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<ri:Resource created="2014-05-28T14:40:22Z" 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>XMM observations of {alpha} Per</title><shortName>J/AJ/145/143</shortName><identifier>ivo://CDS.VizieR/J/AJ/145/143</identifier><altIdentifier>doi:10.26093/cds/vizier.51450143</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pillitteri I.</name></creator><creator><name>Evans N.R.</name></creator><creator><name>Wolk S.J.</name></creator><creator><name>Bruck Syal M.</name></creator><date role="Updated">2018-01-11T06:56:50Z</date><date role="Created">2014-05-28T14:40:22Z</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>open-star-clusters</subject><subject>x-ray-sources</subject><subject>infrared-photometry</subject><description>We report on the analysis of an archival observation of part of the {alpha} Persei cluster obtained with XMM-Newton. We detected 102 X-ray sources in the band 0.3-8.0 keV, of which 39 of them are associated with the cluster as evidenced by appropriate magnitudes and colors from Two Micron All Sky Survey photometry. We extend the X-ray luminosity distribution (XLD) for M dwarfs, to add to the XLD found for hotter dwarfs from spatially extensive surveys of the whole cluster by ROSAT. Some of the hotter stars are identified as a background, possible slightly older group of stars at a distance of approximately 500 pc.</description><source format="bibcode">2013AJ....145..143P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/145/143</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/xmm">B/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/80">V/80 : Low-Mass Stars' Membership in Alpha Persei Cluster (Prosser 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/3403">J/MNRAS/426/3403 : UKIDSS-GCS {alpha} Per members (Lodieu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/367/781">J/MNRAS/367/781 : XMM observations of NGC 2547 (Jeffries+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/125">J/A+A/416/125 : RI photometry in alpha Per and Pleiades (Deacon+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/421/175">J/A+A/421/175 : XMM sources in Blanco 1 (Pillitteri+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/319/215">J/AN/319/215 : Alpha Per cluster low-mass members. 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