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<ri:Resource created="2020-04-20T12:18:43Z" 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>Kepler flare star parameters from DR25</title><shortName>J/ApJS/244/37</shortName><identifier>ivo://CDS.VizieR/J/ApJS/244/37</identifier><altIdentifier>doi:10.26093/cds/vizier.22440037</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Goodarzi H.</name></creator><creator><name>Mehrabi A.</name></creator><creator><name>Khosroshahi H.G.</name></creator><creator><name>He H.</name></creator><date role="Updated">2020-07-21T12:42:54Z</date><date role="Created">2020-04-20T12:18:43Z</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-flares</subject><description>We analyze the light curve of 1740 flare stars to study the relationship between the magnetic feature characteristics and the identified flare activity. Coverage and stability of magnetic features are inspired by rotational modulation of light-curve variations and flare activity of stars are obtained using our automated flare detection algorithm. The results show that: (i) the flare time occupation ratio (or flare frequency) and the total power of flares increase by increasing relative magnetic feature coverage and contrast in F-M-type stars; (ii) magnetic feature stability is highly correlated with the coverage and the contrast of the magnetic structures, as this is the case for the Sun; and (iii) stability, coverage, and contrast of the magnetic features, time occupation ratio, and total power of flares increases for G-, K-, and M-type stars by decreasing the Rossby number due to the excess of the produced magnetic field from dynamo procedure until reaching to the saturation level.</description><source format="bibcode">2019ApJS..244...37G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/244/37</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/V/133">V/133 : Kepler Input Catalog (Kepler, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/112">J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/50">J/AJ/141/50 : White-light flares on cool Kepler stars (Walkowicz+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stars with rot. periods &amp; X-ray luminosities (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/485.478">J/other/Nat/485.478 : Superflares on solar-type stars (Maehara+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/5">J/ApJS/209/5 : Superflares of Kepler stars. 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(Shibayama+, 2013)</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/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/447/2714">J/MNRAS/447/2714 : Flare stars across the H-R diagram (Balona+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/829/23">J/ApJ/829/23 : Stellar flares from Q0-Q17 Kepler LCs (Davenport, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/158">J/AJ/152/158 : Final Kepler transiting pl. search (DR25) (Twicken+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/207">J/ApJ/834/207 : Periodicity &amp; magnitude of Kepler LCs (Mehrabi+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/851/116">J/ApJ/851/116 : Long-term var. of Kepler sun-like stars (Montet+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/30">J/ApJS/229/30 : Revised properties of Q1-17 Kepler targets (Mathur+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/232/26">J/ApJS/232/26 : Catalog of Kepler flare stars (Van Doorsselaere+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/38">J/ApJS/235/38 : Kepler pl. cand. 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