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<ri:Resource created="2022-03-31T14:31:03Z" 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 parameters of LAMOST stars using SLAM</title><shortName>J/ApJS/246/9</shortName><identifier>ivo://CDS.VizieR/J/ApJS/246/9</identifier><altIdentifier>doi:10.26093/cds/vizier.22460009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang Bo</name></creator><creator><name>Liu C.</name></creator><creator><name>Deng L.-C.</name></creator><date role="Updated">2022-10-26T11:12:42Z</date><date role="Created">2022-03-31T14:31:03Z</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>chemical-abundances</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>astronomical-models</subject><subject>giant-stars</subject><subject>surveys</subject><description>The LAMOST survey has provided 9 million spectra in its Data Release 5 (DR5) at R~1800. Extracting precise stellar labels is crucial for such a large sample. In this paper, we report the implementation of the Stellar LAbel Machine (SLAM), which is a data-driven method based on support vector regression (SVR), a robust nonlinear regression technique. Thanks to the capability to model highly nonlinear problems with SVR, SLAM can generally derive stellar labels over a wide range of spectral types. This gives it a unique capability compared to other popular data-driven methods. To illustrate this capability, we test the performance of SLAM on stars ranging from Teff~4000 to ~8000K trained on LAMOST spectra and stellar labels. At g-band signal-to-noise ratio (S/Ng) higher than 100, the random uncertainties of Teff, logg, and [Fe/H] are 50K, 0.09dex, and 0.07dex, respectively. We then set up another SLAM model trained by APOGEE and LAMOST common stars to demonstrate its capability of dealing with high dimensional problems. The spectra are from LAMOST DR5 and the stellar labels of the training set are from APOGEE DR15, including Teff, logg, [M/H], [{alpha}/M], [C/M], and [N/M]. The cross-validated scatters at S/N_g_~100 are 49K, 0.10dex, 0.037dex, 0.026dex, 0.058dex, and 0.106dex for these parameters, respectively. This performance is at the same level as other up-to-date data-driven models.</description><source format="bibcode">2020ApJS..246....9Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/246/9</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/153">V/153 : LAMOST DR4 catalogs (Luo+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/11.924">J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/808/16">J/ApJ/808/16 : Cannon: a new approach to determine abundances (Ness+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for APOGEE chemical elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/836/5">J/ApJ/836/5 : Abundances of LAMOST giants from APOGEE DR12 (Ho+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/478/4513">J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/241/32">J/ApJS/241/32 : OB stars from the LAMOST DR5 spectra (Liu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/8">J/ApJS/244/8 : M-type stars in LAMOST DR5 (Zhong+, 2019)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS home 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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>ObsID</name><description>[101008/585216248]? LAMOST identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>RAJ2000</name><description>Right ascension (J2000) (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (J2000) (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>snrg</name><description>[0/998]? g-band signal-to-noise ratio of the spectra</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Teff</name><description>[-7492/15227] SLAM-predicted effective temperature (teff_slam)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>indexed</flag></column><column><name>e_Teff</name><description>[38.8/241.3] Teff uncertainty (teff_err_slam)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg</name><description>[-41.7/31.3] SLAM-predicted log of surface gravity (logg_slam)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>[0.06/0.7] logg uncertainty (logg_err_slam)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[M/H]</name><description>[-21.6/12] SLAM-predicted metallicity (mh_slam)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[M/H]</name><description>[0.02/0.5] Uncertainty in [M/H] (mh_err_slam)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[a/M]</name><description>[-4.2/7.1] SLAM-predicted [{alpha}/M] (am_slam)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[a/M]</name><description>[0.01/0.2] Uncertainty in [a/M] (am_err_slam)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[C/M]</name><description>[-9/7.5] SLAM-predicted [C/M] (cm_slam)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[C/M]</name><description>[0.04/0.2] Uncertainty in [C/M] (cm_err_slam)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[N/M]</name><description>[-9.5/15.5] SLAM-predicted [N/M] (nm_slam)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[N/M]</name><description>[0.07/0.3] Uncertainty in [N/M] (nm_err_slam)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>O-C</name><description>[0.005/243963] rms deviation between the observed and fitted spectra (rmseppix_slam)</description><ucd>stat.stdev;instr.det.noise;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>K</name><description>[0/1] K giant star selected (1=yes) (ind_kgiant)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>D</name><description>[0.0005/16038]? Distance D (DHo17) (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Fl</name><description>[0/1] APOGEE observation flag (1:observed by APOGEE) (ind_common)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sloan</name><description>Display the online SDSS-DR16 data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>