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<ri:Resource created="2022-08-04T11:55:14Z" 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>3rd HAWC cat. of VHE gamma-ray sources (3HWC)</title><shortName>J/ApJ/905/76</shortName><identifier>ivo://CDS.VizieR/J/ApJ/905/76</identifier><altIdentifier>doi:10.26093/cds/vizier.19050076</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Albert A.</name></creator><creator><name>Alfaro R.</name></creator><creator><name>Alvarez C.</name></creator><creator><name>Angeles Camacho J.R.,Arteaga-Velazquez J.C.</name></creator><creator><name>Arunbabu K.P.</name></creator><creator><name>Avila Rojas D.</name></creator><creator><name>Ayala Solares H.A.,Baghmanyan V.</name></creator><creator><name>Belmont-Moreno E.</name></creator><creator><name>BenZvi S.Y.</name></creator><creator><name>Brisbois C.,Caballero-Mora K.S.</name></creator><creator><name>Capistran T.</name></creator><creator><name>Carraminana A.</name></creator><creator><name>Casanova S.</name></creator><creator><name>Cotti U.,Coutino de Leon S.</name></creator><creator><name>De la Fuente E.</name></creator><creator><name>Diaz Hernandez R.</name></creator><creator><name>Diaz-Cruz L.,Dingus B.L.</name></creator><creator><name>DuVernois M.A.</name></creator><creator><name>Durocher M.</name></creator><creator><name>Diaz-Velez J.C.,Ellsworth R.W.</name></creator><creator><name>Engel K.</name></creator><creator><name>Espinoza C.</name></creator><creator><name>Fan K.L.</name></creator><creator><name>Fang K.,Fernandez Alonso M.</name></creator><creator><name>Fleischhack H.</name></creator><creator><name>Fraija N.</name></creator><creator><name>Galvan-Gamez A.</name></creator><creator><name>Garcia D.,Garcia-Gonzalez J.A.</name></creator><creator><name>Garfias F.</name></creator><creator><name>Giacinti G.</name></creator><creator><name>Gonzalez M.M.</name></creator><creator><name>Goodman J.A.,Harding J.P.</name></creator><creator><name>Hernandez S.</name></creator><creator><name>Hinton J.</name></creator><creator><name>Hona B.</name></creator><creator><name>Huang D.,Hueyotl-Zahuantitla F.</name></creator><creator><name>Huntemeyer P.</name></creator><creator><name>Iriarte A.</name></creator><creator><name>Jardin-Blicq A.,Joshi V.</name></creator><creator><name>Kieda D.</name></creator><creator><name>Lara A.</name></creator><creator><name>Lee W.H.</name></creator><creator><name>Leon Vargas H.</name></creator><creator><name>Linnemann J.T.,Longinotti A.L.</name></creator><creator><name>Luis-Raya G.</name></creator><creator><name>Lundeen J.</name></creator><creator><name>Lopez-Coto R.</name></creator><creator><name>Malone K.,Marandon V.</name></creator><creator><name>Martinez O.</name></creator><creator><name>Martinez-Castellanos I.</name></creator><creator><name>Martinez-Castro J.,Matthews J.A.</name></creator><creator><name>Miranda-Romagnoli P.</name></creator><creator><name>Morales-Soto J.A.</name></creator><creator><name>Moreno E.,Mostafa M.</name></creator><creator><name>Nayerhoda A.</name></creator><creator><name>Nellen L.</name></creator><creator><name>Newbold M.</name></creator><creator><name>Nisa M.U.,Noriega-Papaqui R.</name></creator><creator><name>Olivera-Nieto L.</name></creator><creator><name>Omodei N.</name></creator><creator><name>Peisker A.,Perez Araujo Y.</name></creator><creator><name>Perez-Perez E.G.</name></creator><creator><name>Ren Z.</name></creator><creator><name>Rho C.D.</name></creator><creator><name>Riviere C.,Rosa-Gonzalez D.</name></creator><creator><name>Ruiz-Velasco E.</name></creator><creator><name>Salazar H.</name></creator><creator><name>Salesa Greus F.S.,Sandoval A.</name></creator><creator><name>Schneider M.</name></creator><creator><name>Schoorlemmer H.</name></creator><creator><name>Serna F.</name></creator><creator><name>Sinnis G.</name></creator><creator><name>Smith A.J.,Springer R.W.</name></creator><creator><name>Surajbali P.</name></creator><creator><name>Tollefson K.</name></creator><creator><name>Torres I.</name></creator><creator><name>Torres-Escobedo R.,Ukwatta T.N.</name></creator><creator><name>Urena-Mena F.</name></creator><creator><name>Weisgarber T.</name></creator><creator><name>Werner F.</name></creator><creator><name>Willox E.</name></creator><creator><name>Zepeda A.,Zhou H.</name></creator><creator><name>de Leon C.</name></creator><creator><name>Alvarez J.D.</name></creator><creator><name>The HAWC Collaboration</name></creator><date role="Updated">2023-06-08T11:53:56Z</date><date role="Created">2022-08-04T11:55:14Z</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><description>We present a new catalog of TeV gamma-ray sources using 1523 days of data from the High-Altitude Water Cherenkov (HAWC) Observatory. The catalog represents the most sensitive survey of the northern gamma-ray sky at energies above several TeV, with three times the exposure compared to the previous HAWC catalog, 2HWC. We report 65 sources detected at &gt;=5{sigma} significance, along with the positions and spectral fits for each source. The catalog contains eight sources that have no counterpart in the 2HWC catalog, but are within 1{deg} of previously detected TeV emitters, and 20 sources that are more than 1{deg} away from any previously detected TeV source. Of these 20 new sources, 14 have a potential counterpart in the fourth Fermi Large Area Telescope catalog of gamma-ray sources. We also explore potential associations of 3HWC sources with pulsars in the Australia Telescope National Facility (ATNF) pulsar catalog and supernova remnants in the Galactic supernova remnant catalog.</description><source format="bibcode">2020ApJ...905...76A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/905/76</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/B/psr">B/psr : ATNF Pulsar Catalogue (Manchester+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/67">IX/67 : Incremental Fermi LAT 4th source cat. (4FGL-DR3) (Fermi-LAT col., 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/843/40">J/ApJ/843/40 : The 2HWC HAWC Observatory gamma-ray cat. 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Separation distance from nearest SNR</description><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Type</name><description>SNR Type from the SNRCat, Ferrand &amp; Safi-Harb (2012AdSpR..49.1313F)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column></table><table><name>J/ApJ/905/76/table4</name><description>HAWC sources with the corresponding TeV halo candidate pulsars within 1deg</description><column><name>3HWC</name><description>HAWC Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</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>GLON</name><description>[22.13/200.91] Galactic Longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>[-4.13/20.34] Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>ATNF</name><description>ATNF pulsar, Manchester+ (2005, B/psr)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Age</name><description>[111/342] Age</description><unit>kyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Edot</name><description>[3.25e+34/2.87e+36] Spin-down luminosity, erg/s</description><unit>1e-07W</unit><ucd>phys.luminosity;em.gamma</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dist</name><description>[0.19/5.06] Distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep</name><description>[0.11/0.95] Separation</description><unit>deg</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TeVCat</name><description>Previously detected TeV counterpart of each source</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column></table></schema></tableset></ri:Resource>