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<ri:Resource created="2015-07-24T13:30:38Z" 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>HET Massive Galaxy Survey (HETMGS)</title><shortName>J/ApJS/218/10</shortName><identifier>ivo://CDS.VizieR/J/ApJS/218/10</identifier><altIdentifier>doi:10.26093/cds/vizier.22180010</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>van den Bosch R.C.E.</name></creator><creator><name>Gebhardt K.</name></creator><creator><name>Gultekin K.</name></creator><creator><name>Yildirim A.</name></creator><creator><name>Walsh J.L.</name></creator><date role="Updated">2018-01-02T13:42:35Z</date><date role="Created">2015-07-24T13:30:38Z</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>spectroscopy</subject><subject>radial-velocity</subject><subject>galaxy-kinematics</subject><subject>surveys</subject><description>We have conducted an optical long-slit spectroscopic survey of 1022 galaxies using the 10m Hobby-Eberly Telescope (HET) at McDonald Observatory. The main goal of the HET Massive Galaxy Survey (HETMGS) is to find nearby galaxies that are suitable for black hole mass measurements. In order to measure accurately the black hole mass, one should kinematically resolve the region where the black hole dominates the gravitational potential. For most galaxies, this region is much less than an arcsecond. Thus, black hole masses are best measured in nearby galaxies with telescopes that obtain high spatial resolution. The HETMGS focuses on those galaxies predicted to have the largest sphere-of-influence, based on published stellar velocity dispersions or the galaxy fundamental plane. To ensure coverage over galaxy types, the survey targets those galaxies across a face-on projection of the fundamental plane. We present the sample selection and resulting data products from the long-slit observations, including central stellar kinematics and emission line ratios. The full data set, including spectra and resolved kinematics, is available online. Additionally, we show that the current crop of black hole masses are highly biased toward dense galaxies and that especially large disks and low dispersion galaxies are under-represented. This survey provides the necessary groundwork for future systematic black hole mass measurement campaigns.</description><source format="bibcode">2015ApJS..218...10V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/218/10</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/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/259">VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/443/1231">J/MNRAS/443/1231 : 6dF Galaxy Survey: Fundamental Plane data (Campbell+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/93">J/AJ/147/93 : Simulation of massive early type galaxies (Do+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/116">J/ApJ/775/116 : z&lt;0.06 active BH galaxies from SDSS-DR8 (Reines+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/45">J/AJ/146/45 : Spectroscopy of 6 early-type galaxies (Rusli+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/201/29">J/ApJS/201/29 : Velocity dispersions in active galaxies (Harris+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/26">J/ApJS/199/26 : The 2MASS Redshift Survey (2MRS) (Huchra+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/413/813">J/MNRAS/413/813 : ATLAS3D project. I. (Cappellari+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/727/20">J/ApJ/727/20 : The Megamaser Cosmology Project (MCP). III. (Kuo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/1">J/ApJS/183/1 : Catalog of central stellar velocity dispersions (Ho+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/856">J/ApJ/692/856 : Supermassive BH masses upper limits (Beifiori+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/670/105">J/ApJ/670/105 : Velocity profile of NGC 4151 (Onken+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/808">J/ApJ/662/808 : Cusp radius in luminous elliptical galaxies (Lauer+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/703">J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/305/259">J/MNRAS/305/259 : EFAR galaxies redshifts+velocity dispersions (Wegner+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/100/105">J/ApJS/100/105 : Stellar velocity dispersions. 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