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<ri:Resource created="2024-07-31T08:20:05Z" 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 chromospheric activity of LAMOST sources</title><shortName>J/A+A/688/A23</shortName><identifier>ivo://CDS.VizieR/J/A+A/688/A23</identifier><altIdentifier>doi:10.26093/cds/vizier.36880023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang W.</name></creator><creator><name>Zhang J.</name></creator><creator><name>He H.</name></creator><creator><name>Luo A.</name></creator><creator><name>Zhang H.</name></creator><date role="Updated">2024-11-29T20:04:56Z</date><date role="Created">2024-07-31T08:20:05Z</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>g-stars</subject><subject>spectroscopy</subject><subject>stellar-activity</subject><subject>visible-astronomy</subject><description>The dependence of stellar magnetic activity on stellar parameters is inspired by the chromospheric activity studies based on the large-scale spectroscopic surveys. The main objective of this project is to provide the chromospheric activity parameter database for the LAMOST Low-Resolution Spectroscopic Survey (LRS) spectra of solar-like stars and explore the overall property of stellar chromospheric activity. The CaII H and K lines were employed to construct indicators for assessing and studying the chromospheric activity of solar-like stars. We investigated the widely used bolometric- and photospheric-calibrated chromospheric activity index R'_HK_, derived from the method in the classic literature (R'_HK,classic_) and the method based on the PHOENIX model (R'_HK,PHOENIX_). Since the detailed stellar atmospheric parameters, effective temperature (T_eff_), surface gravity (logg), and metallicity ([Fe/H]) are available for LAMOST, we estimated the chromospheric activity index R'_HK,PHOENIX_, along with the corresponding bolometric calibrated index R_HK,PHOENIX_, taking these parameters into account. We provided the database of the derived chromospheric activity parameters for 1,122,495 LAMOST LRS spectra of solar-like stars. Our calculations show that logR'_HK,PHOENIX_ is approximately linearly correlated with logR'_HK,classic_. The results based on our extensive archive support the view that the dynamo mechanism of solar-like stars is generally consistent with the Sun; and the value of the solar chromospheric activity index is located at the midpoint of the solar-like star sample. We further investigated the proportions of solar-like stars with different chromospheric activity levels (very active, active, inactive, and very inactive). The investigation indicates that the occurrence rate of high levels of chromospheric activity is lower among the stars with effective temperatures between 5600 and 5900K.</description><source format="bibcode">2024A&amp;A...688A..23Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/688/A23</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>https://doi.org/10.5281/zenodo.8378849 : Paper data</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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32388-32390 32392-32394 32396 32416 32418-32419 32422-32423 32446 32489-32491 32564 32566-32567 32581-32585 32587 32609-32611 32620-32621 32623 32628-32629 32631-32633 32635 32686 32696-32697 32699 32709 32711 36711 36714-36715 36722-36723 36726 36732 36734-36735 36765 36778-36779 36783 36794 36801-36803 36832-36833 36836-36837 36839 36849-36851 40859 40880-40882 40889-40891 40907 40913-40915 40921-40923 44990 45019 48982 48997-48999 49008 49011 49014 49020 49022-49023 49093 49095 49116-49117 49119 49141</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/688/A23?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/688/A23/table3</name><description>Catalogue data</description><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>sp</name><description>Display the DR9 LAMOST spectrum, if available</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>ObsId</name><description>Unique observation identifier of LAMOST LRS spectrum</description><ucd>meta.id;obs.param;obs</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>ObsDate</name><description>Spectral observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>fitsname</name><description>FITS file name of LAMOST LRS spectrum</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="45*">char</dataType></column><column><name>snrg</name><description>Signal-to-noise ratio in the g band (S/N_g_) of LAMOST LRS spectrum</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>snrr</name><description>Signal-to-noise ratio in the r band (S/N_r_) of LAMOST LRS spectrum</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>Effective temperature (T_eff_) derived from the LASP</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Teff</name><description>? Uncertainty of Teff derived from the LASP</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg</name><description>Surface gravity (logg) derived from the LASP</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>? Uncertainty of logg derived from the LASP</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>Metallicity ([Fe/H]) derived from the LASP</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>? Uncertainty of [Fe/H] derived from the LASP</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RV</name><description>Radial velocity (V_r_) derived from the LASP</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>? Uncertainty of RV derived from the LASP</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Right ascension (RA) of fiber pointing (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (DEC) of fiber pointing (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>GaiaDR3</name><description>Source identifier in Gaia DR3 catalog</description><ucd>meta.id;meta.main</ucd></column><column><name>Gmag</name><description>G magnitude in Gaia DR3 catalog</description><unit>ag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Stri</name><description>S_tri_ index of LAMOST LRS</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Stri</name><description>? Uncertainty of Stri</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SMWO</name><description>S_MWO_ activity index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SMWO</name><description>? Uncertainty of SMWO</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logRHKcl</name><description>logR_HK_ activity index derived from the method in the classic literature</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logRHKcl</name><description>? Uncertainty of logRHKcl</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logRHKPh</name><description>logR_HK_ activity index derived from the method based on the PHOENIX model</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logRHKPh</name><description>? Uncertainty of logRHKPh</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logRpHKcl</name><description>logR'_HK_ activity index derived from the method in the classic literature</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logRpHKcl</name><description>? Uncertainty of logRpHKcl</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logRpHKPh</name><description>logR'_HK_ activity index derived from the method based on the PHOENIX model</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logRpHKPh</name><description>? Uncertainty of logRpHKPh</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>