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<ri:Resource created="2018-10-30T07:32:51Z" 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>9Y-MST Catalogue</title><shortName>J/A+A/619/A23</shortName><identifier>ivo://CDS.VizieR/J/A+A/619/A23</identifier><altIdentifier>doi:10.26093/cds/vizier.36190023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Campana R.</name></creator><creator><name>Massaro E.</name></creator><creator><name>Bernieri E.</name></creator><date role="Updated">2020-09-01T13:32:45Z</date><date role="Created">2018-10-30T07:32:51Z</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>active-galactic-nuclei</subject><subject>gamma-ray-astronomy</subject><subject>bl-lacertae-objects</subject><description>We describe a catalogue of gamma-ray source candidates selected using the minimum spanning tree (MST) algorithm on the nine year Fermi-LAT sky (Pass 8) at energies higher than 10GeV. The extragalactic sky at absolute Galactic latitudes above 20{deg} has been investigated using rather restrictive selection criteria, resulting in a total sample of 1342 sources. Of these, 249 are new detections that have not been previously associated with gamma-ray catalogues. A large portion of these candidates have interesting counterparts, which are most likely blazars. In this paper, we report the main results of the catalogue selection and search of counterparts.</description><source format="bibcode">2018A&amp;A...619A..23C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/619/A23</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/J/ApJS/171/61">J/ApJS/171/61 : CRATES catalog (Healey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/405">J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010)</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/ApJS/215/14">J/ApJS/215/14 : WIBRaLS catalog (D'Abrusco+, 2014)</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/ApJS/232/18">J/ApJS/232/18 : The third Fermi-LAT &gt;10GeV catalog (3FHL) (Ajello+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/598/A17">J/A+A/598/A17 : The 2WHSP catalog (Chang+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/598/A134">J/A+A/598/A134 : {gamma}-ray signature in WHSP blazars (Arsioli+, 2017)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/619/A23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/619/A23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/619/A23</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/619/A23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/619/A23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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J/ApJS/232/18)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>3FGL</name><description>Counterpart in the 3FGL catalogue 3FGL JHHMM.m+DDMM (Acero et al., 2015, Cat. J/ApJS/218/23)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>2FGL</name><description>Counterpart in the 2FGL catalogue 2FGL JHHMM.m+DDMM (Nolan et al., 2012, Cat. J/ApJS/199/31)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>1FGL</name><description>Counterpart in the 1FGL catalogue 1FGL JHHMM.m+DDMM (Abdo et al., 2010, Cat. 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