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<ri:Resource created="2021-09-02T15:25:52Z" 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 abundances from LAMOST MRS (SPCAnet)</title><shortName>J/ApJ/891/23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/891/23</identifier><altIdentifier>doi:10.26093/cds/vizier.18910023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang R.</name></creator><creator><name>Luo A.-L.</name></creator><creator><name>Chen J.-J.</name></creator><creator><name>Hou W.</name></creator><creator><name>Zhang S.</name></creator><creator><name>Zhao Y.-H.</name></creator><creator><name>Li X.-R.,Hou Y.-H.</name></creator><date role="Updated">2022-07-19T08:10:07Z</date><date role="Created">2021-09-02T15:25:52Z</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>effective-temperature</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>surveys</subject><description>The fundamental stellar atmospheric parameters (Teff and logg) and 13 chemical abundances are derived for medium-resolution spectroscopy from Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Medium Resolution Survey (MRS) data sets with a deep-learning method. The neural networks we designed, named SPCANet, precisely map LAMOST MRS spectra to stellar parameters and chemical abundances. The stellar labels derived by SPCANet have precisions of 119K for Teff and 0.17dex for logg. The abundance precision of 11 elements including [C/H], [N/H], [O/H], [Mg/H], [Al/H], [Si/H], [S/H], [Ca/H], [Ti/H], [Cr/H], [Fe/H], and [Ni/H] are 0.06 {\sim} 0.12 dex, while that of [Cu/H] is 0.19dex. These precisions can be reached even for spectra with signal-to-noise ratios as low as 10. The results of SPCANet are consistent with those from other surveys such as APOGEE, GALAH, and RAVE, and are also validated with the previous literature values including clusters and field stars.</description><source format="bibcode">2020ApJ...891...23W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/891/23</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/279">III/279 : RAVE 5th data release (Kunder+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/153">V/153 : LAMOST DR4 catalogs (Luo+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4377">J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/193">J/AJ/142/193 : RAVE stellar elemental abundances (DR1) (Boeche+, 2011)</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/A+A/562/A71">J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)</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/A+A/573/A55">J/A+A/573/A55 : Gaia-ESO Survey: Tr20, NGC 4815 &amp; 6705 (Tautvaisiene+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for 15 APOGEE elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/49">J/AJ/151/49 : M6 open cluster: star members (Kilicoglu+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/225">J/ApJ/833/225 : -2.6&lt;=[Fe/H]&lt;=0.2 F &amp; G dwarfs. 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(Zhao+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/603/A2">J/A+A/603/A2 : Gaia-ESO Survey abund. radial distribution (Magrini+, 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/AJ/156/142">J/AJ/156/142 : Cluster abund. for APOGEE using SDSS DR14 (Donor+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/126">J/AJ/156/126 : Stellar abundances from BACCHUS analysis (Jonsson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/628/A54">J/A+A/628/A54 : Fe, Mg, Ti in Galactic clusters (Kovalev+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/622/A191">J/A+A/622/A191 : 885 globular cluster giants abundances (Masseron+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/27">J/ApJS/244/27 : Radial velocity measurements in LAMOST-II 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19320-19321 19323 19409 19412-19413 19464-19465 19467 19492-19493 19504 19509-19511 19556 19558-19559 19590-19591 19593 19595 19602-19603 19612 19614-19615 19629 19636-19637 19640-19641 19652-19654 19733 19735 19765 19780 19782-19783 19788-19790 19808-19809 19812 19978 20006 20012 20014 20096-20097 20363 20365-20367 20378-20379 20385 20387 20396-20397 20399 20404 20408 20475 20478-20479 21351 21353 21355 21362 21372 21374 21391 21395-21396 21398-21399 21413 21415 21433 21436 21441 21443 21448 21450 21452-21453 21460-21462 21468 21472 21859 21862-21863 21878 21961 21976-21978 22009-22011 22086-22087 22089-22091 22102-22103 22121 22123 22140-22141 22170-22171 22174-22175 22181 22183 22189 22209 22211 22218-22219 22236-22238 22256 22258 22282 22304 22331 22334-22335 22352-22353 22355 22361 22364-22365 22367 22375 22381 22383 22440 22442-22443 22448-22449 22464 22466-22467 22469 22488-22489 22491 22496-22498 22516-22517 22803 22806-22807 22809-22811 22841 22844-22845 22853-22856 22858-22859 22870-22871 22884-22885 22887-22888 22900-22902 23106-23107 23110 23122 23136-23137 23139 23148-23149 23152-23154 23418-23419 23422-23423 23459 23462-23465 23467 23474 23480 23482-23483 23485 23487 23492 23494-23495 23500-23501 23503 23521 23523 23540-23542 23548 23550-23551 23569 23572-23573 23616-23617 23620-23621 23623 23661-23663 23676 23678-23679 23725 23729 23731 23747 23788-23789 23796 23800 23859 23865 23867 23910 23916 23918-23919 23930 23939 23945 23947 23969 23981-23983 24070-24071 24101 24106-24107 24112-24113 24115-24118 24128-24130 24219 24222-24223 24228-24230 24266 24321 24323 24329 24356-24357 24363 24365-24367 24416-24418 24420-24421 24429-24431 24433 24436-24437 24444 24446-24447 24449-24451 24476-24478 24480-24481 24483 24489-24491 24512-24514 24540-24542 24552 24554 24567 24573 24575 25703 25716 25718-25719 25797 25799 25820 25822-25823 25853 25896 25898 25984 25986-25987 25990-25991 26036-26038 26040 26042-26043 26157-26159 26172 26174-26175 26189 26193 26195 26224-26225 26227 26237 26253-26255 26285 26300-26302 26310 26316 26318-26319 26340 26388 26390 26392-26394 26400-26402 26491 26494-26495 26595 26599 26603 26605-26606 26608-26609 26612-26614 26618 26973 26975 26979 27029-27031 27037 27039 27104-27105 27116-27117 27119 27132-27134 27142-27143 27145 27147 27154 27164 27166 27169 27171 27180-27181 27188 27190 27192-27193 27196 27241-27243 27252 27254-27255 27285 27287 27293 27352-27354 27361 27364-27365 27405 27407 27412 27414-27415 27426 27429 27432 27434 27449 27451 27457-27460 27462-27463 27474 27486 27508 27510 27516 27518 27520 27522 27540-27541 27581-27583 27596-27597 27604 27606 27608-27609 27623 27634-27635 27638 27649-27651 27664 27666-27667 27775 27784-27785 27788 27893 27946-27947 27950 27971 27973-27975 27980-27981 27986 28021-28023 28025 28027 28064-28065 28068-28069 28079 28083 28086-28087 28115 28133-28135 28375 28381 28383 28405 28421 28423 28440-28441 28443 28459 28462 28513 28516-28517 28537 28540 28560 28562 28568 28570 28575 28580-28582 28592 28597-28599 28604-28605 28607 28629-28631 28634 28656 28658 28660-28661 30022-30023 30034-30035 30038 30064-30065 30068 30209-30211 30226 30252-30253 30264 30837 30839 30845 30847 30933 31012 31014-31015 31032 31034 31095 31101 31103 31120 31274 31369-31370 31398-31399 31401 31403 31410-31411 31420 31422 31681-31683 31698 31712-31713 31715 31724-31725 31736 31794 31888-31890 31927 31970-31971 31974 32177 32179 32250 32276-32277 32279 32285 32328-32329 32332-32333 32351 32373-32375 32413 32415 32437 32439 32450-32451 32454-32455 32468-32469 32471 32488-32489 32492-32493 32529 32531 32538 32541 32560-32562 32568 32570 32600-32601 32609 32612-32613 32644-32646 32648 32650-32651 32671 32680-32682 32687 32691 32714-32715 32718 32748-32750 44921-44923 45016-45017 45019 49142-49143</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/891/23?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/891/23/catalog</name><description>LAMOST MRS Stellar Parameters and Chemical Abundances catalog</description><column><name>Qual</name><description>Quality flag: 1=good, 0=bad</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</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>Nmes</name><description>Number of measurements for this star</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>LAMOST</name><description>LAMOST identifier (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Gaia</name><description>Gaia DR2 identifier from cross-match</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>spID_blue</name><description>LAMOST spectral ID for the blue part</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="47*">char</dataType></column><column><name>spID_red</name><description>LAMOST spectral ID for the red part</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="47*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>[-10/79.1] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>S/N_blue</name><description>[10/722] Signal-to-noise ratio of the blue part</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/N_red</name><description>[10/801] Signal-to-noise ratio of the red part</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV_blue</name><description>[-572/571] Uncalibrated radial velocity of the blue part</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV_red</name><description>[-576/618] Uncalibrated radial velocity of the red part</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[3587/7983] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg</name><description>[0.6/5.5] Log of surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-1.92/0.35]? Iron abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[C/H]</name><description>[-1.49/0.85]? Carbon abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[N/H]</name><description>[-1.17/0.46]? Nitrogen abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[O/H]</name><description>[-1.67/0.5]? Oxygen abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Mg/H]</name><description>[-1.9/0.68]? Magnesium abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Al/H]</name><description>[-1.32/0.54]? Aluminum abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Si/H]</name><description>[-1.46/0.5]? Silicon abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[S/H]</name><description>[-1.32/0.46]? Sulfur abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Ca/H]</name><description>[-1.45/0.49]? Calcium abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Ti/H]</name><description>[-1.73/0.56]? Titanium abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Cr/H]</name><description>[-1.45/0.52] Cadmium abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ni/H]</name><description>[-1.63/0.62]? Nickel abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Cu/H]</name><description>[-1.79/0.64]? Copper abundance with respect to hydrogen</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>spIDv</name><description>LAMOST spectral ID (inform of Date, PlateID, SpectrographID, FiberID, MJM, PiplineVersion)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="47*">char</dataType></column></table></schema></tableset></ri:Resource>