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<ri:Resource created="2025-03-20T08:03:37Z" status="active" updated="2026-07-03T06:36:38Z" 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>HST Yellow supergiants in nearby galaxies</title><shortName>J/A+A/695/A226</shortName><identifier>ivo://CDS.VizieR/J/A+A/695/A226</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-nq/lccg</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tranin H.</name></creator><creator><name>Blagorodnova N.</name></creator><creator><name>Karambelkar V.</name></creator><creator><name>Groot P.J.</name></creator><creator><name>Bloemen S.,Vreeswijk P.M.</name></creator><creator><name>Pieterse D.L.A.</name></creator><creator><name>van Roestel J.</name></creator><date role="Updated">2026-07-03T06:36:38Z</date><date role="Created">2025-03-20T08:03:37Z</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>supergiant-stars</subject><subject>hst-photometry</subject><description>After the main sequence phase, stars more massive than 2.5M_{sun}_ rapidly evolve through the Hertzsprung gap as yellow giants and supergiants (YSG), before settling into the red giant branch. Identifying YSG in nearby galaxies is crucial for pinpointing progenitors of luminous red novae (LRNe) - astrophysical transients attributed to stellar mergers. In the era of extensive transient surveys like the Vera Rubin Observatory's LSST, this approach offers a new way to predict and select common envelope transients. This study investigates potential progenitors and precursors of LRNe by analysing Hubble Space Telescope (HST) photometry of stellar populations in galaxies within 20Mpc to identify YSG candidates. Additionally, we use ZTF and MeerLICHT/BlackGEM to identify possible precursors, preparing for future observations by the LSST. We compiled a sample of 369 galaxies with HST exposures in the F475W, F555W, F606W, and F814W filters. We identified YSG candidates using MESA stellar evolution tracks and statistical analysis of color-magnitude diagrams (CMDs). Our sample includes 154,494 YSG candidates with masses between 3 and 20M_{sun}_ and is affected by various contaminants, such as foreground stars and extinguished main-sequence stars. After excluding foreground stars using Gaia proper motions, contamination is estimated at 1% from foreground stars and 20% from extinction affecting main-sequence stars. Combining our YSG candidates with time-domain catalogs yielded several interesting candidates. Notably, we identified 12 LRN precursor candidates for which followup is encouraged. We highlight the importance of monitoring future transients that match YSG candidates to avoid missing potential LRNe and other rare transients. LSST will be a game changer in the search for LRN progenitors and precursors, discovering over 300000 new YSG and 100 precursors within 20Mpc.</description><source format="bibcode">2025A&amp;A...695A.226T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/695/A226</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/J/ApJ/703/441">J/ApJ/703/441 : Yellow supergiants in M31 (Drout+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/97">J/ApJ/750/97 : The yellow and red supergiants of M33 (Drout+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/50">J/ApJ/825/50 : Variable stars in M31 &amp; M33. III. 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F475W observed magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F555W</name><description>? F555W observed magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F606W</name><description>? F606W observed magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? F814W observed magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mstar</name><description>? 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Separation to nearest Chandra source</description><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gaiastar</name><description>Is a high proper-motion Gaia star</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>SType</name><description>Simbad main type</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Scontam</name><description>Is a contaminant according to Simbad type</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table><table><name>J/A+A/695/A226/table4</name><description>List of YSG hosts obtained in this study</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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