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<ri:Resource created="2022-05-11T14:33:44Z" 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>EvryFlare. III. Superflares from Evryscope &amp; TESS</title><shortName>J/ApJ/902/115</shortName><identifier>ivo://CDS.VizieR/J/ApJ/902/115</identifier><altIdentifier>doi:10.26093/cds/vizier.19020115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Howard W.S.</name></creator><creator><name>Corbett H.</name></creator><creator><name>Law N.M.</name></creator><creator><name>Ratzloff J.K.</name></creator><creator><name>Galliher N.,Glazier A. L</name></creator><creator><name>Gonzalez R.</name></creator><creator><name>Vasquez Soto A.</name></creator><creator><name>Fors O.</name></creator><creator><name>del Ser D.</name></creator><creator><name>Haislip J.</name></creator><date role="Updated">2022-09-30T22:14:20Z</date><date role="Created">2022-05-11T14:33:44Z</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>m-stars</subject><subject>two-color-diagrams</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>visible-astronomy</subject><description>Superflares may provide the dominant source of biologically relevant UV radiation to rocky habitable-zone M-dwarf planets (M-Earths), altering planetary atmospheres and conditions for surface life. The combined line and continuum flare emission has usually been approximated by a 9000K blackbody. If superflares are hotter, then the UV emission may be 10 times higher than predicted from the optical. However, it is unknown for how long M-dwarf superflares reach temperatures above 9000K. Only a handful of M-dwarf superflares have been recorded with multiwavelength high-cadence observations. We double the total number of events in the literature using simultaneous Evryscope and Transiting Exoplanet Survey Satellite observations to provide the first systematic exploration of the temperature evolution of M-dwarf superflares. We also increase the number of superflaring M-dwarfs with published time-resolved blackbody evolution by ~10x. We measure temperatures at 2 minutes cadence for 42 superflares from 27 K5-M5 dwarfs. We find superflare peak temperatures (defined as the mean of temperatures corresponding to flare FWHM) increase with flare energy and impulse. We find the amount of time flares emit at temperatures above 14000K depends on energy. We discover that 43% of the flares emit above 14000K, 23% emit above 20000K and 5% emit above 30000K. The largest and hottest flare briefly reached 42000K. Some do not reach 14000 K. During superflares, we estimate M-Earths orbiting &lt;200 Myr stars typically receive a top-of-atmosphere UV-C flux of ~120W/m^2^ and up to 10^3^W/m^2^, 100-1000 times the time-averaged X-ray and UV flux from Proxima Cen.</description><source format="bibcode">2020ApJ...902..115H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/902/115</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/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</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/AJ/132/866">J/AJ/132/866 : New M dwarfs in solar neighborhood (Riaz+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/460/695">J/A+A/460/695 : Search for Associations Containing Young stars (Torres+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2340">J/AJ/134/2340 : Membership of Praesepe &amp; Coma Berenices (Kraus+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/15">J/ApJS/207/15 : M dwarf flare spectra (Kowalski+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/443/2561">J/MNRAS/443/2561 : CONCH-SHELL catalog of nearby M dwarfs (Gaidos+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/146">J/AJ/147/146 : Spectroscopy of Tuc-Hor candidate members (Kraus+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/81">J/ApJ/788/81 : BANYAN III. 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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>[5796048/441398770] TESS Input catalog ID</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>m_TIC</name><description>Number of flares for this star</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Date</name><description>Observation date and time (ISO 8601, UTC) (1)</description><unit>s</unit><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>logEg'</name><description>[31.2/35.1] Evryscope flare energy (erg)</description><unit>log(1e-07J)</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logET</name><description>[31.25/35] TESS flare energy (erg)</description><unit>log(1e-07J)</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>g'Amp</name><description>[0.08/7.3] Evryscope amplitude in normalized flux, A_g'_ ({Delta}F/F)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>TAmp</name><description>[0.01/0.65] TESS amplitude in normalized flux, A_T_ ({Delta}F/F</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Color</name><description>[0.07/6.6] Flare color between normalized-flux amplitudes (A_g'_-A_T_)</description><unit>mag</unit><ucd>phot.color;em.opt;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Color</name><description>[0.003/0.6] Uncertainty in Color</description><unit>mag</unit><ucd>stat.error;phot.color</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TeffPk</name><description>[2700/43200] Peak temperature, avg. temperature in FWHM</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_TeffPk</name><description>[300/3300] Uncertainty in TeffPk</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TeffTot</name><description>[2600/50000] Total temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_TeffTot</name><description>[200/13400]? 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