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<ri:Resource created="2026-01-29T09:44:57Z" status="active" updated="2026-03-02T06:25:50Z" 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>Matter properties ALFALFA galaxies with TNG100 code</title><shortName>J/A+A/706/A64</shortName><identifier>ivo://CDS.VizieR/J/A+A/706/A64</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yang M.</name></creator><creator><name>Zhu L.</name></creator><creator><name>Yu N.</name></creator><creator><name>Lei Y.</name></creator><creator><name>Cai R.</name></creator><creator><name>Wang J.</name></creator><creator><name>Zheng Z.</name></creator><date role="Updated">2026-03-02T06:25:50Z</date><date role="Created">2026-01-29T09:44:57Z</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><subject>h-i-line-emission</subject><subject>spectroscopy</subject><subject>astrometry</subject><subject>radio-galaxies</subject><subject>radio-sources</subject><subject>stellar-masses</subject><subject>galaxy-radii</subject><description>This paper aims to investigate the galaxy-halo connection using a large sample of individual galaxies with HI-integrated spectra. We determined their dark matter content by applying a dynamical method based on HI line widths measured with the curve-of-growth technique, together with inclination corrections inferred from optical images. We built a sample of 2453 gas-rich, predominantly late-type galaxies spanning a stellar mass range of 10^8.7^M_{sun}_ to 10^11.4^M_{sun}_ by matching them one-to-one with their counterparts from the ALFALFA survey and the TNG100 simulation, ensuring a direct match of stellar mass and HI radius. We generated mock images and mock HI-integrated spectra for TNG100 galaxies, and applied the same dynamical method to both ALFALFA and TNG100 mock galaxies to infer their dark matter masses. Across all stellar mass bins, ALFALFA galaxies exhibit lower median dark matter masses than the mock TNG100 simulation results. In each bin, this offset is driven by a tail of galaxies with comparatively low dark matter content, which becomes more prominent toward higher stellar masses. In the highest mass bin (M*&gt;10^11^M_{sun}_), late-type ALFALFA galaxies show a median dark matter mass that is 23% lower than that of their counterparts in the TNG100 dark-matter-only simulation, with 32% of ALFALFA galaxies having M_DM_(&lt;R_HI_)&lt;10^11.5^M_{sun}_, compared to 17% in the mock TNG100 sample. These results suggest that a larger fraction of massive late-type galaxies reside in relatively less massive dark matter haloes than predicted by the TNG100 simulation.</description><source format="bibcode">2026A&amp;A...706A..64Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/706/A64</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/A+A/544/A65">J/A+A/544/A65 : GALEX Arecibo SDSS survey. VI. (Catinella+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/261/21">J/ApJS/261/21 : HI emission line profile of ALFALFA nearby galaxies</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/AJ/160/271">J/AJ/160/271 : A catalog of ~30000 galaxies with ALFALFA-SDSS</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/170">J/AJ/142/170 : ALFALFA survey: the {alpha}.40 HI source catalog</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/460/2143">J/MNRAS/460/2143 : HI size-mass relation of galaxies (Wang+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/34">J/MNRAS/436/34 : GALEX Arecibo SDSS survey. 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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>AGC</name><description>Arecibo General Catalog ID (AGC) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>RAJ2000</name><description>Right Ascension of the optical counterpart (J2000) (RA)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination of the optical counterpart (J2000) (DEC)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Dist</name><description>Luminosity distance from the ALFALFA catalog (Dist)</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dist</name><description>Error in distance (e_Dist)</description><unit>Mpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>Stellar mass (logMstar) (2)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logM*</name><description>Error in stellar mass (e_logMstar)</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMHI</name><description>HI mass total (logMHI) (3)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMHI</name><description>Error in HI mass (e_logMHI)</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RHI</name><description>HI size radius of HI disk (RHI) (4)</description><unit>kpc</unit><ucd>phys.size.radius;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RHI</name><description>Error in HI size (e_RHI)</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b/a</name><description>Axis ratio in optical r-band image (b/a)</description><ucd>phys.angSize;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i</name><description>Optical inclination angle (incl)</description><unit>deg</unit><ucd>src.orbital.inclination;pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_i</name><description>Error in inclination (e_incl)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMdyn</name><description>Dynamical mass within RHI (logMdyn)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMdyn</name><description>Error in dynamical mass (e_logMdyn)</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMHIr</name><description>HI mass enclosed within RHI (logMHI_rhi)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMDM</name><description>Dark matter mass within R_HI (logMdm) (5)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMDM</name><description>Error in dark matter mass (e_logMdm)</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Haynes+2018</name><description>Display the ALFALFA data of Haynes 2011AJ....142..170H, Cat. J/AJ/142/170</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Sloan</name><description>Display the online SDSS-DR16 data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/A+A/706/A64/tng2453</name><description>TNG100 galaxies with matched mock observations</description><column><name>logMgasR</name><description>Total gas mass within R_HI (Mgas_RHI)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMDMR</name><description>Dark matter mass within R_HI (Mdm_RHI)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMdynR</name><description>Total dynamical mass within R_HI (Mdyn_RHI)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></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>IDsbHalo</name><description>TNG100 subhalo ID (subhalo_id)</description><ucd>meta.id</ucd></column><column><name>IDgroup</name><description>TNG100 group ID (group_id)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AGC</name><description>The 1-to-1 Matched AGC number (matched_AGC)</description><ucd>meta.id;meta.main</ucd></column><column><name>Dist</name><description>Luminosity distance from the ALFALFA catalog (Dist)</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Re</name><description>Effective radius 3D (Re)</description><unit>kpc</unit><ucd>phys.size.radius;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*5Re</name><description>Stellar mass within 5Re (Mstar_5Re)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RHI</name><description>HI size defined by definition (RHI_defined)</description><unit>kpc</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMHI2.2R</name><description>HI mass within 2.2 RHI defined (MHI_2.2RHI_defined)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RHIw</name><description>HI size estimated by Wang et al. (2016MNRAS.460.2143W, Cat. J/MNRAS/460/2143) (R_HI)</description><unit>kpc</unit><ucd>phys.size.radius;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*R</name><description>Stellar mass within R_HI (Mstar_RHI)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b/a</name><description>Projected axis ratio of r-band (b/a)</description><ucd>phys.angSize;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMdoR</name><description>Mass for counterparts in dark-matter-only simulation (Mdark_only_RHI)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Paxis</name><description>LOS projection axis in TNG100 (project_axis)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>i</name><description>Inclination angle using Sanchez-Janssen et al. (2010) (incl) (1)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_i</name><description>Error on inclination (e_incl)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W85</name><description>Deprojected W85 HI linewidth of mock HI spectra (W85_cor3d)</description><unit>km/s</unit><ucd>spect.line.width;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_W85</name><description>Error on W85 (e_W85_cor3d)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vrot</name><description>Rotation velocity (Vrot) (2)</description><unit>km/s</unit><ucd>phys.veloc.rotat;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vrot</name><description>Error on Vrot (e_Vrot)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMdynm</name><description>Dynamical mass inferred from mock observation (Mdyn_mock)</description><unit>log(solMass)</unit><ucd>phys.mass;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logMdynm</name><description>Error on logMdynm (e_Mdyn_mock)</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>