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<ri:Resource created="2019-12-03T09:06:19Z" 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>3HSP blazars catalog</title><shortName>J/A+A/632/A77</shortName><identifier>ivo://CDS.VizieR/J/A+A/632/A77</identifier><altIdentifier>doi:10.26093/cds/vizier.36320077</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chang Y.-L.</name></creator><creator><name>Arsioli B.</name></creator><creator><name>Giommi P.</name></creator><creator><name>Padovani P.</name></creator><creator><name>Brandt C.</name></creator><date role="Updated">2021-04-06T14:20:48Z</date><date role="Created">2019-12-03T09:06:19Z</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>bl-lacertae-objects</subject><subject>gamma-ray-astronomy</subject><description>High-synchrotron peaked blazars (HSPs or HBLs) play a central role in very high-energy (VHE) {gamma}-ray astronomy, and likely in neutrino astronomy. Currently, the largest compilation of HSP blazars, the 2WHSP sample, includes 1691 sources, but it is not complete in the radio or in the X-ray band. In order to provide a larger and more accurate set of HSP blazars that is useful for future statistical studies and to plan for VHE/TeV observations, we present the 3HSP catalogue, the largest sample of extreme and high-synchrotron peaked (EHSP; HSP) blazars and blazar candidates. We implemented several ways to improve the size and the completeness of the 2WHSP catalogue and reduced the selection biases to be taken into consideration in population studies. By discarding the IR constraint and relaxing the radio-IR and IR-X-ray slope criteria, we were able to select more sources with peak close to the 10^15^Hz threshold and objects where the host galaxy dominates the flux. The selection of extra sources now commences with a crossmatching between radio and X-ray surveys, applying a simple flux ratio cut. We also considered Fermi-LAT catalogues to find reasonable HSP-candidates that are detected in the {gamma}-ray band but are not included in X-ray or radio source catalogues. The new method, and the use of newly available multi-frequency data, allowed us to add 395 sources to the sample, to remove 73 2WHSP sources that were previously agged as uncertain and could not be confirmed as genuine HSP blazars, and to update parameters obtained by fitting the synchrotron component. The 3HSP catalogue includes 2013 sources, 88% of which with a redshift estimation, a much higher percentage than in any other list of HSP blazars. All new {gamma}-ray detections are described in the First and Second Brazil ICRANet {gamma}-ray blazar catalogues (1BIGB &amp; 2BIGB) also taking into account the 4FGL list of {gamma}-ray sources published by the Fermi Large Area Telescope (Fermi-LAT) team. Moreover, the cross-matching between the 2WHSP, 2FHL HSP, and IceCube neutrino positions suggests that HSPs are likely counterparts of neutrino events, which implies the 3HSP catalogue is also useful in that respect. The 3HSP catalogue shows improved completeness compared to its predecessors, the 1WHSP and 2WHSP catalogues, and follows the track of their increasing relevance for VHE astronomy.</description><source format="bibcode">2019A&amp;A...632A..77C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/632/A77</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/218/23">J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)</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/A+A/598/A17">J/A+A/598/A17 : The 2WHSP catalog (Chang+, 2017)</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/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/632/A77</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/632/A77</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, 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Redshift flag (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Gamma</name><description>Fermi gamma-ray counterpart</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>FOM</name><description>Figure of Merit (G2)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WHSP</name><description>2WHSP counterpart (2WHSPJHHMMSS.s+DDMMSS)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">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/A+A/632/A77/table2</name><description>The extreme sources</description><column><name>z</name><description>? Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_z</name><description>[1/5]? Redshift flag (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FOM</name><description>Figure of Merit (G2)</description><ucd>meta.bib.fig</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>Name</name><description>Designation (3HSPJHHMMSS.s+DDMMSS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>l_lognu</name><description>Limit flag on lognu</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>lognu</name><description>Log Synchrotron peak frequency</description><unit>log(Hz)</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>u_lognu</name><description>[?] Uncertainty flag on lognu</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>BZCat</name><description>[5BZ BGU] BZCat counterpart</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>WHSP</name><description>[yes ] 2WHSP counterpart</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Gamma</name><description>Fermi gamma-ray counterpart (2)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>TeV</name><description>TeV counterpart</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column></table><table><name>J/A+A/632/A77/table3</name><description>Fermi association</description><column><name>3FHL</name><description>Fermi 3FHL counterpart (JHHMM.m+DDMM)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">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>Name</name><description>Designation (3HSPJHHMMSS.s+DDMMSS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>4FGL</name><description>Fermi 4FGL counterpart (JHHMM.m+DDMM)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>n_4FGL</name><description>[*] Note on 4FGL (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Kaur2019</name><description>[yes no] Counterpart in Kaur et al. (2019ApJ...871...94K)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table><table><name>J/A+A/632/A77/table4</name><description>Sources without radio counterparts</description><column><name>z</name><description>? Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>Name</name><description>Designation (3HSP JHHMMSS.s+DDMMSS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>lognu</name><description>Log Synchrotron peak frequency</description><unit>log(Hz)</unit><ucd>em.freq;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_z</name><description>[0/5]? Redshift flag (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Gamma</name><description>4FGL name (4FGL JHHMM.m+DDMM)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>FOM</name><description>Figure of merit (G2)</description><ucd>meta.bib.fig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>