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<ri:Resource created="2014-08-01T12:59:43Z" 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>Wolf-Rayet and RSG stars in M101. I. HST photometry</title><shortName>J/AJ/146/162</shortName><identifier>ivo://CDS.VizieR/J/AJ/146/162</identifier><altIdentifier>doi:10.26093/cds/vizier.51460162</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shara M.M.</name></creator><creator><name>Bibby J.L.</name></creator><creator><name>Zurek D.</name></creator><creator><name>Crowther P.A.</name></creator><creator><name>Moffat A.F.J.</name></creator><creator><name>Drissen L.</name></creator><date role="Updated">2014-08-21T15:07:09Z</date><date role="Created">2014-08-01T12:59:43Z</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>galaxies</subject><subject>hst-photometry</subject><subject>supergiant-stars</subject><subject>wolf-rayet-stars</subject><description>Assembling a catalog of at least 10000 Wolf-Rayet (W-R) stars is an essential step in proving (or disproving) that these stars are the progenitors of Type Ib and Type Ic supernovae. To this end, we have used the Hubble Space Telescope (HST) to carry out a deep, HeII optical narrowband imaging survey of the ScI spiral galaxy M101. Almost the entire galaxy was imaged with the unprecedented depth and resolution that only the HST affords. Differenced with archival broadband images, the narrowband images allow us to detect much of the W-R star population of M101. We describe the extent of the survey and our images, as well as our data reduction procedures. A detailed broadband-narrowband imaging study of a field east of the center of M101, containing the giant star-forming region NGC5462, demonstrates our completeness limits, how we find W-R candidates, their properties and spatial distribution, and how we rule out most contaminants. We use the broadband images to locate luminous red supergiant (RSG) candidates. The spatial distributions of the W-R and RSG stars near NGC 5462 are strikingly different. W-R stars dominate the complex core, while RSGs dominate the complex halo. Future papers in this series will describe and catalog more than a thousand W-R and RSG candidates that are detectable in our images, as well as spectra of many of those candidates.</description><source format="bibcode">2013AJ....146..162S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/146/162</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/114">J/AJ/146/114 : Massive stars in M101. I. HST BVI photometry (Grammer+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/124">J/ApJ/733/124 : Cepheids in M101 observed with HST (Shappee+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/508/491">J/ApJ/508/491 : M101 Cepheids (Stetson+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/463/26">J/ApJ/463/26 : VI photometry of 29 Cepheids in M101. 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