro+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/189">VII/189 : Catalog of Pulsars (Taylor+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A141">J/A+A/588/A141 : The MWA view of Fermi blazars (Giroletti+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/14">J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/23">J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A64">J/A+A/562/A64 : Fermi detection of BL Lac objects (Wu+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/34">J/ApJS/209/34 : The first Fermi-LAT &gt;10GeV catalog (1FHL) (Ackermann+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/17">J/ApJS/208/17 : 2nd Fermi LAT cat. of gamma-ray pulsars (2PC) (Abdo+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/16">J/ApJS/207/16 : BL Lac candidates for TeV observations (Massaro+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/135">J/ApJ/764/135 : Spectroscopic redshifts of BL Lac objects (Shaw+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/31">J/ApJS/199/31 : Fermi LAT second source catalog (2FGL) (Nolan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/49">J/ApJ/748/49 : Optical spectroscopy of 1LAC broad-line blazars (Shaw+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/597">J/ApJ/700/597 : FERMI LAT detected blazars (Abdo+, 2009)</relatedResource><relatedResource>http://fermi.gsfc.nasa.gov/ssc/ : Fermi Science Support Center home page</relatedResource><relatedResource>http://tevcat.uchicago.edu/ : TeVCat home page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2FHL</name><description>2FHL name (JHHMM.m+DDMMe) (Source_Name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>pE</name><description>Previously detected extended source (link to table 4)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Right ascension; J2000 (RAJ2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination; J2000 (DEJ2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>GLON</name><description>Galactic longitude (GLON)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude (GLAT)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pos</name><description>[0/0.2] Position uncertainty at 68% confidence level (Pos_err_68)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TS</name><description>[25/5601] Test statistic (TS)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gam</name><description>[0.9/15] Observed spectral index (Spectral_Index) (1)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gam</name><description>? 1{sigma} uncertainty on the observed spectral index (Unc_Spectral_Index)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SpD11</name><description>? Intrinsic spectral index computed using the Dominguez et al. (2011MNRAS.410.2556D) EBL model (Intr_Spectrl_Index_D11) (1)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_SpD11</name><description>? 1{sigma} uncertainty on SpD11 (Unc_Intr_Spectral_Index_D11)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SpG12</name><description>? Intrinsic spectral index computed using the Gilmore et al. (2012MNRAS.422.3189G) (1) EBL model (Intr_Spectra_Index_G12)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_SpG12</name><description>? 1{sigma} uncertainty on SpG12 (Unc_Intr_Spectral_Index_G12)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F50</name><description>Integral photon flux from 50GeV to 2TeV (Flux50)</description><unit>ph.cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F50</name><description>1{sigma} uncertainty on F50 (Unc_Flux50)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>S50</name><description>Energy flux from 50GeV to 2TeV in erg/cm^2^/s (Energy_Flux50)</description><unit>mW.m**-2</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_S50</name><description>1{sigma} uncertainty on S50 (Unc_Energy_Flux50)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F171</name><description>Integral photon flux from 50 to 171GeV (Flux50_171GeV)</description><unit>ph.cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F171</name><description>[-0.1/]? 1{sigma} negative uncertainty on F171 (Unc_Flux50_171GeV)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_F171</name><description>? 1{sigma} positive uncertainty on F171 (Positive_Unc_Flux50_171GeV) (2)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TS171</name><description>Square root of the Test Statistic between 50 and 171GeV (Sqrt_TS50_171GeV)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F585</name><description>Integral photon flux from 171 to 585GeV (Flux171_585GeV)</description><unit>ph.cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F585</name><description>[-0.1/]? 1{sigma} negative uncertainty on F585 (Unc_Flux171_585GeV)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_F585</name><description>? 1{sigma} positive uncertainty on F585 (Positive_Unc_Flux171_585GeV) (2)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TS585</name><description>Square root of the Test Statistic between 171 and 585GeV (Sqrt_TS171_585GeV)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F2000</name><description>Integral photon flux from 585GeV to 2TeV (Flux585_2000GeV)</description><unit>ph.cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F2000</name><description>[-0.1/]? 1{sigma} negative uncertainty on F2000 (Unc_Flux585_2000GeV)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_F2000</name><description>? 1{sigma} positive uncertainty on F2000 (Positive_Unc_Flux585_2000GeV) (2)</description><unit>ph.cm**-2.s**-1</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TS2000</name><description>Square root of the Test Statistic between 585GeV and 2TeV (Sqrt_TS585_2000GeV)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Npred</name><description>[3/378] Predicted number of photons from the source (Npred)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EHEP</name><description>[52/1997]? Highest photon energy (HEP_Energy) (3)</description><unit>GeV</unit><ucd>em.energy;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PHEP</name><description>[0.85/1]? Probability that the HEP is coming from the source, &gt;=0.85 (HEP_Prob) (3)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ROI</name><description>[1/143] Region of interest number (ROI)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Assoc</name><description>Name of the most likely associated source (ASSOC)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>PBAY</name><description>[0.8/1]? Probability of association from the Bayesian method (ASSOC_PROB_BAY)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PLR</name><description>[0.7/1]? Probability of association from the likelihood ratio method (ASSOC_PROB_LR)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Class</name><description>Class designation for the most likely association (CLASS) (4)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>z</name><description>[0/2.1]? Redshift (when available) of the most likely associated source (Redshift) (5)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NuPk</name><description>? Observed Synchrotron peak frequency (NuPeak_obs)</description><unit>Hz</unit><ucd>em.freq;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>3FGL</name><description>Name of the most likely associated source in the 3FGL (_3FGL_Name)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>1FHL</name><description>Name of the most likely associated source in the 1FHL (_1FHL_Name)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>TeVCat</name><description>Name of the most likely associated source in the TeVCat (TeVCat_Name)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJS/222/5/table5</name><description>New 2FHL extended sources</description><column><name>e_Gamma</name><description>[0.1/0.3] 1{sigma} uncertainty on Gamma</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2FHL</name><description>2FHL name (JHHMM.m+DDMMe) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>TS</name><description>[75.6/109.3] Test Statistic</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TSex</name><description>[29.9/83.4] Extended Test Statistic TS_ext_</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TS2p</name><description>[12.9/26.2] Second point source TS (TS_2pts_)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F50</name><description>[7.2/17.6] Integral photon flux from 50GeV to 2TeV</description><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F50</name><description>[1.7/2.8] 1{sigma} uncertainty on F50</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gamma</name><description>[1.5/2.2] Observed spectral index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Assoc</name><description>Name of the most likely associated source</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Class</name><description>Class designation for the most likely association</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Rad</name><description>[0.2/1.3] Radius</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJS/222/5/rois</name><description>Region of interests (ROIs) list</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ROI</name><description>[1/154] Running sequence number of the Region of Interest (ROI)</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[5/25] Radius</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJS/222/5/table4</name><description>2FHL extended sources previously detected by the Fermi-LAT</description><column><name>Mod</name><description>Spatial model</description><ucd>stat.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2FHL</name><description>2FHL name (JHHMM.m+DDMMe) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>GLON</name><description>[6.5/347.4] Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>[-32.9/3.1] Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>TS</name><description>[28/438] Test Statistic</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Assoc</name><description>Name of the most likely associated source</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Class</name><description>Class designation for the most likely association</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Ext</name><description>Extension(s) (2)</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table></schema></tableset></ri:Resource>