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<ri:Resource created="2021-12-15T08:11:31Z" 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>BH masses and bulge+disk UV-3.6um color relations</title><shortName>J/ApJ/898/83</shortName><identifier>ivo://CDS.VizieR/J/ApJ/898/83</identifier><altIdentifier>doi:10.26093/cds/vizier.18980083</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dullo B.T.</name></creator><creator><name>Bouquin A.Y.K.</name></creator><creator><name>Gil de Paz A.</name></creator><creator><name>Knapen J.H.</name></creator><creator><name>Gorgas J.</name></creator><date role="Updated">2022-03-21T08:47:28Z</date><date role="Created">2021-12-15T08:11:31Z</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>black-holes</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>ultraviolet-astronomy</subject><subject>two-color-diagrams</subject><subject>surveys</subject><description>The tight correlations between supermassive black hole (SMBH) mass (MBH) and the properties of the host galaxy have useful implications for our understanding of the growth of SMBHs and of the evolution of galaxies. Here, we present newly observed correlations between MBH and the host galaxy total UV-[3.6] color (C_UV,tot_, Pearson's r=0.6-0.7) for a sample of 67 galaxies (20 early-type galaxies and 47 late-type galaxies) with directly measured MBH in the Galaxy Evolution Explorer/S4G survey. The colors are carefully measured in a homogeneous manner using the far-UV, near-UV, and 3.6{mu}m magnitudes of the galaxies and their multicomponent structural decompositions in the literature. We find that more massive SMBHs are hosted by (early- and late-type) galaxies with redder colors, but the M_BH_-C_UV,tot_ relations for the two morphological types have slopes that differ at ~2{sigma} level. Early-type galaxies define a red sequence in the M_BH_-C_UV,tot_ diagrams, while late-type galaxies trace a blue sequence. Within the assumption that the specific star formation rate of a galaxy (sSFR) is well traced by L_UV_/L_3.6_, it follows that the SMBH masses for late-type galaxies exhibit a steeper dependence on sSFR than those for early-type galaxies. The M_BH_-C_UV,tot_ and M_BH_-L_3.6,tot_ relations for the sample galaxies reveal a comparable level of vertical scatter in the log MBH direction, approximately 5%-27% more than the vertical scatter of the M_BH_-{sigma} relation. Our M_BH_-C_UV,tot_ relations suggest different channels of SMBH growth for early- and late-type galaxies, consistent with their distinct formation and evolution scenarios. These new relations offer the prospect of estimating SMBH masses reliably using the galaxy color alone. Furthermore, we show that they are capable of estimating intermediate black hole masses in low-mass early- and late-type galaxies.</description><source format="bibcode">2020ApJ...898...83D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/898/83</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/VII/237">VII/237 : HYPERLEDA. I. 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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>Name</name><description>Galaxy Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>mFUV</name><description>[9.6/18.1] Dust-corrected FUV total (bulge+disk) apparent magnitude</description><unit>mag</unit><ucd>phot.mag;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_mFUV</name><description>[0.2/0.64] Upper uncertainty in mFUV</description><unit>mag</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mFUV</name><description>[0.2/0.64] Lower uncertainty in mFUV</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mNUV</name><description>[9.29/15.77] Dust-corrected NUV total (bulge+disk) apparent magnitude</description><unit>mag</unit><ucd>phot.mag;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_mNUV</name><description>[0.2/0.63] Upper uncertainty in mNUV</description><unit>mag</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mNUV</name><description>[0.2/0.63] Lower uncertainty in mNUV</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>m3.6</name><description>[6.2/12] Dust-corrected 3.6um total (bulge+disk) apparent magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_m3.6</name><description>[0.2/0.61] Upper uncertainty in m3.6</description><unit>mag</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_m3.6</name><description>[0.2/0.61] Lower uncertainty in m3.6</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BTuv</name><description>[0.01/1]? NUV and FUV Bulge-to-total ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BTir</name><description>[0/1] 3.6um Bulge-to-total ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DTuv</name><description>[0.37/0.99]? NUV and FUV Disk-to-total ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DTir</name><description>[0.17/90]? 3.6um Disk-to-total ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DcorrB3.6</name><description>[0.01/0.57] Bulge dust correction in 3.6um</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DcorrD3.6</name><description>[0.04/0.24]? Disk dust correction in 3.6um</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DcorrBfuv</name><description>[0.17/2.32]? Bulge dust correction in FUV</description><unit>mag</unit><ucd>phot.mag;em.UV;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DcorrDfuv</name><description>[0.53/1.84]? Disk dust correction in FUV</description><unit>mag</unit><ucd>phot.mag;em.UV;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DcorrBnuv</name><description>[0.18/2.34]? Bulge dust correction in NUV</description><unit>mag</unit><ucd>phot.mag;em.UV;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DcorrDnuv</name><description>[0.45/1.85]? Disk dust correction in NUV</description><unit>mag</unit><ucd>phot.mag;em.UV;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logMBH</name><description>[4.4/9.4] Supermassive black hole mass (2)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_logMBH</name><description>[0.03/2.1] Upper uncertainty in logMBH</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMBH</name><description>[0.03/7.6] Lower uncertainty in logMBH</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V16</name><description>Display data from van den Bosch, 2016, J/ApJ/831/134</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>B18</name><description>Display data from Bouquin+ 2018, J/ApJS/234/18</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></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><column><name>NED</name><description>NED column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>LEDA</name><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/898/83/tabled1</name><description>Predicted black hole masses for 1382 GALEX/S^4^G galaxies with no measured BH masses</description><column><name>Name</name><description>Galaxy Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">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>TType</name><description>[-5/10] Galaxy T-type from HyperLeda</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMBH-FUV</name><description>[2.6/10] Tentative BH mass, M_BH_-C_FUV,tot_ (1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMBH-NUV</name><description>[3/10] Tentative BH mass, M_BH_-C_NUV,tot_ (1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B18</name><description>Display data from Bouquin+ 2018, J/ApJS/234/18</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></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><column><name>NED</name><description>NED column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>LEDA</name><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>