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<ri:Resource created="2022-03-31T14:57:23Z" status="active" updated="2025-06-13T15:25:00Z" 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>Early-type star stellar rotations in LAMOST MRS. I.</title><shortName>J/ApJS/257/22</shortName><identifier>ivo://CDS.VizieR/J/ApJS/257/22</identifier><altIdentifier>doi:10.26093/cds/vizier.22570022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sun W.</name></creator><creator><name>Duan X.-W.</name></creator><creator><name>Deng L.</name></creator><creator><name>de Grijs R.</name></creator><creator><name>Zhang Bo</name></creator><creator><name>Liu C.</name></creator><date role="Updated">2022-09-30T21:57:56Z</date><date role="Created">2022-03-31T14:57:23Z</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>early-type-stars</subject><subject>effective-temperature</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>chemical-abundances</subject><subject>stellar-masses</subject><subject>surveys</subject><description>We derive stellar parameters and abundances ("stellar labels") of 40034 late-B and A-type main-sequence stars extracted from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope Medium Resolution Survey (LAMOST-MRS). The primary selection of our early-type sample was obtained from LAMOST Data Release 7 based on spectral-line indices. We employed the Stellar Label Machine to derive their spectroscopic stellar parameters, drawing on Kurucz spectral synthesis models with 6000&lt;Teff&lt;15000K and -1&lt;[M/H]&lt;1dex. For a signal-to-noise ratio of ~60, the cross validated scatter is ~75K, 0.06dex, 0.05dex, and ~3.5km/s for Teff, logg, [M/H], and vsini, respectively. A comparison with objects with prior known stellar labels shows great consistency for all stellar parameters, except for logg. Although this is an intrinsic caveat that comes from the MRS's narrow wavelength coverage, it only has a minor effect on estimates of the stellar rotation rates because of the decent spectral resolution and the profile-fitting method employed. The masses and ages of our early-type sample stars were inferred from nonrotating stellar evolution models. This paves the way for reviewing the properties of stellar rotation distributions as a function of stellar mass and age.</description><source format="bibcode">2021ApJS..257...22S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/257/22</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/B/pastel">B/pastel : The PASTEL catalogue (Soubiran+, 2016-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/pollux">B/pollux : POLLUX database of synthetic stellar spectra (Palacios+ 2010-2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/226">III/226 : Rotational Velocities of Stars (Glebocki+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/146">V/146 : LAMOST DR1 catalogs (Luo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/153">V/153 : LAMOST DR4 catalogs (Luo+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/94/687">J/ApJS/94/687 : Old stellar populations. 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(computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></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>GaiaEDR3</name><description>Gaia EDR3 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>obsid</name><description>[588904135/747816243] LAMOST MRS observation identifier</description><ucd>meta.id;obs.param;obs</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>RA_ICRS</name><description>Gaia EDR3 right ascension (ICRS) at Ep=2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>Gaia EDR3 declination (ICRS) at Ep=2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>EWHa</name><description>[2.4/10] Line indice, H{alpha} equivalent width, Angstroms</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EWMg</name><description>[-0.2/10] Line indice, Mg Ib equivalent width, Angstroms</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVelb</name><description>[-249.2/250] Radial velocity, blue arm</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVelr</name><description>[-204/184] Radial velocity, red arm</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[7000/14499] Effective temperature from SLAM</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[0/401] Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[3.13/4.84] Surface gravity from 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>[0/0.5] Uncertainty in logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[M/H]</name><description>[0/0.3] Uncertainty in [M/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vsini</name><description>[3.5/449.5] Projected rotation velocity from SLAM</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_vsini</name><description>[0/18] Uncertainty in vsini</description><unit>km/s</unit><ucd>stat.error;phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLstar</name><description>[0.7/3.4] Logarithmic luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logLstar</name><description>[0.012/0.12] Uncertainty in logLstar</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mstar</name><description>[1.5/6.1] Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mstar</name><description>[0/0.1] Uncertainty in Mstar</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>t/tms</name><description>[0/1] Life span from the zero-age main sequence (ZAMS) to the terminal-age main sequence (TAMS)</description><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_t/tms</name><description>[0/0.15] Uncertainty in t/tms</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNRb</name><description>[0/999] Signal-to-noise ratio, blue arm</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNRr</name><description>[0/999] Signal-to-noise ratio, red arm</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>chi2b</name><description>[0/24] {chi}^2 estimate of best fit of blue arm</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>