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<ri:Resource created="2015-07-18T13:37:18Z" 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>Abundances from SEGUE Stellar Parameters Pipeline</title><shortName>J/ApJ/798/122</shortName><identifier>ivo://CDS.VizieR/J/ApJ/798/122</identifier><altIdentifier>doi:10.26093/cds/vizier.17980122</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Miller A.A.</name></creator><creator><name>Bloom J.S.</name></creator><creator><name>Richards J.W.</name></creator><creator><name>Lee Y.S.</name></creator><creator><name>Starr D.L.</name></creator><creator><name>Butler N.R.,Tokarz S.</name></creator><creator><name>Smith N.</name></creator><creator><name>Eisner J.A.</name></creator><date role="Updated">2015-07-18T13:52:09Z</date><date role="Created">2015-07-18T13:37:18Z</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>variable-stars</subject><subject>metallicity</subject><subject>effective-temperature</subject><subject>surveys</subject><description>A fundamental challenge for wide-field imaging surveys is obtaining follow-up spectroscopic observations: there are &gt;10^9^ photometrically cataloged sources, yet modern spectroscopic surveys are limited to ~fewx10^6^ targets. As we approach the Large Synoptic Survey Telescope era, new algorithmic solutions are required to cope with the data deluge. Here we report the development of a machine-learning framework capable of inferring fundamental stellar parameters (T_eff_, logg, and [Fe/H]) using photometric-brightness variations and color alone. A training set is constructed from a systematic spectroscopic survey of variables with Hectospec/Multi-Mirror Telescope. In sum, the training set includes ~9000 spectra, for which stellar parameters are measured using the SEGUE Stellar Parameters Pipeline (SSPP). We employed the random forest algorithm to perform a non-parametric regression that predicts T_eff_, logg, and [Fe/H] from photometric time-domain observations. Our final optimized model produces a cross-validated rms error (RMSE) of 165K, 0.39dex, and 0.33dex for T_eff_, logg, and [Fe/H], respectively. Examining the subset of sources for which the SSPP measurements are most reliable, the RMSE reduces to 125K, 0.37dex, and 0.27dex, respectively, comparable to what is achievable via low-resolution spectroscopy. For variable stars this represents a {approx}12%-20% improvement in RMSE relative to models trained with single-epoch photometric colors. As an application of our method, we estimate stellar parameters for ~54000 known variables. We argue that this method may convert photometric time-domain surveys into pseudo-spectrographic engines, enabling the construction of extremely detailed maps of the Milky Way, its structure, and history.</description><source format="bibcode">2015ApJ...798..122M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/798/122</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/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><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/J/AJ/145/13">J/AJ/145/13 : Metal-poor stars from SDSS/SEGUE. I. Abundances (Aoki+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/203/32">J/ApJS/203/32 : Machine-learned ASAS Classif. Cat. (MACC) (Richards+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/112">J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/2602">J/MNRAS/414/2602 : Automated classification of HIP variables (Dubath+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/90">J/AJ/141/90 : SEGUE stellar parameter pipeline. V. (Lee+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/26">J/ApJ/728/26 : QSO selection based on photom. variability (Macleod+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/494/739">J/A+A/494/739 : Automatic classification of OGLE variables (Sarro+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/973">J/AJ/134/973 : SDSS Stripe 82 star catalogs (Ivezic+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/466">J/AJ/138/466 : NSVS variables automated classification (Hoffman+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2070">J/AJ/136/2070 : SEGUE stellar parameter pipeline. III. (Allende Prieto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2050">J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. 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