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<ri:Resource created="2025-02-04T13:22:59Z" status="active" updated="2025-07-18T20:15:24Z" 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>Elemental abundances from DESI EDR spectra</title><shortName>J/ApJS/273/19</shortName><identifier>ivo://CDS.VizieR/J/ApJS/273/19</identifier><altIdentifier>doi:10.26093/cds/vizier.22730019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang M.</name></creator><creator><name>Xiang M.</name></creator><creator><name>Ting Y.-S.</name></creator><creator><name>Wang J.</name></creator><creator><name>Li H.</name></creator><creator><name>Zou Hu</name></creator><creator><name>Nie J.</name></creator><creator><name>Mou L.,Wu T.</name></creator><creator><name>Wu Y.</name></creator><creator><name>Liu J.</name></creator><date role="Updated">2025-07-18T20:15:24Z</date><date role="Created">2025-02-04T13:22:59Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><subject>surveys</subject><subject>milky-way-galaxy</subject><description>Stellar abundances for a large number of stars provide key information for the study of Galactic formation history. Large spectroscopic surveys such as the Dark Energy Spectroscopic Instrument (DESI) and LAMOST take median-to-low-resolution (R&lt;~5000) spectra in the full optical wavelength range for millions of stars. However, the line-blending effect in these spectra causes great challenges for elemental abundance determination. Here we employ DD-Payne, a data-driven method regularized by differential spectra from stellar physical models, to the DESI early data release spectra for stellar abundance determination. Our implementation delivers 15 labels, including effective temperature Teff, surface gravity logg, microturbulence velocity v_mic_, and the abundances for 12 individual elements, namely C, N, O, Mg, Al, Si, Ca, Ti, Cr, Mn, Fe, and Ni. Given a spectral signal-to-noise ratio of 100 per pixel, the internal precisions of the label estimates are about 20K for Teff, 0.05dex for logg, and 0.05dex for most elemental abundances. These results agree with the theoretical limits from the Cramer-Rao bound calculation within a factor of 2. The majority of the accreted halo stars contributed by the Gaia-Enceladus-Sausage are discernible from the disk and in situ halo populations in the resultant [Mg/Fe]-[Fe/H] and [Al/Fe]-[Fe/H] abundance spaces. We also provide distance and orbital parameters for the sample stars, which spread over a distance out to ~100kpc. The DESI sample has a significantly higher fraction of distant (or metal- poor) stars than the other existing spectroscopic surveys, making it a powerful data set for studying the Galactic outskirts.</description><source format="bibcode">2024ApJS..273...19Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/273/19</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/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/286">III/286 : APOGEE-2 DR17 final allStar catalog (Abdurro'uf+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/292">VII/292 : DESI Legacy Imaging Surveys DR8 photometric redshifts (Duncan, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/497/497">J/A+A/497/497 : Physical param. from JHK flux (Gonzalez-Hernandez+, 2009)</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/ApJ/836/5">J/ApJ/836/5 : Abundances of LAMOST giants from APOGEE DR12 (Ho+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/245/34">J/ApJS/245/34 : Abund. for 6 million stars from LAMOST DR5 (Xiang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/493/5195">J/MNRAS/493/5195 : Milky Way halo stars ages and kinematics (Das+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/891/23">J/ApJ/891/23 : Stellar abundances from LAMOST MRS (SPCAnet) (Wang+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/246/9">J/ApJS/246/9 : Stellar parameters of LAMOST stars using SLAM (Zhang+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/NatAs/5.640">J/other/NatAs/5.640 : Chronologically dating early assembly (Montalban+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/649/A3">J/A+A/649/A3 : Gaia EDR3 photometric passbands (Riello+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/253/22">J/ApJS/253/22 : Ks abs. magnitudes from LAMOST for OB stars (Xiang+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/513/1557">J/MNRAS/513/1557 : Accreted halo stars abundances (Carrillo+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/931/147">J/ApJ/931/147 : Very metal-poor stars with LAMOST &amp; Subaru. 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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>RAJ2000</name><description>Target right ascension (J2000) (TARGET_RA)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>[-31.6/85] Target declination (J2000) (TARGET_DEC)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>ID</name><description>DESI target identifier (TARGET_ID)</description><ucd>meta.id;meta.main</ucd></column><column><name>Survey</name><description>Name of the DESI survey (SURVEY)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Prog</name><description>Name of the program (PROGRAM)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Prim</name><description>[FT] Primary, false or true (PRIMARY)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Hpix</name><description>[683/45007] Healpix ID (HEALPIX)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>snrB</name><description>[-6.3/473.2] Median spectral signal-to-noise ratio in B-band (SNRB)</description><ucd>stat.snr;stat.median;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>snrG</name><description>[-0.3/608] Median spectral signal-to-noise ratio in G-band (SNRG)</description><ucd>stat.snr;stat.median;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>snrR</name><description>[0.2/771] Median spectral signal-to-noise ratio in R-band (SNRR)</description><ucd>stat.snr;stat.median;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV</name><description>[-1500/1500] Radial velocity from DESI EDR catalog (RV)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RV</name><description>[0.0001/2341] RV uncertainty (RV_ERR)</description><unit>km/s</unit><ucd>stat.error;phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Teff</name><description>[2642/8863]? 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Iron abundance (FEH)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]</name><description>[0.007/1.4]? [Fe/H] Uncertainty (FEH_ERR)</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[C/Fe]</name><description>[-1.4/2.1]? Log of C/Fe abundance (C_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[C/Fe]</name><description>[0.004/1.8]? [C/Fe] Uncertainty (C_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[N/Fe]</name><description>[-1.9/2.2]? Log of N/Fe abundance (N_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[N/Fe]</name><description>[0.009/3]? [N/Fe] Uncertainty (N_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Mg/Fe]</name><description>[-0.8/1.4]? Log of Mg/Fe abundance (MG_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Mg/Fe]</name><description>[0.005/3]? [Mg/Fe] Uncertainty (MG_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[O/Fe]</name><description>[-0.8/1.6]? Log of O/Fe abundance (O_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[O/Fe]</name><description>[0.006/2]? [O/Fe] Uncertainty (O_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Al/Fe]</name><description>[-1.3/1.5]? Log of Al/Fe abundance (AL_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Al/Fe]</name><description>[0.01/2.5]? [Al/Fe] Uncertainty (AL_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/Fe]</name><description>[-0.9/1.4]? Log of Si/Fe abundance (SI_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Si/Fe]</name><description>[0.007/2.1]? [Si/Fe] Uncertainty (SI_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]</name><description>[-0.9/1.4]? Log of Ca/Fe abundance (CA_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Ca/Fe]</name><description>[0.006/2]? [Ca/Fe] Uncertainty (CA_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ti/Fe]</name><description>[-1.2/1.5]? Log of Ti/Fe abundance (TI_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Ti/Fe]</name><description>[0.006/1.5]? [Ti/Fe] Uncertainty (TI_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Cr/Fe]</name><description>[-1.9/1]? Log of Cr/Fe abundance (CR_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Cr/Fe]</name><description>[0.009/3.6]? [Cr/Fe] Uncertainty (CR_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Mn/Fe]</name><description>[-1.4/0.9]? Log of Mn/Fe abundance (MN_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Mn/Fe]</name><description>[0.008/3.2]? [Mn/Fe] Uncertainty (MN_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ni/Fe]</name><description>[-0.9/1.1]? Log of Ni/Fe abundance (NI_FE)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Ni/Fe]</name><description>[0.008/3.1]? [Ni/Fe] Uncertainty (NI_FE_ERR)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vmic</name><description>[-0.63/3.13]? Microturbulent velocity (VMIC)</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Vmic</name><description>[0.009/3.4]? Vmic uncertainty (VMIC_ERR)</description><unit>km/s</unit><ucd>stat.error;phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CorTeff-logg</name><description>[-1/0.87] The correlation coefficients between Teff and logg (COR_TEFF_LOGG)</description><ucd>stat.correlation;phys.temperature.effective;phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CorTeff-feh</name><description>[-1/0.81] The correlation coefficients between Teff and [Fe/H] (COR_TEFF_FEH)</description><ucd>stat.correlation;phys.temperature.effective;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Corlogg-feh</name><description>[-1/0.72] The correlation coefficients between logg and [Fe/H] (COR_LOGG_FEH)</description><ucd>stat.correlation;phys.gravity;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>q_Chi2</name><description>[-3.2/3.9e+6]? A quality flag describing the {chi}^2^ of the spectral fit (CHISQ_FLAG)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Chi2</name><description>[0.009/773000]? The {chi}^2^ of the spectral fit (CHISQ)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>VR</name></column></table></schema></tableset></ri:Resource>