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<ri:Resource created="2026-05-22T13:56:55Z" status="active" updated="2026-05-22T13:15:12Z" 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>Asteroseismology of 687 TESS red giants</title><shortName>J/ApJS/279/37</shortName><identifier>ivo://CDS.VizieR/J/ApJS/279/37</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhou J.</name></creator><creator><name>Bi S.</name></creator><creator><name>Li Y.</name></creator><creator><name>Yu J.</name></creator><creator><name>Li T.</name></creator><creator><name>Zhang X.</name></creator><creator><name>Ye L.</name></creator><creator><name>Li M.</name></creator><creator><name>Long L.,Sun T.</name></creator><creator><name>Chen Y.</name></creator><date role="Updated">2026-05-22T13:15:12Z</date><date role="Created">2026-05-22T13:56:55Z</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>asteroseismology</subject><subject>giant-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>The individual modes and asymptotic parameters are important characteristics of stellar oscillation. Using TESS 2 minute cadence data from Sectors 1 to 75, we perform asteroseismic analysis of 687 red giants, and provide their oscillation mode parameters. The mode parameters, including frequencies {nu}_n,l_, amplitudes A_n,l_, and line widths {Gamma}_n,l_, are obtained through Markov Chain Monte Carlo fitting. The median uncertainty for frequency is 0.047{mu}Hz. Using the radial mode frequencies, we calculate the values of {Delta}{nu}, and derive asymptotic parameters ({epsilon}p, {epsilon}c, {delta}{nu}0l, q, and {Delta}{Pi}1) based on l=0,1,2 modes. For red giants with {Delta}{nu}&gt;15.6{mu}Hz, there is a weaker correlation between {delta}{nu}02 and {Delta}{nu}, and a stronger mass dependence, compared to stars with lower {Delta}{nu}. Additionally, the ratio {delta}{nu}02/{Delta}{nu} presents a pronounced increase with {Delta}{nu} decrease, as these stars undergo rapid core contraction and their convective envelopes extend deep into the interior. At this stage, the ratio {delta}{nu}02/{Delta}{nu} may serve as a robust indicator for diagnosing the location of the convective boundary. Furthermore, the {epsilon}c values can be a potential index to distinguish red clump (RC) and secondary RC stars from red giant branch stars in the TESS field.</description><source format="bibcode">2025ApJS..279...37Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/279/37</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A143">J/A+A/540/A143 : Oscillations of red giants observed by Kepler (Mosser+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/L41">J/ApJ/765/L41 : Asteroseismic classification of KIC objects (Stello+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/1">J/ApJS/210/1 : Asteroseismic study of solar-type stars (Chaplin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/2">J/ApJS/211/2 : Revised properties of Q1-16 Kepler targets (Huber+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/827/50">J/ApJ/827/50 : Kepler faint red giants (Mathur+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/158">J/AJ/152/158 : Final Kepler transiting planet search (DR25) (Twicken+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/1297">J/MNRAS/463/1297 : Asteroseismology of misclassified red giants (Yu+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/172">J/ApJ/835/172 : Kepler asteroseismic LEGACY sample. 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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>TIC</name><description>[1713457/468827515] TESS input catalog identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>primary</flag></column><column><name>dnu</name><description>[1.45/69.8] Large separation, {Delta}{nu}</description><unit>uHz</unit><ucd>em.freq;src.var;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dnu</name><description>[0.01/0.7] Uncertainty in dnu</description><unit>uHz</unit><ucd>stat.error;em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>epsc</name><description>[0.43/1.7]? Dimensionless offset, {epsilon}_c_</description><ucd>arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_epsc</name><description>[0.02/0.7]? Uncertainty in epsp</description><ucd>stat.error;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>epsp</name><description>[-0.32/1.63] Dimensionless offset, {epsilon}_p_</description><ucd>arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_epsp</name><description>[0.01/0.9] Uncertainty in epsp</description><ucd>stat.error;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>d02</name><description>[0.17/6.03]? Small frequency separation, {delta}{nu}_02_</description><unit>uHz</unit><ucd>em.freq;src.var;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_d02</name><description>[0.02/1.6]? Uncertainty in d02</description><unit>uHz</unit><ucd>stat.error;em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>d01</name><description>[-3.3/2.1]? Small frequency spacing, {delta}{nu}_01_</description><unit>uHz</unit><ucd>em.freq;src.var;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_d01</name><description>[0.02/75.5]? Uncertainty in d01</description><unit>uHz</unit><ucd>stat.error;em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>q</name><description>[0.05/0.7]? Coupling factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_q</name><description>[0/1.52]? 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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>l</name><description>[0/2] mode</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>fc</name><description>[5/1450.21] mode frequency parameter {nu}_n,l_</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_fc</name><description>[0/1.5] Uncertainty in fc</description><unit>uHz</unit><ucd>stat.error;em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Amp</name><description>[0.16/93.5]? amplitude parameters, A_n,l_</description><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Amp</name><description>[0.1/15.5]? Uncertainty in Amp</description><ucd>stat.error;src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lw</name><description>[0/4.5]? linewidth parameters, {Gamma}_n,l_</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_lw</name><description>[0/1.2]? Uncertainty in lw</description><unit>uHz</unit><ucd>stat.error;em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lnK</name><description>[-26/2660.21] Bayesian factor to assess existence of a mode</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_lnK</name><description>[0/238.5] Uncertainty in lnK</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>