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<ri:Resource created="2017-02-24T14:20:58Z" 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>Tully-Fisher relation in disk galaxies from SPARC</title><shortName>J/ApJ/816/L14</shortName><identifier>ivo://CDS.VizieR/J/ApJ/816/L14</identifier><altIdentifier>doi:10.26093/cds/vizier.18169014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lelli F.</name></creator><creator><name>McGaugh S.S.</name></creator><creator><name>Schombert J.M.</name></creator><date role="Updated">2017-06-19T07:57:15Z</date><date role="Created">2017-02-24T14:20:58Z</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-rotation</subject><description>In a {Lambda} cold dark matter ({Lambda}CDM) cosmology, the baryonic Tully-Fisher relation (BTFR) is expected to show significant intrinsic scatter resulting from the mass-concentration relation of dark matter halos and the baryonic-to-halo mass ratio. We study the BTFR using a sample of 118 disk galaxies (spirals and irregulars) with data of the highest quality: extended HI rotation curves (tracing the outer velocity) and Spitzer photometry at 3.6{mu}m (tracing the stellar mass). Assuming that the stellar mass-to-light ratio ({Upsilon}_*_) is nearly constant at 3.6{mu}m, we find that the scatter, slope, and normalization of the BTFR systematically vary with the adopted {Upsilon}_*_. The observed scatter is minimized for {Upsilon}_*_&gt;~0.5M_{Sun}_/L_{Sun}_, corresponding to nearly maximal disks in high-surface-brightness galaxies and BTFR slopes close to ~4. For any reasonable value of {Upsilon}_*_, the intrinsic scatter is ~0.1dex, below general {Lambda}CDM expectations. The residuals show no correlations with galaxy structural parameters (radius or surface brightness), contrary to the predictions from some semi-analytic models of galaxy formation. These are fundamental issues for {Lambda}CDM cosmology.</description><source format="bibcode">2016ApJ...816L..14L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/816/L14</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/827/L19">J/ApJ/827/L19 : Central surface densities in SPARC disk galaxies (Lelli+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/157">J/AJ/152/157 : Mass models for 175 disk galaxies with SPARC (Lelli+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/134">J/AJ/147/134 : Tully-Fisher relation for S^4^G galaxies (Zaritsky+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A71">J/A+A/566/A71 : HI study of 18 nearby dwarf galaxies (Lelli+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/94">J/ApJ/765/94 : Calibration of the mid-IR Tully-Fisher relation (Sorce+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/821">J/ApJ/669/821 : CO Tully-Fisher relation for host galaxies of QSOs (Ho+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/945">J/AJ/134/945 : Tully-Fisher relation for SDSS galaxies (Pizagno+, 2007)</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/816/L14</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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