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<ri:Resource created="2020-12-17T08:46:53Z" 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>M giant stars asteroseismology with Kepler and APOGEE</title><shortName>J/AJ/160/18</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/18</identifier><altIdentifier>doi:10.26093/cds/vizier.51600018</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Auge C.</name></creator><creator><name>Huber D.</name></creator><creator><name>Heinze A.</name></creator><creator><name>Shappee B.J.</name></creator><creator><name>Tonry J.</name></creator><creator><name>Chakrabarti S.,Sanderson R.E.</name></creator><creator><name>Denneau L.</name></creator><creator><name>Flewelling H.</name></creator><creator><name>Holoien T.W.-S.</name></creator><creator><name>Kochanek C.S.,Pignata G.</name></creator><creator><name>Sickafoose A.</name></creator><creator><name>Stalder B.</name></creator><creator><name>Stanek K.Z.</name></creator><creator><name>Stello D.</name></creator><creator><name>Thompson T.A.</name></creator><date role="Updated">2021-07-05T06:49:24Z</date><date role="Created">2020-12-17T08:46:53Z</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>effective-temperature</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Evolved stars near the tip of the red giant branch show solar-like oscillations with periods spanning hours to months and amplitudes ranging from ~1mmag to ~100mmag. The systematic detection of the resulting photometric variations with ground-based telescopes would enable the application of asteroseismology to a much larger and more distant sample of stars than is currently accessible with space-based telescopes such as Kepler or the ongoing Transiting Exoplanet Survey Satellite mission. We present an asteroseismic analysis of 493 M giants using data from two ground-based surveys: the Asteroid Terrestrial-impact Last Alert System (ATLAS) and the All-Sky Automated Survey for Supernovae (ASAS-SN). By comparing the extracted frequencies with constraints from Kepler, the Sloan Digital Sky Survey Apache Point Observatory Galaxy Evolution Experiment, and Gaia we demonstrate that ground-based transient surveys allow accurate distance measurements to oscillating M giants with a precision of ~15%. Using stellar population synthesis models we predict that ATLAS and ASAS-SN can provide asteroseismic distances to ~2x106 galactic M giants out to typical distances of 20-50kpc, vastly improving the reach of Gaia and providing critical constraints for Galactic archeology and galactic dynamics.</description><source format="bibcode">2020AJ....160...18A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/18</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/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource 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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/ApJ/844/102">J/ApJ/844/102 : KIC star plxs from asteroseismology vs Gaia (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/94">J/AJ/154/94 : APOGEE-2 data from DR16 (Majewski+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/L4">J/ApJ/844/L4 : PS1 RRab stars tracing outer Virgo overdensity (Sesar+,2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/866/99">J/ApJ/866/99 : Radii of KIC stars &amp; planets using Gaia DR2 (Berger+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/241">J/AJ/156/241 : Catalog of variable stars measured by ATLAS (Heinze+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/236/42">J/ApJS/236/42 : Asteroseismology of ~16000 Kepler red giants (Yu+, 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