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<ri:Resource created="2019-06-17T13:36:00Z" 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 long- and short-cadence flare parameters</title><shortName>J/ApJ/859/87</shortName><identifier>ivo://CDS.VizieR/J/ApJ/859/87</identifier><altIdentifier>doi:10.26093/cds/vizier.18590087</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yang H.</name></creator><creator><name>Liu J.</name></creator><creator><name>Qiao E.</name></creator><creator><name>Zhang H.</name></creator><creator><name>Gao Q.</name></creator><creator><name>Cui K.</name></creator><creator><name>Han H.</name></creator><date role="Updated">2019-07-24T13:45:14Z</date><date role="Created">2019-06-17T13:36:00Z</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>Flare research is becoming a burgeoning realm of interest in the study of stellar activity due to the launch of Kepler in 2009. Kepler provides data with two time resolutions, i.e., the long-cadence (LC) data with a time resolution of 30 minutes and the short-cadence (SC) data with a time resolution of 1 minute, both of which can be used to study stellar flares. In this paper, we search flares in light curves with both LC data and SC data, and compare them in aspects of the true-flare rate, the flare energy, the flare amplitude, and the flare duration. It is found that LC data systematically underestimated the energies of flares by 25%, and underestimated the amplitudes of flares by 60% compared with SC flares. The durations are systematically overestimated by 50% compared with SC flares. However, the above percentages are poorly constrained and there is a lot of scatter. About 60% of SC flares have not been detected by LC data. We investigate the limitation of LC data, and suggest that although LC data cannot reflect the detailed profiles of flares, they can also capture the basic properties of stellar flares.</description><source format="bibcode">2018ApJ...859...87Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/859/87</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 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/ApJ/743/138">J/ApJ/743/138 : Spectroscopic survey of bright white dwarfs (Gianninas+, 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/other/Nat/485.478">J/other/Nat/485.478 : Superflares on solar-type stars (Maehara+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/4">J/ApJ/754/4 : HST monitoring of flaring stars in Gal. bulge (Osten+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/2240">J/MNRAS/431/2240 : Activity in A-type stars from Kepler (Balona, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. 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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>KIC</name><description>[1025986/12406908] Kepler Input Catalog identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Ind</name><description>[0/939] Flare Index (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BTime</name><description>[131.9/1587] Flare start time, Kepler Barycentric Julian Day (BKJD), BJD-2454833</description><unit>d</unit><ucd>time.start</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ETime</name><description>[131.9/1587] Flare end time, Kepler Barycentric Julian Day (BKJD), BJD-2454833</description><unit>d</unit><ucd>time.end</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Amp</name><description>[97.3/3551809.1] Flare amplitude in parts per million</description><unit>1e-06count</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logE</name><description>[30/36.6] log of flare energy, in ergs</description><unit>log(1e-07J)</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ns</name><description>Number of SC flare measurements for this long-cadence flare (link to Table 3)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/859/87/table3</name><description>The parameters of short-cadence (SC) flares for 156 KIC stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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