<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2014-09-08T13:01:33Z" 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>M31 Cepheids with HST/WFC3</title><shortName>J/ApJ/745/156</shortName><identifier>ivo://CDS.VizieR/J/ApJ/745/156</identifier><altIdentifier>doi:10.26093/cds/vizier.17450156</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Riess A.G.</name></creator><creator><name>Fliri J.</name></creator><creator><name>Valls-Gabaud D.</name></creator><date role="Updated">2017-11-29T11:47:56Z</date><date role="Created">2014-09-08T13:01:33Z</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>hst-photometry</subject><subject>infrared-sources</subject><subject>galaxies</subject><description>We present measurements of 68 classical Cepheids, most detected from the Canada-France-Hawaii Telescope POMME Survey, with periods from 10 to 78 days observed in the near-infrared by the Panchromatic Hubble Andromeda Treasury Program using the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST). The combination of HST's resolution and the use of near-infrared measurements provide a dramatic reduction in the dispersion of the period-luminosity relation over the present optical, ground-based data. Even using random phase magnitudes we measure a dispersion of just 0.17mag, implying a dispersion of just 0.12mag for mean magnitudes. The error in the mean for this relation is 1% in distance. Combined with similar observations of Cepheids in other hosts and independent distance determinations, we measure a distance to M31 of {mu}_0_=24.38+/-0.06(statistical)+/-0.03(systematic), 752+/-27kpc, in good agreement with past measurements though with a better, 3% precision here. The result is also in good agreement with independent distance determinations from two detached eclipsing binaries allowing for an independent calibration of the Cepheid luminosities and a determination of the Hubble constant.</description><source format="bibcode">2012ApJ...745..156R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/745/156</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/AJ/145/106">J/AJ/145/106 : M31 Cepheid disk sample of 1st year of PS1 (Kodric+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/752/95">J/ApJ/752/95 : PHAT stellar cluster survey. I. Year 1 (Johnson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/730/119">J/ApJ/730/119 : HST/WFC3 obs. of Cepheids in SN Ia hosts (Riess+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A70">J/A+A/509/A70 : Study of an eclipsing binary in M31 (Vilardell+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/A+ARV/15.289">J/other/A+ARV/15.289 : Distances of local galaxies (Tammann+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/423">J/A+A/445/423 : WeCAPP Survey. M31 variables (Fliri+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/421/509">J/A+A/421/509 : AGAPE catalogue of M31 variables (Ansari+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/351/1071">J/MNRAS/351/1071 : POINT-AGAPE Survey. M31 variables (An+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/402/113">J/A+A/402/113 : (RI)c photometry of variables in M31 (Joshi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/175">J/AJ/126/175 : M31Y eclipsing binaries and Cepheids (Bonanos+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/504/113">J/ApJ/504/113 : F175W and F275W photometry of M31 and M32 (Brown+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/126/401">J/A+AS/126/401 : M 31 Cepheids periods (Magnier+ 1997)</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/745/156</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/745/156</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/745/156</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/745/156</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/745/156</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/745/156</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/745/156/table1 (M31 Cepheids in WFC3 F160W and F110W)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/745/156/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/745/156/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/745/156/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>10.89624194</ra><dec>41.258875</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2623 2666 2709 2752</spatial><spectral>1.1796835550914393e-19 2.052997531460547e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/745/156?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/745/156/table1</name><description>M31 Cepheids in WFC3 F160W and F110W</description><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>RAJ2000</name><description>[10.81/11.58] Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[41.15/42.22] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>ID</name><description>Identification (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Per</name><description>[10/78] Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160W</name><description>[16/19.3] HST/WFC3 F160W magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F160W</name><description>[0.03/0.05] F160W uncertainty (2)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110W</name><description>[16.5/19.7] HST/WFC3 F110W magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F110W</name><description>[0.02/0.2] F110W uncertainty</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bias</name><description>[0/0.02] Photometric bias</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[O/H]</name><description>[8.8/9.1] Metallicity, 12+log[O/H] based on Zaritsky et al. (1994ApJ...420...87Z)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>D31</name><description>Cross-match within 3" with DIRECT catalog (J/AJ/126/175)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PS1</name><description>Cross-match within 3" Kodric et al. 2013 (Cat. J/AJ/145/106)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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></table></schema></tableset></ri:Resource>