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<ri:Resource created="2024-06-14T10:38:56Z" 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>VELOCE I. Cepheids High-precision RVs</title><shortName>J/A+A/686/A177</shortName><identifier>ivo://CDS.VizieR/J/A+A/686/A177</identifier><altIdentifier>doi:10.26093/cds/vizier.36860177</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Anderson R.I.</name></creator><creator><name>Viviani G.</name></creator><creator><name>Shetye S.S.</name></creator><creator><name>Mowlavi N.</name></creator><creator><name>Eyer L.</name></creator><creator><name>Palaversa L.,Holl B.</name></creator><creator><name>Blanco-Cuaresma S.</name></creator><creator><name>Kravchenko K.</name></creator><creator><name>Pawlak M.</name></creator><creator><name>Cruz Reyes M.,Khan S.</name></creator><creator><name>Netzel H.E.</name></creator><creator><name>Loebling L.</name></creator><creator><name>Papics P.I.</name></creator><creator><name>Postel A.</name></creator><creator><name>Roelens M.,Spetsieri Z.T.</name></creator><creator><name>Thoul A.</name></creator><creator><name>Zak J.</name></creator><creator><name>Bonvin V.</name></creator><creator><name>Martin D.V.</name></creator><creator><name>Millon M.,Saesen S.</name></creator><creator><name>Wyttenbach A.</name></creator><creator><name>Figueira P.</name></creator><creator><name>Marmier M.</name></creator><creator><name>Prins S.</name></creator><creator><name>Raskin G.,van Winckel H.</name></creator><date role="Updated">2024-11-07T20:03:53Z</date><date role="Created">2024-06-14T10:38:56Z</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>variable-stars</subject><subject>spectroscopic-binary-stars</subject><subject>radial-velocity</subject><description>We present the first data release of VELOCE, a project dedicated to measuring high-precision radial velocities (RVs) of Galactic classical Cepheids (henceforth: Cepheids). VELOCE DR1 comprises 18225 RV measurements of 258 bona fide classical Cepheids on both hemispheres collected mainly between 2010 and 2022, as well as 1,161 observations of 164 additional stars, the majority of which were previously misclassified as Cepheids. The median per-observation RV uncertainty for Cepheids is 0.037km/s and reaches 2m/s for the brightest stars observed with Coralie. Non- variable standard stars were used to characterize RV zero-point stability and to provide a base for future cross-calibrations. We determined zero-point differences between VELOCE and 31 literature data sets using template fitting, which we also used to investigate linear period changes of 146 Cepheids. Seventy-three spectroscopic binary Cepheids and 13 candidate binary Cepheids were identified using VELOCE data alone and are investigated in detail in a companion paper (VELOCE II). VELOCE DR1 provides several new insights into the pulsational variability of Cepheids. Chiefly among these are: a) the most detailed description of the Hertzsprung progression based on RVs to date, b) the identification of double-peaked bumps in the pulsation curve, and c) clear evidence that virtually all Cepheids feature spectroscopic variability signals that lead to modulated RV variability at the level of tens to hundreds of m/s that cannot be satisfactorily modeled using single-periodic Fourier series. We identified 36 stars exhibiting such modulated variability, of which four also exhibit orbital motion. Linear radius variations depend strongly on pulsation period, and a steep increase in slope of the delta R/p vs log P-relation is found near 10 d. This effect, combined with significant RV amplitude differ- ences at fixed period challenge the existence of a tight relation between Baade-Wesselink projection factors and pulsation periods. We investigated the accuracy of RV time-series measurements, v_gamma_, and RV amplitudes published by the ESA mission Gaia's third data release and determined an offset of 0.65+/-0.11km/s relative to VELOCE. Whenever possible, we recommend adopting a single set of template correlation parameters for distinct classes of large amplitude variable stars to avoid systematic offsets in v_gamma among stars belonging to the same class. Peak-to-peak amplitudes of Gaia RVs exhibit significant (16%) dispersion. Potential differences of RV amplitudes require further inspection, notably in the context of projection factor calibration.</description><source format="bibcode">2024A&amp;A...686A.177A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/686/A177</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/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/674/A22">J/A+A/674/A22 : Gaia DR3. 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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>Ref</name><description>Literature or instrument reference</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>Nstars</name><description>[1/68] Number of stars used to determine the zero-point</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nclusters</name><description>[1/219] Number of clusters used to determine the zero-point</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ZP</name><description>Zero-point difference between VELOCE and the reference</description><unit>km/s</unit><ucd>meta.ref;pos.frame;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_ZP</name><description>Uncertainty on the zero-point difference</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BibCodes</name><description>Bibcode for the references</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="59*">char</dataType></column></table><table><name>J/A+A/686/A177/table6</name><description>Linear period change rates (dP/dt)</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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Phase difference between the fifth and the first Fourier harmonics</description><unit>rad</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/686/A177/tableb1</name><description>Other targets in VELOCE</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType><flag>nullable</flag></column><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>Name</name><description>Name of the target</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>NRV</name><description>[0/199] Number of radial velocity measurements</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CCFpeak</name><description>[yn] Peak of the cross-correlation function flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CCFodd</name><description>[yn?] CCF looks significantly different from those of classical Cepheids flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ncomp</name><description>Specify if more than one absorption component was noticed</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Emission</name><description>Exhibits signs of emission features</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>vRV</name><description>[yn? NA] RV variability flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>vFWHW</name><description>[yn? NA] FWHM variability flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>vAsym</name><description>[yn? NA] Line asymmetry variability flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>vLineDepth</name><description>[yn? NA] Line depth variability flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>CCFnote</name><description>Additional notes on the CCF</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="46*">char</dataType></column><column><name>GaiaDR3</name><description>Gaia DR3 source_id</description><ucd>meta.id</ucd></column><column><name>Class</name><description>Gaia DR3 classification</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>G22</name><description>Gavras et al. (2023A&amp;A...674A..22G, Cat. J/A+A/674/A22) classification</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>