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<ri:Resource created="2026-05-22T10:02:47Z" status="active" updated="2026-07-03T00:00:00Z" 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>CARMENES M dwarfs projected rotational velocities</title><shortName>J/A+A/709/A244</shortName><identifier>ivo://CDS.VizieR/J/A+A/709/A244</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Varas R.</name></creator><creator><name>Morello G.</name></creator><creator><name>Zechmeister M.</name></creator><creator><name>Amado P.J.</name></creator><creator><name>Pozuelos F.J.,Caballero J.A.</name></creator><creator><name>Claret A.</name></creator><creator><name>Cifuentes C.</name></creator><creator><name>Morales R.</name></creator><creator><name>Quirrenbach A.,Reiners A.</name></creator><creator><name>Ribas I.</name></creator><creator><name>Bejar V.J.S.</name></creator><creator><name>Cortes-Contreras M.</name></creator><creator><name>Hatzes A.P.,Henning T.</name></creator><creator><name>Hermelo I.</name></creator><creator><name>Ruh H.L.</name></creator><creator><name>Schweitzer A.</name></creator><creator><name>Tabernero H.M.,Zapatero Osorio M.R.</name></creator><date role="Updated">2026-05-22T09:03:30Z</date><date role="Created">2026-05-22T10:02:47Z</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>dwarf-stars</subject><subject>m-stars</subject><subject>visible-astronomy</subject><description>Stellar rotation is closely linked to both the age and the magnetic activity of stars. Through gyrochronology, it provides a means to estimate stellar ages and trace the evolution of planetary systems, and it is also crucial to constrain and correct stellar activity effects for robust exoplanet detection and characterisation. CARMENES is a dual-channel, high-resolution (R&gt;80000) spectrograph that has been highly successful in detecting exoplanets around M-dwarf stars using the radial-velocity technique, and it also enables precise measurements of the projected rotational velocity (vsini) from spectral line broadening. We present an oversampled convolution method incorporating a realistic limb-darkening model to determine vsini from CARMENES spectra by comparing observed spectra with that of a template star. The advantages over existing methods in the literature have been assessed using high-resolution synthetic spectra spanning effective temperatures of 2500-4000K and projected rotational velocities of up to 50km/s. Applied to 392 M dwarfs observed with CARMENES, our method yields vsini measurements (or upper limits at 2km/s) with a median relative uncertainty of 6.8%, substantially smaller than the 15.4% reported in the literature. This work provides the largest uniform catalog of vsini measurements for M dwarfs, including significantly updated values for several targets, along with 36 new targets.</description><source format="bibcode">2026A&amp;A...709A.244V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/709/A244</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></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/A+A/709/A244</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Karmn</name><description>Karmn name (karmn)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Name</name><description>Common name (Name)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>f_vsiniA</name><description>Flag of the adopted vsini (e.g. vsini&lt;2km/s) (adopted_vsini_flag)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>vsiniA</name><description>Adopted vsini for the catalogue (adopted_vsini_kms)</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_vsiniA</name><description>? 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