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<ri:Resource created="2023-11-16T09:57:22Z" status="active" updated="2026-08-03T07:31:04Z" 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>Flares in the Kepler short cadence data</title><shortName>J/MNRAS/502/2033</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/502/2033</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-fp-1zh</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jackman J.A.G.</name></creator><creator><name>Shkolnik E.</name></creator><creator><name>Loyd R.O.P.</name></creator><date role="Updated">2026-08-03T07:31:04Z</date><date role="Created">2023-11-16T09:57:22Z</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><subject>effective-temperature</subject><subject>stellar-radii</subject><subject>visible-astronomy</subject><description>We present the results of a search for stellar flares from stars neighbouring the target sources in the Kepler short cadence data. These flares have been discarded as contaminants in previous surveys and therefore provide an unexplored resource of flare events, in particular high-energy events from faint stars. We have measured M dwarf flare energies up to 1.5x10^35^erg, pushing the limit for flare energies measured using Kepler data. We have used our sample to study the flaring activity of wide binaries, finding that the lower mass counterpart in a wide binary flares more often at a given energy. Of the 4430 flares detected in our original search, 298 came from a neighbouring star, a rate of 6.7+/-0.4 per cent for the Kepler short cadence light curves. 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