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<ri:Resource created="2022-09-09T09:47:57Z" 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>SEGUE-2 updated stellar parameter pipeline</title><shortName>J/ApJS/259/60</shortName><identifier>ivo://CDS.VizieR/J/ApJS/259/60</identifier><altIdentifier>doi:10.26093/cds/vizier.22590060</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rockosi C.M.</name></creator><creator><name>Sun Lee Y.</name></creator><creator><name>Morrison H.L.</name></creator><creator><name>Yanny B.</name></creator><creator><name>Johnson J.A.,Lucatello S.</name></creator><creator><name>Sobeck J.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Allende Prieto C.</name></creator><creator><name>An D.</name></creator><creator><name>Bizyaev D.,Blanton M.R.</name></creator><creator><name>Casagrande L.</name></creator><creator><name>Eisenstein D.J.</name></creator><creator><name>Gould A.</name></creator><creator><name>Gunn J.E.,Harding P.</name></creator><creator><name>Ivans I.I.</name></creator><creator><name>Jacobson H.R.</name></creator><creator><name>Janesh W.</name></creator><creator><name>Knapp G.R.,Kollmeier J.A.</name></creator><creator><name>Lepine S.</name></creator><creator><name>Lopez-Corredoira M.</name></creator><creator><name>Ma Z.</name></creator><creator><name>Newberg H.J.,Pan K.</name></creator><creator><name>Prchlik J.</name></creator><creator><name>Sayers C.</name></creator><creator><name>Schlesinger K.J.</name></creator><creator><name>Simmerer J.</name></creator><creator><name>Weinberg D.H.</name></creator><date role="Updated">2022-09-30T23:22:04Z</date><date role="Created">2022-09-09T09:47:57Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>metallicity</subject><subject>radial-velocity</subject><subject>globular-star-clusters</subject><subject>surveys</subject><subject>milky-way-galaxy</subject><description>The Sloan Extension for Galactic Understanding and Exploration 2 (SEGUE-2) obtained 128,288 low-resolution spectra (R~1800) of 118,958 unique stars in the first year of the Sloan Digital Sky Survey-III (2008-2009). SEGUE-2 targeted prioritized distant halo tracers (blue horizontal-branch stars, K giants, and M giants) and metal-poor or kinematically hot populations. The main goal of SEGUE-2 was to target stars in the distant halo and measure their kinematics and chemical abundances to learn about the formation and evolution of the Milky Way. We present the SEGUE-2 field placement and target selection strategies. We discuss the success rate of the targeting based on the SEGUE-2 spectra and other spectroscopic and astrometric surveys. We describe the final SEGUE-2/SDSS-III improvements to the stellar parameter determinations based on the SEGUE Stellar Parameter Pipeline. We report a (g-i) color-effective temperature relation calibrated to the IRFM. We evaluate the accuracy and uncertainties associated with these stellar parameters by comparing with fundamental parameters, a sample of high-resolution spectra of SEGUE stars analyzed homogeneously, stars in well-studied clusters, and stars observed in common by the APOGEE survey. The final SEGUE spectra, calibration data, and derived parameters described here were released in SDSS-III Data Release 9 and continue to be included in all subsequent SDSS Data Releases. Because of its faint limiting magnitude and emphasis on the distant halo, the public SEGUE-2 data remain an important resource for the spectroscopy of stars in the Milky Way.</description><source format="bibcode">2022ApJS..259...60R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/259/60</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/53/791">J/ApJS/53/791 : Spectroscopy of AB stars in halo (Pier, 1983)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/90/2089">J/AJ/90/2089 : Stars of very low metal abundance. 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