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<ri:Resource created="2022-03-09T09:37:08Z" 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>GBT HI obs. of ultradiffuse galaxies</title><shortName>J/ApJ/902/39</shortName><identifier>ivo://CDS.VizieR/J/ApJ/902/39</identifier><altIdentifier>doi:10.26093/cds/vizier.19020039</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Karunakaran A.</name></creator><creator><name>Spekkens K.</name></creator><creator><name>Zaritsky D.</name></creator><creator><name>Donnerstein R.L.,Kadowaki J.</name></creator><creator><name>Dey A.</name></creator><date role="Updated">2023-09-05T06:57:17Z</date><date role="Created">2022-03-09T09:37:08Z</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>h-i-line-emission</subject><subject>galaxies</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>galaxy-classification-systems</subject><subject>two-color-diagrams</subject><description>We present neutral hydrogen (HI) observations using the Robert C. Byrd Green Bank Telescope (GBT) of 70 optically detected UDG candidates in the Coma region from the Systematically Measuring Ultra-Diffuse Galaxies survey (SMUDGes). We detect HI in 18 targets, confirming nine to be gas-rich UDGs and the remainder to be foreground dwarfs. None of our HI-detected UDGs are Coma Cluster members and all but one are in low-density environments. The HI-detected UDGs are bluer and have more irregular morphologies than the redder, smoother candidates not detected in HI, with the combination of optical color and morphology being a better predictor of gas richness than either parameter alone. There is little visual difference between the gas-rich UDGs and the foreground dwarfs in the SMUDGes imaging, and distances are needed to distinguish between them. We find that the gas richnesses of our HI-confirmed UDGs and those from other samples scale with their effective radii in two stellar mass bins, possibly providing clues to their formation. We attempt to place our UDGs on the baryonic Tully-Fisher relation (BTFR) using optical ellipticities and turbulence-corrected HI line widths to estimate rotation velocities, but the potential systematics associated with fitting smooth Sersic profiles to clumpy, low-inclination disks of low surface brightness precludes a meaningful analysis of potential BTFR offsets. These observations are a pilot for a large campaign now under way at the GBT to use the HI properties of gas-rich UDGs to quantitatively constrain how these galaxies form and evolve.</description><source format="bibcode">2020ApJ...902...39K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/902/39</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/VIII/77">VIII/77 : HI spectral properties of galaxies (Springob+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/22">J/AJ/113/22 : Tully-Fisher Relation. I. 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xsi:type="vs:VOTableType">float</dataType></column><column><name>logMHI</name><description>[6.45/9.22] Log, H I mass (3)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMHI</name><description>[0.08/0.72] Uncertainty in logMHI</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMstar</name><description>[5.64/8.57] Log, stellar mass (4)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</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>DV</name><description>[5/25] Velocity resolution of spectrum used to compute H I properties</description><unit>km/s</unit><ucd>spect.resolution</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>rmsDV</name><description>[0.45/4.76] RMS noise of spectrum at {Delta}V</description><unit>mJy</unit><ucd>instr.det.noise</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vsys</name><description>[420/11585] Heliocentric systemic velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Vsys</name><description>[1/6] Uncertainty in Vsys</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>W50c</name><description>[8/102] Velocity width of the HI detection (1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_W50c</name><description>[2/8] Uncertainty in W50c</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SHI</name><description>[0.13/4.37] Integrated H I flux</description><unit>Jy.km/s</unit><ucd>phot.flux.density;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SHI</name><description>[0.04/0.21] Uncertainty in SHI</description><unit>Jy.km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMstar</name><description>[0.2/0.75] Uncertainty in logMstar</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMbary</name><description>[6.68/9.41] Log, baryonic mass, 1.33*MHI+Mstar</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMbary</name><description>[0.08/0.72] Uncertainty in logMbary</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Reff</name><description>[0.2/5.85] Effective radius using reff (Table 1) and DHI</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Reff</name><description>[0.02/0.62] Uncertainty in Reff</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/902/39/table3</name><description>HI properties of dwarfs</description><column><name>SMDG</name><description>Adopted SMUDGes UDG candidate name (HHMMSSs+DDMMSS; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</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>DV</name><description>[5/25] Velocity resolution of spectrum used to compute H I properties</description><unit>km/s</unit><ucd>spect.resolution</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>rmsDV</name><description>[0.45/4.76] RMS noise of spectrum at {Delta}V</description><unit>mJy</unit><ucd>instr.det.noise</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vsys</name><description>[420/11585] Heliocentric systemic velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Vsys</name><description>[1/6] Uncertainty in Vsys</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>W50c</name><description>[8/102] Velocity width of the HI detection (1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_W50c</name><description>[2/8] Uncertainty in W50c</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SHI</name><description>[0.13/4.37] Integrated H I flux</description><unit>Jy.km/s</unit><ucd>phot.flux.density;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SHI</name><description>[0.04/0.21] Uncertainty in SHI</description><unit>Jy.km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DHI</name><description>[6/165.5] Distance estimate (2)</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMHI</name><description>[6.45/9.22] Log, H I mass (3)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMHI</name><description>[0.08/0.72] Uncertainty in logMHI</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMstar</name><description>[5.64/8.57] Log, stellar mass (4)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMstar</name><description>[0.2/0.75] Uncertainty in logMstar</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMbary</name><description>[6.68/9.41] Log, baryonic mass, 1.33*MHI+Mstar</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMbary</name><description>[0.08/0.72] Uncertainty in logMbary</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Reff</name><description>[0.2/5.85] Effective radius using reff (Table 1) and DHI</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Reff</name><description>[0.02/0.62] Uncertainty in Reff</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/902/39/table4</name><description>HI properties of non-detections</description><column><name>SMDG</name><description>Adopted SMUDGes UDG candidate name (HHMMSSs+DDMMSS; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</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>f_SMDG</name><description>Flag on upper limit, *= Offset in GBT pointing (see Table 1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Dlim</name><description>[3.8/100.0] Adopted distance (1)</description><unit>Mpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_Dlim</name><description>Source for Dlim (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logMHIlim</name><description>[5.94/8.8] 5{sigma} upper limit on MHI</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MHIlim/Lg</name><description>[0.25/3.5] Upper limit on the gas richness</description><unit>solMass/solLum</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/902/39/table5</name><description>Inclinations and rotation velocities</description><column><name>SMDG</name><description>Adopted SMUDGes UDG candidate name (HHMMSSs+DDMMSS; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</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>OT</name><description>Object type: UDG or foreground dwarf</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>sSet</name><description>[1/2] Object type (1)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>iGF</name><description>[33/69] Inclination calculated using Eq.4 (2)</description><unit>deg</unit><ucd>src.orbital.inclination;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VGF</name><description>[3/53] Rotational velocity (3)</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>iBTFR</name><description>[4/20]? Inclination required to lie on the BTFR (4)</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>