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<ri:Resource created="2015-12-14T13:31:26Z" 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 abundances</title><shortName>J/ApJ/808/16</shortName><identifier>ivo://CDS.VizieR/J/ApJ/808/16</identifier><altIdentifier>doi:10.26093/cds/vizier.18080016</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>Ho A.Y.Q.</name></creator><creator><name>Zasowski G.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2015-12-14T13:31:26Z</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>metallicity</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>New spectroscopic surveys offer the promise of stellar parameters and abundances ("stellar labels") for hundreds of thousands of stars; this poses a formidable spectral modeling challenge. In many cases, there is a subset of reference objects for which the stellar labels are known with high(er) fidelity. We take advantage of this with The Cannon, a new data-driven approach for determining stellar labels from spectroscopic data. The Cannon learns from the "known" labels of reference stars how the continuum-normalized spectra depend on these labels by fitting a flexible model at each wavelength; then, The Cannon uses this model to derive labels for the remaining survey stars. We illustrate The Cannon by training the model on only 542 stars in 19 clusters as reference objects, with Teff, logg, and [Fe/H] as the labels, and then applying it to the spectra of 55000 stars from APOGEE DR10. The Cannon is very accurate. Its stellar labels compare well to the stars for which APOGEE pipeline (ASPCAP) labels are provided in DR10, with rms differences that are basically identical to the stated ASPCAP uncertainties. Beyond the reference labels, The Cannon makes no use of stellar models nor any line-list, but needs a set of reference objects that span label-space. The Cannon performs well at lower signal-to-noise, as it delivers comparably good labels even at one-ninth the APOGEE observing time. We discuss the limitations of The Cannon and its future potential, particularly, to bring different spectroscopic surveys onto a consistent scale of stellar labels.</description><source format="bibcode">2015ApJ...808...16N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/808/16</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/III/272">III/272 : RAVE 4th data release (Kordopatis+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/125">J/ApJ/794/125 : IN-SYNC. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AP</name><description>? Apoge version (4412 or 4413)</description><ucd>meta.software</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ID</name><description>Steller identifier (1) \linkRole{2MASS data for this object or within 1" if not 2MASS name}</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>Teff</name><description>[3140/5722] 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>[1/285] The 1{sigma} uncertainty in Teff</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>[-1.4/5.2] 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>[0.003/0.6] The 1{sigma} uncertainty in log(g)</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>[-3/3.4] Metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>[0.001/0.4] The 1{sigma} uncertainty in [Fe/H]</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>[0.01/810] The {chi}^2^ value</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vscat</name><description>[0/522068] Velocity scatter</description><unit>km/s</unit><ucd>stat.error;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TFlag</name><description>The APOGEE_TARGET2 flag \pFile{_640x300}{J/ApJ/808/16/flags_t2.htx}{Binary flag}; see text for more explanations</description><ucd>meta.code</ucd></column><column><name>AFlag</name><description>The APOGEE_ASPCAPFLAG flag (2) \pFile{_640x300}{J/ApJ/808/16/flags.htx}{Binary flag}; see text for more explanations</description><ucd>meta.code</ucd></column><column><name>CFlag</name><description>[CS] Commissioning flag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Dref</name><description>[0.002/1] Distance between test star and nearest reference object (4)</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EFlag</name><description>[0/1] Extrapolation flag (5)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M13</name><description>Sources within 0.5" from Meszaros, 2013, J/AJ/146/133</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Positions from IDs (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 IDs (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column></table></schema></tableset></ri:Resource>