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<ri:Resource created="2022-11-07T14:45:16Z" 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>LAMOST DR7 stellar param. from RRNet model</title><shortName>J/ApJS/261/36</shortName><identifier>ivo://CDS.VizieR/J/ApJS/261/36</identifier><altIdentifier>doi:10.26093/cds/vizier.22610036</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Xiong S.</name></creator><creator><name>Li X.</name></creator><creator><name>Liao C.</name></creator><date role="Updated">2022-11-15T07:26:26Z</date><date role="Created">2022-11-07T14:45:16Z</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>astronomical-models</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><description>This work proposes a residual recurrent neural network (RRNet) for synthetically extracting spectral information and estimating stellar atmospheric parameters together with 15 chemical element abundances for medium-resolution spectra from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). The RRNet consists of two fundamental modules: a residual module and a recurrent module. The residual module extracts spectral features based on the longitudinally driving power from parameters, while the recurrent module recovers spectral information and restrains the negative influences from noises based on Cross-band Belief Enhancement. RRNet is trained by the spectra from common stars between LAMOST DR7 and the APOGEE-Payne catalog. The 17 stellar parameters and their uncertainties for 2.37 million medium-resolution spectra from LAMOST DR7 are predicted. For spectra with a signal-to-noise ratio &gt;=10, the precision of estimations (Teff and logg) are 88K and 0.13dex, respectively, elements C, Mg, Al, Si, Ca, Fe, and Ni are 0.05-0.08dex, and N, O, S, K, Ti, Cr, and Mn are 0.09-0.14dex, while that of Cu is 0.19dex. Compared with StarNet and SPCANet, RRNet shows higher accuracy and robustness. In comparison to Apache Point Observatory Galactic Evolution Experiment and Galactic Archaeology with HERMES surveys, RRNet manifests good consistency within a reasonable range of bias.</description><source format="bibcode">2022ApJS..261...36X</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/261/36</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/146">V/146 : LAMOST DR1 catalogs (Luo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</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/other/RAA/11.924">J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for the APOGEE elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/126">J/AJ/156/126 : Stellar parameters from BACCHUS analysis (Jonsson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/245/34">J/ApJS/245/34 : Abundances for 6 million stars from LAMOST DR5 (Xiang+, 2019)</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/A+A/640/A127">J/A+A/640/A127 : Open cluster properties with Gaia and LAMOST (Zhong+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/506/150">J/MNRAS/506/150 : The GALAH+ Survey DR3 (Buder+, 2021)</relatedResource><relatedResource>http://www.lamost.org/dr7/ : LAMOST DR7 home page</relatedResource><relatedResource>http://github.com/Chan-0312/RRNet : RRNet code and trained models</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/ApJS/261/36</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/261/36</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/261/36</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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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 27356 27361 27364-27365 27405 27407 27409-27412 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 27622-27623 27634-27635 27638 27649-27651 27664 27666-27667 27775 27784-27785 27788 27893 27946-27947 27950 27970 27973 27975 27986 27992 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 28543 28560 28562 28568 28570 28580-28582 28592 28629-28631 28660-28661 30022-30023 30034-30035 30038 30064-30065 30068 30209-30211 30226 30240-30241 30243 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 32536 32538 32541 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/ApJS/261/36?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/261/36/rrnetcat</name><description>The LAMOST-RRNet catalog</description><column><name>MgH</name><description>[-1.9/0.6] [Mg/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</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>[N/H]</name><description>[-1.94/0.9] [N/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>obsID</name><description>[588902003/747816250] Identification of LAMOST spectrum</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</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>[-9.15/79.1] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Nameb</name><description>Spectrum extension name of blue part</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Namer</name><description>Spectrum extension name of red part</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>SNRb</name><description>[10/999] Signal-to-noise ratio of blue part</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNRr</name><description>[10/999] Signal-to-noise ratio of red part</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[3779/6597] 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>[33/484] Teff uncertainty</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg</name><description>[0.95/4.8] 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>e_logg</name><description>[0.08/0.8] logg uncertainty</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CH</name><description>[-2.38/0.34] [C/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_CH</name><description>[0.029/0.5] CH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[N/H]</name><description>[0.038/0.52] [N/H] uncertainty</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>OH</name><description>[-1.44/0.44] [O/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_OH</name><description>[0.028/0.5] OH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_MgH</name><description>[0.02/0.4] MgH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>AlH</name><description>[-2.7/0.8] [Al/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_AlH</name><description>[0.027/0.6] AlH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SiH</name><description>[-1.81/0.61] [Si/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SiH</name><description>[0.019/0.31] SiH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SH</name><description>[-1.91/0.5] [S/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SH</name><description>[0.039/0.42] SH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>KH</name><description>[-2.1/0.5] [K/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_KH</name><description>[0.04/0.61] KH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>CaH</name><description>[-1.97/0.52] [Ca/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_CaH</name><description>[0.02/0.4] CaH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TiH</name><description>[-1.75/0.6] [Ti/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_TiH</name><description>[0.026/0.6] TiH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>CrH</name><description>[-2.25/0.64] [Cr/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_CrH</name><description>[0.028/0.5] CrH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MnH</name><description>[-2.1/0.5] [Mn/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_MnH</name><description>[0.029/0.6] MnH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[Fe/H]</name><description>[-1.88/0.61] [Fe/H] abundance</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Fe/H]</name><description>[0.025/0.4] [Fe/H] uncertainty</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NiH</name><description>[-2.55/0.72] [Ni/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_NiH</name><description>[0.02/0.5] NiH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>CuH</name><description>[-2.6/0.6] [Cu/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_CuH</name><description>[0.05/0.7] CuH uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flag</name><description>[0/1] Recommended flag: 1=good</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FileName</name><description>Name of the FITS file LAMOST spectrum</description><ucd>meta.id;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="45*">char</dataType></column></table></schema></tableset></ri:Resource>