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<ri:Resource created="2016-09-22T13:13:14Z" 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>The Cannon: a new approach to determine masses</title><shortName>J/ApJ/823/114</shortName><identifier>ivo://CDS.VizieR/J/ApJ/823/114</identifier><altIdentifier>doi:10.26093/cds/vizier.18230114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ness M.</name></creator><creator><name>Hogg D.W.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Martig M.</name></creator><creator><name>Pinsonneault M.H.</name></creator><creator><name>Ho A.Y.Q.</name></creator><date role="Updated">2018-10-12T12:35:34Z</date><date role="Created">2016-09-22T13:13:14Z</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>giant-stars</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>chemical-abundances</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>The mass of a star is arguably its most fundamental parameter. For red giant stars, tracers luminous enough to be observed across the Galaxy, mass implies a stellar evolution age. It has proven to be extremely difficult to infer ages and masses directly from red giant spectra using existing methods. From the Kepler and APOGEE surveys, samples of several thousand stars exist with high-quality spectra and asteroseismic masses. Here we show that from these data we can build a data-driven spectral model using The Cannon, which can determine stellar masses to ~0.07dex from APOGEE DR12 spectra of red giants; these imply age estimates accurate to ~0.2dex (40%). We show that The Cannon constrains these ages foremost from spectral regions with CN absorption lines, elements whose surface abundances reflect mass-dependent dredge-up. We deliver an unprecedented catalog of 70000 giants (including 20000 red clump stars) with mass and age estimates, spanning the entire disk (from the Galactic center to R~20kpc). We show that the age information in the spectra is not simply a corollary of the birth-material abundances [Fe/H] and [{alpha}/Fe], and that, even within a monoabundance population of stars, there are age variations that vary sensibly with Galactic position. Such stellar age constraints across the Milky Way open up new avenues in Galactic archeology.</description><source format="bibcode">2016ApJ...823..114N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/823/114</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/ApJ/819/2">J/ApJ/819/2 : APOGEE kinematics. I. Galactic bulge overview (Ness+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/221/24">J/ApJS/221/24 : SDSS-III APOGEE H-band spectral line lists (Shetrone+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/2127">J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/808/16">J/ApJ/808/16 : The Cannon: new approach to determine abundances (Ness+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/577/A9">J/A+A/577/A9 : Sc, V, Mn, and Co in Milky Way stars (Battistini+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/19">J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/125">J/ApJ/794/125 : IN-SYNC. I. APOGEE stellar parameters (Cottaar+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/133">J/AJ/146/133 : Stellar parameters from SDSS-III APOGEE DR10 (Meszaros+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A147">J/A+A/549/A147 : Abundances of microlensed Bulge dwarf stars V. (Bensby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A138">J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)</relatedResource><relatedResource>http://www.sdss3.org/ : SDSS-III home page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/823/114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/823/114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/823/114</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/823/114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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44966 44967 44968 44969 44971 44986 45008 45009 45011 45020 45021 48982 48983 48985 48987 49013 49015</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/823/114?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/823/114/table1</name><description>Stellar parameters, masses and ages as determined by The Cannon for APOGEE giants</description><column><name>Type</name><description>Red giant type (1)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2MASS</name><description>2MASS identifier (HHMMSSss+DDMMSSs; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Teff</name><description>[4054/5120] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Teff</name><description>[0.7/73] Uncertainty in Teff (6)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(g)</name><description>[1.3/3.4] log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(g)</name><description>[0.004/0.2] Uncertainty in log(g) (6)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-0.9/0.4] log Fe/H number abundance (2)</description><unit>log(Sun)</unit><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>[0.001/0.06] Uncertainty in [Fe/H] (6)</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[a/Fe]</name><description>[-0.03/0.3] log {alpha}/Fe number abundance (2)</description><unit>log(Sun)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[a/Fe]</name><description>[0.001/0.03] Uncertainty in [a/Fe] (6)</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>lnM</name><description>[-1.1/1.9] ln stellar mass (3)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_lnM</name><description>[0.006/0.3] Uncertainty in lnM (6)</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>lnAge</name><description>[-2.8/5.3] ln stellar age (4)</description><unit>log(Gyr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_lnAge</name><description>[0.01/0.6] Uncertainty in lnAge (6)</description><unit>log(Gyr)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>chi2</name><description>[0.1/24.3] The {chi}^2^ statistic (5)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rgal</name><description>[-13.25/21.77] Galactocentric radius</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from 2MASS names (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>_DE</name><description>Positions from 2MASS names (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column></table></schema></tableset></ri:Resource>