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<ri:Resource created="2026-04-27T08:37:19Z" status="active" updated="2026-04-27T08:18:07Z" 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>SOUX AGN sample with SDSS-XMM-Newton surveys</title><shortName>J/MNRAS/520/2781</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/520/2781</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kynoch D.</name></creator><creator><name>Mitchell J.A.J.</name></creator><creator><name>Ward M.J.</name></creator><creator><name>Done C.</name></creator><creator><name>Lusso E.</name></creator><creator><name>Landt H.</name></creator><date role="Updated">2026-04-27T08:18:07Z</date><date role="Created">2026-04-27T08:37:19Z</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>quasars</subject><subject>active-galactic-nuclei</subject><subject>black-holes</subject><subject>astronomical-object-identification</subject><subject>accretion</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>x-ray-sources</subject><subject>radio-sources</subject><subject>ultraviolet-astronomy</subject><subject>line-intensities</subject><subject>galaxy-kinematics</subject><description>We assemble a sample of 696 type 1 active galactic nuclei (AGN) up to a redshift of z = 2.5, all of which have an SDSS spectrum containing at least one broad emission line (H{alpha}, H{beta}, or Mg II) and an XMM-Newton X-ray spectrum containing at least 250 counts in addition to simultaneous optical/ultraviolet photometry from the XMM Optical Monitor. Our sample includes quasars and narrow-line Seyfert 1s: thus our AGN span a wide range in luminosity, black hole mass, and accretion rate. We determine single-epoch black hole mass relations for the three emission lines and find that they provide broadly consistent mass estimates whether the continuum or emission line luminosity is used as the proxy for the broad emission line region radius. We explore variations of the UV/X-ray energy index {alpha}_ox_ with the UV continuum luminosity and with black hole mass and accretion rate, and make comparisons to the physical quasar spectral energy distribution model QSOSED. The majority of the AGN in our sample lie in a region of parameter space with 0.02 &lt; L/L_Edd_ &lt; 2 as defined by this model, with narrow- line type 1 AGN offset to lower masses and higher accretion rates than typical broad-line quasars. We find differences in the dependence of {alpha}_ox_ on UV luminosity between both narrow/broad-line and radio-loud/quiet subsets of AGN: {alpha}_ox_ has a slightly weaker dependence on UV luminosity for broad-line AGN and radio-loud AGN have systematically harder {alpha}_ox_.</description><source format="bibcode">2023MNRAS.520.2781K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/520/2781</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/MNRAS/504/5726">J/MNRAS/504/5726 : IR lines of AGNs accretion disk (Fernandez-Ontiveros+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/496/245">J/MNRAS/496/245 : L_x_-L_uv_-L_radio_ relation in radio-loud quasars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/422/3268">J/MNRAS/422/3268 : Relation between X-ray and optical spectra (Jin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/581">J/MNRAS/383/581 : Broad-line Balmer decrements in blue AGN (Dong+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/843/30">J/ApJ/843/30 : MgII line vs 3000{AA} continuum analysis in 68 QSOs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/819/154">J/ApJ/819/154 : SDSS-DR7 QSOs with X-ray and UV luminosities (Lusso+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/125">J/ApJ/753/125 : Near-IR spectroscopy follow-up of 60 SDSS-DR7 QSOs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/682">J/ApJ/613/682 : AGN central masses and broad-line region sizes</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/17">J/ApJS/249/17 : SDSS QSO DR14 spectral properties (Rakshit+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/241/34">J/ApJS/241/34 : The SDSS Reverberation Mapping (SDSS-RM) project</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/39">J/ApJS/229/39 : Narrow line Seyfert 1 galaxies from SDSS-DR12</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/4">J/ApJS/206/4 : SED and bolometric corrections for luminous QSOs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/128">J/ApJS/166/128 : Narrow line Seyfert 1 galaxies from SDSS-DR3 (Zhou+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/387">J/AJ/130/387 : SDSS-ROSAT AGN data (Strateva+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/663/L7">J/A+A/663/L7 : Quasars as high-redshift standard candles (Sacchi+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A34">J/A+A/512/A34 : XMM-COSMOS Type 1 AGNs (Lusso+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/76">VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/286">VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/59">IX/59 : XMM-Newton Serendipitous Source Catalogue 4XMM-DR9</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/340">II/340 : XMM-OM Serendipitous Source Survey Catalogue 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Logarithm of the continuum luminosity at 3000 {AA} rest-frame from the SDSS spectrum (LOG_L3000)</description><unit>1e-07W</unit><ucd>phys.luminosity;spect.continuum;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logL3000</name><description>? Uncertainty on logL3000 (LOG_L3000_ERR)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>q_logL3000</name><description>? Quality flag indicator on logL3000 (QUALITY_L3000) (2)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>logL4400sp</name><description>? Logarithm of the continuum luminosity at 4400 {AA} rest-frame from the SDSS spectrum (LOG_L4400_SPEC)</description><unit>1e-07W</unit><ucd>phys.luminosity;spect.continuum;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logL4400ph</name><description>? Logarithm of the continuum luminosity at 4400 {AA} rest-frame from SDSS photometry (LOG_L4400_PHOT_SDSS)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logL5100</name><description>? Logarithm of the continuum luminosity at 5100 {AA} rest-frame from the SDSS spectrum (LOG_L5100)</description><unit>1e-07W</unit><ucd>phys.luminosity;spect.continuum;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logL5100</name><description>Uncertainty on logL5100 (LOG_L5100_ERR)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>q_logL5100</name><description>? Quality flag indicator on logL5100 (QUALITY_L5100) (3)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FWHMHa</name><description>? Full-width at half-maximum of the broad H{alpha} emission line (FWHM_HA_BR)</description><unit>km/s</unit><ucd>spect.line.width;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FWHMHa</name><description>? Uncertainty on FWHMHa (FWHM_HA_BR_ERR)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>WaveHa</name><description>? Peak wavelength of the broad H {alpha} emission line (PEAK_HA_BR)</description><unit>0.1nm</unit><ucd>em.wl;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_WaveHa</name><description>? Uncertainty on WaveHa (PEAK_HA_BR_ERR)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWHa</name><description>Equivalent width of the broad H {alpha} emission line (EW_HA_BR)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>e_EWHa</name><description>Uncertainty on EWHa (EW_HA_BR_ERR)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>logLHa</name><description>? Logarithm of the luminosity of the broad H {alpha} emission line (LOGL_HA_BR)</description><unit>1e-07W</unit><ucd>phys.luminosity;spect.line;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logLHa</name><description>? Uncertainty on logLHa (LOGL_HA_BR_ERR)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>q_logLHa</name><description>? Quality flag indicator on logLHa (QUALITY_HA) (4)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FWHMHb</name><description>? Full-width at half-maximum of the broad H {bata} emission line (FWHM_HB_BR)</description><unit>km/s</unit><ucd>spect.line.width;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FWHMHb</name><description>? Uncertainty on FWHMHb (FWHM_HB_BR_ERR)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>WaveHb</name><description>? Peak wavelength of the broad H {beta} emission line (PEAK_HB_BR)</description><unit>0.1nm</unit><ucd>em.wl;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_WaveHb</name><description>? Uncertainty on WaveHb (PEAK_HB_BR_ERR)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWHb</name><description>Equivalent width of the broad H{beta} emission line (EW_HB_BR)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>e_EWHb</name><description>Uncertainty on EWHb (EW_HB_BR_ERR)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>logLHb</name><description>? Logarithm of the luminosity of the broad H {beta} emission line (LOGL_HB_BR)</description><unit>1e-07W</unit><ucd>phys.luminosity;spect.line;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logLHb</name><description>? Uncertainty on logLHb (LOGL_HB_BR_ERR)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>q_logLHb</name><description>? Quality flag indicator on logLHb (QUALITY_HB) (5)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FWHMMgII</name><description>? Full-width at half-maximum of the broad Mg II emission line (FWHM_MGII_BR)</description><unit>km/s</unit><ucd>spect.line.width;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FWHMMgII</name><description>? Uncertainty on FWHMmgII (FWHM_MGII_BR_ERR)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>WaveMgII</name><description>? Peak wavelength of the broad Mg II emission line (PEAK_MGII_BR)</description><unit>0.1nm</unit><ucd>em.wl;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_WaveMgII</name><description>? Uncertainty on WavemgII (PEAK_MGII_BR_ERR)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWMgII</name><description>? Equivalent width of the broad Mg II emission line (EW_MGII_BR)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EWMgII</name><description>? Uncertainty on EWmgII (EW_MGII_BR_ERR)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SepMgII</name><description>Flag for modelled MgII region method (MGII_SEP) (9)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TypeLine</name><description>Flag for AGN types 1 broad line as B 595 times and narrow line as N 101 times (LINEWIDTH)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MBH1</name><description>? The BH mass estimate from FWHMHa and logL5100 (MASS_HA_5100_MR16) (10)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH2</name><description>? The BH mass estimate from FWHMHa and logLHa (MASS_HA_HA_MR16) (10)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH3</name><description>? The BH mass estimate from FWHMHb and logL5100 (MASS_HB_5100_MR16) (10)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH4</name><description>? The BH mass estimate from FWHMHb and logLHb (MASS_HB_HB_G10) (11)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH5</name><description>? The BH mass estimate from FWHMmgII and logL3000 (MASS_MGII_3000_MR16) (10)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH6</name><description>? The BH mass estimate from FWHMmgII and logLmgII (MASS_MGII_MGII_W18) (12)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH7</name><description>? The BH mass estimate from FWHMHa and logL5100 using the calibrated relation in section 4 of this work (MASS_HA_5100_K23)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH8</name><description>? The BH mass estimate from FWHMHa and logLHa using the calibrated relation in section 4 of this work (MASS_HA_HA_K23)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH9</name><description>? The BH mass estimate from FWHMHb and logLHb using the calibrated relation in section 4 of this work (MASS_HB_HB_K23)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH10</name><description>? The BH mass estimate from FWHMmgII and logL3000 using the calibrated relation in section 4 of this work (MASS_MGII_3000_K23)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MBH11</name><description>? The BH mass estimate from FWHMmgII and logLmgII using the calibrated relation in section 4 of this work (MASS_MGII_MGII_K23)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>QHa5100</name><description>? Quality flag for MBH1 and MBH7 (Q_MASS_HA_5100) (13)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>QHB5100</name><description>? Quality flag for MBH3 and MBH (Q_MASS_HB_5100) (14)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>QMgII3000</name><description>? Quality flag for MBH5 and MBH10 (Q_MASS_MGII_3000) (15)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MBH</name><description>Logarithm of our preferred BH mass estimate (LOG_MASS_PREF_VALUE)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_MBH</name><description>Flag for which BH mass estimate is the preferred one (LOG_MASS_PREF_SOURCE) (7)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>ObsID</name><description>The XMM-Newton obsID for the X-ray and OM photometric data from 4XMM-DR9 of Webb et al. 2020A&amp;A...641A.136W, Cat. IX/59 (XMM_OBSID)</description><ucd>meta.id.assoc</ucd></column><column><name>Source</name><description>The unique X-ray source number taken from the 4XMM-DR9 of Webb et al. 2020A&amp;A...641A.136W, Cat. IX/59 (XMM_SRCID)</description><ucd>meta.id.assoc</ucd></column><column><name>logL2keV</name><description>Logarithm of monochromatic X-ray L{nu}_2keV_ flux at rest-frame 2 keV estimated from the XMM-Newton band fluxes as seen in sect 3.2 (LOG_L2KEV)</description><unit>1e-07W.Hz**-1</unit><ucd>phys.luminosity;em.X-ray.soft</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL2keV</name><description>Uncertainty on logL2keV (LOG_L2KEV_ERR)</description><unit>1e-07W.Hz**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>GammaX</name><description>Estimated X-ray photon index as seen in section 3.2 (GAMMA_X)</description><ucd>spect.index;em.X-ray.soft</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_GammaX</name><description>Uncertainty on GammaX (GAMMA_X_ERR)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>alphaOX</name><description>? Optical-X-ray energy index (ALPHA_OX) (16)</description><ucd>spect.index;arith.ratio;em.X-ray.soft</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_alphaOX</name><description>? Uncertainty on alphaOX (ALPHA_OX_ERR)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_alphaOX</name><description>The L2500 column measurement used to calculate UV/X-ray energy index {alpha}_ox_ (LOG_L2500_ALPHA_OX)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>n_RL</name><description>The L4400 column measurement used to calculate RL radio loudness energy index (LOG_L4400_R_LOUD)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Balmer</name><description>Flag for Balmer lines as K23 for this work 60 times and as R20 636 times for Rakshit et al. 2020ApJS..249...17R, Cat. J/ApJS/249/17 (BALMER_SOURCE)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>MgII</name><description>Flag for Mg II as K23 for this work 100 times and as R20 596 times for Rakshit et al. 2020ApJS..249...17R, Cat. J/ApJS/249/17 (MGII_SOURCE)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table></schema></tableset></ri:Resource>