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<ri:Resource created="2021-09-16T16:20:43Z" status="active" updated="2025-06-13T15:25:00Z" 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>Identifying 3FHL. V. CTIO-COSMOS spectra</title><shortName>J/ApJS/254/26</shortName><identifier>ivo://CDS.VizieR/J/ApJS/254/26</identifier><altIdentifier>doi:10.26093/cds/vizier.22540026</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rajagopal M.</name></creator><creator><name>Marchesi S.</name></creator><creator><name>Kaur A.</name></creator><creator><name>Dominguez A.</name></creator><creator><name>Silver R.</name></creator><creator><name>Ajello M.</name></creator><date role="Updated">2022-01-19T12:35:09Z</date><date role="Created">2021-09-16T16:20:43Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>gamma-ray-astronomy</subject><subject>astronomical-object-identification</subject><description>As a follow-up to the optical spectroscopic campaign aimed at achieving completeness in the Third Catalog of Hard Fermi-LAT Sources (3FHL), we present here the results of a sample of 28 blazars of an uncertain type observed using the 4m telescope at Cerro Tololo Inter-American Observatory in Chile. Out of these 28 sources, we find that 25 are BL Lacertae objects (BL Lacs) and 3 are flat-spectrum radio quasars (FSRQs). We measure redshifts or lower limits for 16 of these blazars, and it is observed that the 12 remaining blazars have featureless optical spectra. These results are part of a more extended optical spectroscopy follow-up campaign for 3FHL blazars, where, until now, 51 blazars of an uncertain type have been classified into BL Lac and FSRQ categories. Furthermore, this campaign has resulted in redshift measurements and lower limits for 15 of these sources. Our results contribute toward attaining a complete sample of blazars above 10 GeV, which then will be crucial in extending our knowledge on blazar emission mechanisms and the extragalactic background light.</description><source format="bibcode">2021ApJS..254...26R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/254/26</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/259">VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/495/691">J/A+A/495/691 : Multifrequency catalog of blazars, Roma-BZCAT (Massaro+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/538/A26">J/A+A/538/A26 : BL Lac objects beyond z=1.3 (Rau+, 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/764/135">J/ApJ/764/135 : Spectroscopic redshifts of BL Lac objects (Shaw+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/73">J/ApJ/780/73 : Redshifts of BL Lac objects from Fermi (Ajello+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/579/A34">J/A+A/579/A34 : 1WHSP: VHE {gamma}-ray blazar candidates (Arsioli+, 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/ApJS/233/3">J/ApJS/233/3 : VLBA Extragalactic Proper Motion Catalog (Truebenbach+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/33">J/ApJS/247/33 : The Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/643/A103">J/A+A/643/A103 : Fermi-LAT sources low-energy counterparts (Pena-Herazo+, 2020)</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/ApJS/254/26</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/254/26</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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36910 36973 37523 38316 41155 41325 41966 41970 42571 42920 43085 43443 43996 44290 44902 45632 45820 46564 47497 48090 48778 48933</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/254/26?format=ascii</footprint><waveband>Gamma-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/254/26/table1</name><description>List of sources and their properties sorted in the order of increasing R.A. values</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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