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<ri:Resource created="2026-02-18T14:31:38Z" status="active" updated="2026-02-18T14:27:44Z" 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>Estimated magnitudes &amp; distances of LAMOST DR10 stars</title><shortName>J/AJ/169/266</shortName><identifier>ivo://CDS.VizieR/J/AJ/169/266</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yang C.</name></creator><creator><name>Xue X.-X.</name></creator><creator><name>Liu C.</name></creator><creator><name>Tian H.</name></creator><creator><name>Zhu L.</name></creator><creator><name>Zhang L.</name></creator><date role="Updated">2026-02-18T14:27:44Z</date><date role="Created">2026-02-18T14:31:38Z</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>stellar-distance</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>surveys</subject><description>Using the distance estimation method outlined in J. L. Carlin et al., a Bayesian approach specifically tailored for LAMOST data, we estimated distances for 7,450,303 spectra from 5,394,174 unique stars in the LAMOST DR10 low-resolution data set. To accommodate the significant increase in data volume and quality in LAMOST DR10, several improvements were applied to the method in J. L. Carlin et al.: utilizing denser isochrones, increasing the density of interpolated isochrone grids, and incorporating Gaia G-band magnitudes alongside Two Micron All Sky Survey K-band magnitudes for more comprehensive distance estimates. A comparison with Gaia parallaxes shows good consistency across the data. For parallaxes below 1mas, the estimated distances are underestimated by 4% for the K band and 10% for the G band, while for parallaxes below 0.25mas, the distances are overestimated by 9% for the K band and 7% for the G band. Distance uncertainties initially increase with distance, with relative distance uncertainties starting at 5% at 1kpc and rising to 17% at 20kpc, then decreasing to 10%-15% for distances greater than 50kpc. The number of stars with distances between 5 and 10kpc is ~1.8x10^5^, and ~6x10^4^ for distances greater than 10kpc.</description><source format="bibcode">2025AJ....169..266Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/169/266</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/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/389">II/389 : The Pan-STARRS release 1 (PS1) Survey - DR2 (Magnier+, 2025)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/162">V/162 : LAMOST DR11 catalogs (Luo+, 2026)</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/880/65">J/ApJ/880/65 : LAMOST K giants in Galactic halo substructures (Yang+, 2019)</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/ApJS/247/9">J/ApJS/247/9 : FGK stars magnetic activ. in LAMOST-Kepler field (Zhang+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/28">J/ApJS/247/28 : K2 star parameters from Gaia &amp; LAMOST (Hardegree-Ullman+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/910/46">J/ApJ/910/46 : Galactic anticenter substructure stars from LAMOST (Li+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/266/14">J/ApJS/266/14 : Am stars selected in LAMOST DR8-DR10 (Tian+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/267/5">J/ApJS/267/5 : S-type stars from LAMOST MRS DR10 spectra (Chen+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/224">J/AJ/165/224 : Distance determinations for LAMOST DR8 K-giants (Zhang+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/271/60">J/ApJS/271/60 : Magnetic activ. of G-type stars from LAMOST &amp; TESS (Su+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/272/43">J/ApJS/272/43 : Am and Ap star candidates from LAMOST DR10 (Yang+, 2024)</relatedResource><relatedResource>http://www.lamost.org/dr10/catalogue : LAMOST DR10 v2.0 database</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/AJ/169/266</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/169/266</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/169/266</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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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>Sp</name><description>Display the LAMOST DR10 spectrum</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>ObsID</name><description>[101001/1018116242] Unique identifier for the LAMOST spectrum (obsid)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Target</name><description>Target designation, JHHMMSS.ss+DDMMSS.s (designation)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Obs.Date</name><description>Target observation date (obsdate)</description><ucd>time.epoch;obs</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>RAJ2000</name><description>Fiber pointing right Aacension (J2000) (ra_obs)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Fiber pointing declination (J2000) (dec_obs)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>subClass</name><description>Stellar spectral type (subclass) (1)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>PanSTARRS</name><description>? Pan-STARRS (II/349) identifier (ps_id)</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>GaiaDR3</name><description>? Gaia DR3 (I/355) source ID (gaia\_source\_id)</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>Ksmag</name><description>[3.16/17.64]? Observed magnitude in the 2MASS Ks band (2)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>[5.68/21.03]? Observed magnitude in the Gaia DR3 G band (3)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(B-V)</name><description>[0.0/50.71] Color excess (Schlegel+, 1998ApJ...500..525S)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AKs</name><description>[0.0/14.2] Extinction in 2MASS Ks band (4)</description><unit>mag</unit><ucd>phys.absorption;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AG</name><description>[0.01/138.94] Extinction in Gaia G band (4)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ksmag0</name><description>[-3.33/17.64]? Extinction-corrected photometric magnitude in the 2MASS Ks band</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gmag0</name><description>[-124.61/20.93]? Extinction-corrected photometric magnitude in the Gaia G-band</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KsMag-16</name><description>[-8.0/6.13] 16th percentile of the cumulative PDF for KsMag (5)</description><unit>mag</unit><ucd>stat.min;phys.magAbs;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KsMag-50</name><description>[-8.0/6.18] 50th percentile of the cumulative PDF for KsMag (5)</description><unit>mag</unit><ucd>phys.magAbs;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KsMag-84</name><description>[-8.0/6.25] 84th percentile of the cumulative PDF for KsMag (5)</description><unit>mag</unit><ucd>stat.max;phys.magAbs;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GMag-16</name><description>[-4.0/9.15] 16th percentile of the cumulative PDF for GMag (5)</description><unit>mag</unit><ucd>stat.min;phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GMag-50</name><description>[-4.0/9.27] 50th percentile of the cumulative PDF for GMag (5)</description><unit>mag</unit><ucd>phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GMag-84</name><description>[-4.0/9.7] 84th percentile of the cumulative PDF for GMag (5)</description><unit>mag</unit><ucd>stat.max;phys.magAbs;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DistKs-16</name><description>[0.05/285.52]? Distance derived from KsMag-84 and Kmag0 (6)</description><unit>kpc</unit><ucd>stat.min;pos.distance;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DistKs-50</name><description>[0.05/295.14]? Distance derived from KsMag-50 and Kmag0 (6)</description><unit>kpc</unit><ucd>pos.distance;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DistKs-84</name><description>[0.05/1050.42]? Distance derived from KsMag-84 and Kmag0 (6)</description><unit>kpc</unit><ucd>stat.max;pos.distance;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>errDistKs</name><description>[0.0/71.99]? Distance uncertainty, calculated as (DistKs84-DistKs16)/2</description><unit>kpc</unit><ucd>stat.error;pos.distance;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DistG-16</name><description>[0.05/191.55]? Distance derived from GMag-84 and Gmag0 (6)</description><unit>kpc</unit><ucd>stat.min;pos.distance;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DistG-50</name><description>[0.05/235.66]? Distance derived from GMag-50 and Gmag0 (6)</description><unit>kpc</unit><ucd>pos.distance;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DistG-84</name><description>[0.05/709.1]? Distance derived from GMag-16 and Gmag0 (6)</description><unit>kpc</unit><ucd>stat.max;pos.distance;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>errDistG</name><description>[0.0/49.68]? Distance uncertainty, calculated as (DistG84-DistG16)/2</description><unit>kpc</unit><ucd>stat.error;pos.distance;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>