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<ri:Resource created="2023-06-13T06:49:59Z" 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>Stellar properties in SFRs from SDSS APOGEE-2</title><shortName>J/AJ/165/51</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/51</identifier><altIdentifier>doi:10.26093/cds/vizier.51650051</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Roman-Zuniga C.G.</name></creator><creator><name>Kounkel M.</name></creator><creator><name>Hernandez J.</name></creator><creator><name>Ramirez K.P.,Lopez-Valdivia R.</name></creator><creator><name>Covey K.R.</name></creator><creator><name>Stutz A.M.</name></creator><creator><name>Roman-Lopes A.</name></creator><creator><name>Campbell H.,Khilfeh E.</name></creator><creator><name>Tapia M.</name></creator><creator><name>Stringfellow G.S.</name></creator><creator><name>Downes J.J.</name></creator><creator><name>Stassun K.G.,Minniti D.</name></creator><creator><name>Bayo A.</name></creator><creator><name>Kim J.S.</name></creator><creator><name>Suarez G.</name></creator><creator><name>Ybarra J.E.,Fernandez-Trincado J.G.</name></creator><creator><name>Longa-Pena P.</name></creator><creator><name>Ramirez-Preciado V.</name></creator><creator><name>Serna J.,Lane R.R.</name></creator><creator><name>Garcia-Hernandez D.A.</name></creator><creator><name>Beaton R.L.</name></creator><creator><name>Bizyaev D.</name></creator><creator><name>Pan K.</name></creator><date role="Updated">2024-10-07T15:33:00Z</date><date role="Created">2023-06-13T06:49:59Z</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>star-forming-regions</subject><subject>pre-main-sequence-stars</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><subject>infrared-photometry</subject><subject>extinction</subject><description>The Sloan Digital Sky Survey IV APOGEE-2 primary science goal was to observe red giant stars throughout the Galaxy to study its dynamics, morphology, and chemical evolution. The APOGEE instrument, a high-resolution 300-fiber H-band (1.55-1.71{mu}m) spectrograph, is also ideal to study other stellar populations in the Galaxy, among which are a number of star-forming regions and young open clusters. We present the results of the determination of six stellar properties (Teff, logg, [Fe/H], L/L{sun}, M/M{sun}, and age) for a sample that is composed of 3360 young stars, of subsolar to supersolar types, in 16 Galactic star formation and young open cluster regions. Those sources were selected by using a clustering method that removes most of the field contamination. Samples were also refined by removing targets affected by various systematic effects of the parameter determination. The final samples are presented in a comprehensive catalog that includes all six estimated parameters. This overview study also includes parameter spatial distribution maps for all regions and Hertzsprung-Russell (log(L/L{sun} vs. Teff) diagrams. This study serves as a guide for detailed studies on individual regions and paves the way for the future studies on the global properties of stars in the pre-main-sequence phase of stellar evolution using more robust samples.</description><source format="bibcode">2023AJ....165...51R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/51</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/B/simbad">B/simbad : Simbad objects catalogue (M.Wenger 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/2124">J/AJ/121/2124 : {lambda} Ori pre-main-sequence stars photometry (Dolan+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/387">J/AJ/123/387 : VRI photometry of {lambda}Ori SFR (Dolan+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/397/177">J/A+A/397/177 : IR star clusters and stellar groups catalog (Bica+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1916">J/AJ/126/1916 : JHK photometry of young clusters near the Sun (Porras+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A109">J/A+A/533/A109 : Pisa pre-main sequence tracks and isochrones (Tognelli+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A29">J/A+A/557/A29 : Young stellar clusters in the Rosette (Cambresy+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/125">J/ApJ/794/125 : IN-SYNC. 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