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<ri:Resource created="2002-03-08T21:59:19Z" 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>The ROSAT brightest cluster sample - I.</title><shortName>J/MNRAS/301/881</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/301/881</identifier><altIdentifier>doi:10.26093/cds/vizier.73010881</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ebeling H.</name></creator><creator><name>Edge A.C.</name></creator><creator><name>Boehringer H.</name></creator><creator><name>Allen S.W.</name></creator><creator><name>Crawford C.S.,Fabian A.C.</name></creator><creator><name>Voges W.</name></creator><creator><name>Huchra J.P.</name></creator><date role="Updated">2024-06-25T20:18:19Z</date><date role="Created">2002-03-08T21:59:19Z</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>galaxy-clusters</subject><subject>x-ray-sources</subject><subject>surveys</subject><description>We present a 90 per cent flux-complete sample of the 201 X-ray-brightest clusters of galaxies in the northern hemisphere ({delta}&gt;=0{deg}), at high Galactic latitudes (|b|&gt;= 20{deg}), with measured redshifts z&lt;=0.3 and fluxes higher than 4.4x10^-12^erg/cm^2^/s in the 0.112.4 keV band. The sample, called the ROSAT Brightest Cluster Sample (BCS), is selected from ROSAT All-Sky Survey data and is the largest X-ray-selected cluster sample compiled to date. In addition to Abell clusters, which form the bulk of the sample, the BCS also contains the X-ray-brightest Zwicky clusters and other clusters selected from their X-ray properties alone. Effort has been made to ensure the highest possible completeness of the sample and the smallest possible contamination by non-cluster X-ray sources. X-ray fluxes are computed using an algorithm tailored for the detection and characterization of X-ray emission from galaxy clusters. These fluxes are accurate to better than 15 per cent (mean 1{sigma} error).</description><source format="bibcode">1998MNRAS.301..881E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/301/881</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/J/ApJ/502/558">J/ApJ/502/558 : Catalog of ROSAT galaxy clusters (Vikhlinin+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/514/148">J/ApJ/514/148 : ROSAT survey of bright galaxies clusters (De Grandi+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/306/857">J/MNRAS/306/857 : ROSAT Brightest Cluster Sample. III. (Crawford+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/318/333">J/MNRAS/318/333 : Extended ROSAT Bright Cluster Sample (Ebeling+ 2000)</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/MNRAS/301/881</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/301/881</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/301/881</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/301/881</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/301/881</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/301/881</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/301/881/table3 (The ROSAT Brightest Cluster Sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/301/881/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/301/881/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/301/881/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>0.044</ra><dec>8.277</dec><sr>0.005555555555555556</sr></testQuery></capability><facility>ROSAT</facility><coverage><spatial>6/3 6 50 87 206-207 306 361 929 986 1006 2173 2186 2227 2251 2432 4206 4317 4394 4672 4867 4976 5030 5099-5100 5305 5327 5346 5524 5536 5585 5618 5701 5881 5931 6019 6039 6088 6223 6337 6522 6609 6611 6639 6655 7004 7011 7026 7187 7242 7513 7516 7756 7768 7814 8220 8223 8258 8264 8268 8271 8422 8442 8507 8520 8524 8526 8575 8589 8648 8788 8823 8919 8963 8969 9036 9047 9050 9052 9072 9144 9168 9287 9333 9354 9366 9468 9476 9506 9508 9583 9764 9776 9997 10180 10182 10271 10311-10312 10318 10379 10416 10442 10526-10527 10664 10691 10717 11042 11080 11287 11591 11626 11809 11846 12121 12253 12642 12653 15085 16030 16294 17840 18009 18035 18168 18184 18324 18411 18939 19097 19130 19204 19314 19432 19451 19501 19516 19542 19608 19656 19912 19930 19935 19941 19993 20021 20029 20072 20083 20095 20300 20302 20308 20335 20355 20361 20371 21977 22972 23023 23306 23324 23349 23384 23451 25981 26037 26042 26197 26302 26432 27428 27595 27652 27660 27676 27740 27742 27760 27765 27966 28005 28174 28220 28249 28265 28271 28360 28414 28430 28471 28622 28663 31398 31509 31537 32362 32500 32503 32693 32739 32746</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/301/881?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/301/881/table3</name><description>The ROSAT Brightest Cluster Sample</description><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>n_Name</name><description>Note on Name (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Name</name><description>Cluster name (2)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RA</name><description>Right ascension (B1950)</description><ucd>pos.eq.ra</ucd></column><column><name>DE</name><description>Declination (B1950)</description><ucd>pos.eq.dec</ucd></column><column><name>RAJ2000</name><description>X-ray right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>X-ray declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>NH</name><description>Hydrogen column density from Stark et al. (1992, Cat. &lt;J/ApJS/79/77&gt;)</description><unit>1e+20cm**-2</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Texp</name><description>RASS exposition time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CR(VTP)</name><description>PSPC count rate in PHA (Pulse Height Analyser) channels 11 to 235 originally detected by VTP (Voronoi tesselation and percolation)</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R(VTP)</name><description>Equivalent radius of the source detected by VTP (Voronoi tesselation and percolation)</description><unit>arcmin</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CR</name><description>Final PSCP count rate (3)</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CR</name><description>rms uncertainty on CR (4)</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>kT</name><description>Intra-cluster medium gas temperature used in conversion from count rates to energy fluxes</description><unit>keV</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_kT</name><description>[e] e: temperature estimated</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FX</name><description>Unabsorbed X-ray energy flux in the 0.1-2.4keV band (10-12erg/cm2/s)</description><unit>1e-15W.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LX</name><description>Intrinsic X-ray luminosity in 0.1-2.4keV band</description><unit>1e+37W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_z</name><description>Redshift reference in refs.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/MNRAS/301/881/refs</name><description>References</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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