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<ri:Resource created="2025-02-20T14:51:56Z" status="active" updated="2025-06-30T20:16:26Z" 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>BTFR's study of ~10000 HyperLEDA galaxies</title><shortName>J/MNRAS/511/6160</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/511/6160</identifier><altIdentifier>doi:10.26093/cds/vizier.75116160</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kourkchi E.</name></creator><creator><name>Tully R.B.</name></creator><creator><name>Courtois H.M.</name></creator><creator><name>Dupuy A.</name></creator><creator><name>Guinet D.</name></creator><date role="Updated">2025-06-30T20:16:26Z</date><date role="Created">2025-02-20T14:51:56Z</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>galaxies</subject><subject>galaxy-groups</subject><subject>infrared-astronomy</subject><subject>visible-astronomy</subject><subject>radio-sources</subject><subject>photometry</subject><subject>spectroscopy</subject><subject>h-i-line-emission</subject><subject>stellar-masses</subject><subject>radial-velocity</subject><subject>astrometry</subject><description>The interstellar gas in spiral galaxies can constitute a significant fraction of the baryon mass and it has been demonstrated that the sum of stellar and gas components correlates well with the kinematic signature of the total mass content, the widths of H I line profiles. The correlation of baryonic mass with H I linewidths is used here to obtain distances for 9984 galaxies extending to ~0.05c. The sample is H I flux limited and a correction is required to account for an H I selection bias. The absolute scale is established by 64 galaxies with known distances from studies of Cepheid variables and/or the magnitudes of stars at the tip of the red giant branch. The calibration of the baryonic relationship results in a determination of the Hubble constant of H_0_ = 75.5 +/- 2.5 km/s/Mpc. The error estimate is statistical. This material will be combined with contributions from other methodologies in a subsequent paper where systematic uncertainties will be investigated.</description><source format="bibcode">2022MNRAS.511.6160K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/511/6160</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/902/145">J/ApJ/902/145 : Cosmicflows-4 Tully-Fisher distances (Kourkchi+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/646/A113">J/A+A/646/A113 : Towards Cosmicflows-4 HI data catalog (Dupuy+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1938">J/AJ/138/1938 : EDD All Digital HI profile catalog (Courtois+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/171">J/AJ/149/171 : 2MASS galaxy group catalog (Tully, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/843/16">J/ApJ/843/16 : Galaxy groups within 3500km/s (Kourkchi+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/2005">J/MNRAS/414/2005 : Cosmic flows observations (Courtois+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/184">J/ApJ/676/184 : Peculiar motion away from the Local Void (Tully+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/237">VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/238">VII/238 : HYPERLEDA. II. Homogenized HI data (Paturel+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/861/49">J/ApJ/861/49 : ALFALFA extragalactic HI source catalog (Haynes+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/816/L14">J/ApJ/816/L14 : Tully-Fisher relation in disk galaxies from SPARC</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/792/129">J/ApJ/792/129 : WISE W1/W2 Tully-Fisher relation calibrator data</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/75">VII/75 : Infrared Photometry and 21cm data for nearby galaxies</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/896/3">J/ApJ/896/3 : Cosmicflows-4: Tully-Fisher relation calibrations</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/884/82">J/ApJ/884/82 : SDSS, WISE and HI data of local spiral galaxies</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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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>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (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>indexed</flag></column><column><name>PGC</name><description>The ID number of the galaxy in the Principal Galaxy Catalog (PGC) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>f_PGC</name><description>[] Quality flag (Flag) (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>DMav</name><description>? The average of distance moduli measured using optical and infrared data (DM_av_)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_DMav</name><description>? The reported DM_av_ uncertainty is the maximum adjusted error of the optical and infrared moduli (errDM_av_)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DMriz</name><description>? The measured distance modulus from the averaged optical BTFRi (DM_riz_) (3)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_DMriz</name><description>[]? 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J/ApJ/676/184 (V_LS_)</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VCMB</name><description>Radial velocity in the rest frame of the cosmic microwave background (V_CMB)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.cmb</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>fg</name><description>The cosmological correction factor f_g_ (f_g_) (13)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f</name><description>The cosmological correction factor f_j_ (f_j_) (10)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logWimx</name><description>The logarithm of the inclination-corrected H I linewidth (logW^i^_mx_) (11)</description><unit>log(km.s**-1)</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logWimx</name><description>Mean error of logWimx (errlogWimx)</description><unit>log(km.s**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F21</name><description>The H I 21-cm integrated flux (F_21_)</description><unit>Jy.km/s</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F21</name><description>Mean error of F21 (errF_21_)</description><unit>Jy.km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i</name><description>The inclination angle of the galaxy (Inc)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_i</name><description>? Mean error of i (errInc)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>g*mag</name><description>? The SDSS g corrected magnitude in the AB system (g*) (12)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r*mag</name><description>? The SDSS r corrected magnitude in the AB system (r*) (12)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>i*mag</name><description>? The SDSS i corrected magnitude in the AB system (i*) (12)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>z*mag</name><description>? The SDSS z corrected magnitude in the AB system (z*) (12)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W1*mag</name><description>? The WISE W1 corrected magnitude in the AB system (W1*) (12)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W2*mag</name><description>? The WISE W2 corrected magnitude in the AB system (W2*) (12)</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>QS</name><description>? The manually assigned quality grade for the photometry of SDSS images ranging from 0 for the poorest to 5 for the best photometric quality (Q_S_)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SGL</name><description>Supergalactic longitude in supergalactic reference frame (SGL)</description><unit>deg</unit><ucd>pos</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SGB</name><description>Supergalactic latitude in supergalactic reference frame (SGB)</description><unit>deg</unit><ucd>pos</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Nkt</name><description>Number of galaxies in the parent group identified in KourKchi &amp; Tully 2017ApJ...843...16K, Cat. J/ApJ/843/16 (N_kt_)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N15</name><description>Number of galaxies in the parent group identified in Tully 2015AJ....149..171T, Cat. J/AJ/149/171 (N_15_)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SGLg</name><description>Supergalactic longitude of parent group in the supergalactic frame of reference (SGL^g^)</description><unit>deg</unit><ucd>meta.id.parent;pos.supergalactic.lon;pos.lg</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SGBg</name><description>Supergalactic latitude of parent group in the supergalactic frame of reference (SGB^g^)</description><unit>deg</unit><ucd>meta.id.parent;pos.supergalactic.lat;pos.lg</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vgh</name><description>The average velocity of the parent group in heliocentric rest frame (V^g^_h_)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VgLS</name><description>The average velocity of the parent group in Local Sheet rest frame (V^g^_LS_)</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VgCMB</name><description>The average velocity of the parent group in CMB rest frame (V^g^_CMB_)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.cmb</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>