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<ri:Resource created="2019-02-12T13:56:32Z" 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 HectoMAP cluster survey. II. X-ray clusters</title><shortName>J/ApJ/855/100</shortName><identifier>ivo://CDS.VizieR/J/ApJ/855/100</identifier><altIdentifier>doi:10.26093/cds/vizier.18550100</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sohn J.</name></creator><creator><name>Chon G.</name></creator><creator><name>Bohringer H.</name></creator><creator><name>Geller M.J.</name></creator><creator><name>Diaferio A.</name></creator><creator><name>Hwang H.S.,Utsumi Y.</name></creator><creator><name>Rines K.J.</name></creator><date role="Updated">2020-06-15T07:38:06Z</date><date role="Created">2019-02-12T13:56:32Z</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>galaxy-clusters</subject><subject>x-ray-sources</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>surveys</subject><description>We apply a friends-of-friends algorithm to the HectoMAP redshift survey and cross-identify associated X-ray emission in the ROSAT All-Sky Survey data (RASS). The resulting flux-limited catalog of X-ray cluster surveys is complete to a limiting flux of ~3x10^-13^erg/s/cm^2^ and includes 15 clusters (7 newly discovered) with redshifts z&lt;=0.4. HectoMAP is a dense survey (~1200 galaxies deg^-2^) that provides ~50 members (median) in each X-ray cluster. We provide redshifts for the 1036 cluster members. Subaru/Hyper Suprime-Cam imaging covers three of the X-ray systems and confirms that they are impressive clusters. The HectoMAP X-ray clusters have an LX-{sigma}cl scaling relation similar to that of known massive X-ray clusters. The HectoMAP X-ray cluster sample predicts ~12000+/-3000 detectable X-ray clusters in RASS to the limiting flux, comparable with previous estimates.</description><source format="bibcode">2018ApJ...855..100S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/855/100</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/IX/10">IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/4">VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/86">VII/86 : Groups of Galaxies. 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