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<ri:Resource created="2023-01-09T15:21:28Z" 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>Gaia-ASAS-SN classical Cepheid sample. I.</title><shortName>J/ApJ/914/127</shortName><identifier>ivo://CDS.VizieR/J/ApJ/914/127</identifier><altIdentifier>doi:10.26093/cds/vizier.19140127</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Inno L.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Stanek K.Z.</name></creator><creator><name>Jayasinghe T.</name></creator><creator><name>Poggio E.</name></creator><creator><name>Drimmel R.,Rotundi A.</name></creator><date role="Updated">2023-01-24T12:10:28Z</date><date role="Created">2023-01-09T15:21:28Z</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>milky-way-galaxy</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We present a well-defined and characterized all-sky sample of classical Cepheids in the Milky Way, obtained by combining two time-domain all-sky surveys: Gaia DR2 (Gaia Col. 2018; see I/345) and All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee+ 2014AAS...22323603S). We first use parallax and variability information from Gaia to select ~30000 bright (G&lt;17) Cepheid candidates with M_K_{&lt;}-1. We then analyze their ASAS-SN V-band light curves, determining periods and classifying the light curves using their Fourier parameters. This results in ~1900 likely Galactic Cepheids, which we estimate to be &gt;~90% complete and pure within our adopted selection criteria. This is the largest all-sky sample of Milky Way Cepheids that has such a well-characterized selection function, needed for population modeling and for systematic spectroscopic follow-up foreseen with Sloan Digital Sky Survey-V. About 130 of these potential Cepheids have not been documented in the literature even as possible candidates.</description><source format="bibcode">2021ApJ...914..127I</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/914/127</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/576/A30">J/A+A/576/A30 : NIR LC templates for classical Cepheids (Inno+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/241">J/AJ/156/241 : Variable stars measured by ATLAS (Heinze+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/68/315">J/AcA/68/315 : OGLE Galactic Cepheids (Udalski+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/622/A60">J/A+A/622/A60 : Gaia DR2 misclassified RR Lyrae list (Clementini+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/58">J/ApJ/883/58 : Cepheids from VVV in Gal. midplane (Dekany+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/482/3058">J/MNRAS/482/3058 : New variable stars towards Galactic Bulge (Kains+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A14">J/A+A/625/A14 : Reclassification of Cepheids in Gaia DR2 (Ripepi+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/365.478">J/other/Sci/365.478 : Milky Way classical Cepheids sample (Skowron+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/18">J/ApJS/249/18 : The ZTF catalog of periodic variable stars (Chen+, 2020)</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/ApJ/914/127</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/914/127</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/914/127</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/914/127</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>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>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2015.5 (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2015.5 (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>Mode</name><description>Pulsation mode ("F"=1269 occurrences; or "1O"=622 occurrences)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>PF</name><description>[0.3/64.1] Period from Lomb-Scargle (LS) method</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N</name><description>[46/786] Number of observing epochs</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vmag</name><description>[7.1/17.3] Mean V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A1</name><description>[0.007/0.6] Amplitude, A_1_</description><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R21</name><description>[0.003/0.8] Ratio of 2nd to 1st Fourier amplitudes</description><ucd>phot.mag;arith.ratio;stat.Fourier</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R31</name><description>[0.003/0.5] Ratio of 3rd to 1st Fourier amplitudes</description><ucd>phot.mag;arith.ratio;stat.Fourier</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>phi21</name><description>[0.009/6.3] Ratio of 2nd to 1st phase differences</description><ucd>time.phase;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>phi31</name><description>[-6.2/6.3] Ratio of 3rd to 1st phase differences</description><ucd>time.phase;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DeltaG</name><description>[0.06/2.8] Gaia G band variability</description><unit>mag</unit><ucd>src.var.amplitude;phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ratio</name><description>[1.1/1.9] Ratio of Gaia Blue to Red passband variability</description><ucd>phot.mag;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RA_ICRS</name><description>Right Ascension (ICRS) at Epoch=2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>[-78.7/79.6] Declination (ICRS) at Epoch=2015.5</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Cont</name><description>[0/1] Possible contamination flag (1=contaminated)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Lit</name><description>Source of photometric data (1)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>ID</name><description>Stellar identifier from literature</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>ModeLit</name><description>Pulsation mode</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Per</name><description>[0.37/51.42]? 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