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<ri:Resource created="2021-08-17T09:33:49Z" 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>Superflares on solar-type stars from TESS first year</title><shortName>J/ApJ/890/46</shortName><identifier>ivo://CDS.VizieR/J/ApJ/890/46</identifier><altIdentifier>doi:10.26093/cds/vizier.18900046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tu Z.-L.</name></creator><creator><name>Yang M.</name></creator><creator><name>Zhang Z.J.</name></creator><creator><name>Wang F.Y.</name></creator><date role="Updated">2021-09-29T13:20:08Z</date><date role="Created">2021-08-17T09:33:49Z</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>g-stars</subject><subject>stellar-flares</subject><description>Superflares, which are strong explosions on stars, have been well studied with the progress of spacetime-domain astronomy. In this work, we present the study of superflares on solar-type stars using Transiting Exoplanet Survey Satellite (TESS) data. Thirteen sectors of observations during the first year of the TESS mission covered the southern hemisphere of the sky, containing 25734 solar-type stars. We verified 1216 superflares on 400 solar-type stars through automatic search and visual inspection with 2 minute cadence data. Our result suggests a higher superflare frequency distribution than the result from Kepler. This may be because the majority of TESS solar-type stars in our data set are rapidly rotating stars. The power-law index {gamma} of the superflare frequency distribution (dN/dE{propto}E^-{gamma}^) is constrained to be {gamma}=2.16+/-0.10, which is a little larger than that of solar flares but consistent with the results from Kepler. Because only seven superflares of Sun-like stars are detected, we cannot give a robust superflare occurrence frequency. Four stars were accompanied by unconfirmed hot planet candidates. Therefore, superflares may possibly be caused by stellar magnetic activities instead of planet-star interactions. We also find an extraordinary star, TIC43472154, which exhibits about 200 superflares per year. In addition, the correlation between the energy and duration of superflares (T_duration_{propto}E^{beta}^) is analyzed. We derive the power-law index to be {beta}=0.42+/-0.01, which is a little larger than {beta} = 1/3 from the prediction according to magnetic reconnection theory.</description><source format="bibcode">2020ApJ...890...46T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/890/46</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/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 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/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/50">J/AJ/141/50 : White-light flares on cool stars from Kepler (Walkowicz+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/93">J/AJ/143/93 : Rotational velocities in early-M stars (Reiners+, 2012)</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. I. (Shibayama+, 2013)</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/ApJ/849/36">J/ApJ/849/36 : Flaring activity of M dwarfs in the Kepler field (Yang+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/851/91">J/ApJ/851/91 : Stat. studies of solar white-light flares (Namekata+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/614/A76">J/A+A/614/A76 : CARMENES input catalogue of M dwarfs. III. (Jeffers+, 2018)</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/ApJS/241/29">J/ApJS/241/29 : Flare catalog through LC data of Kepler DR25 (Yang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/88">J/ApJ/883/88 : Short-duration flares from GALEX &amp; Kepler (Brasseur+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/60">J/AJ/159/60 : Flares from 1228 stars in TESS sectors 1 &amp; 2 (Gunther+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/CoSka/51.78">J/other/CoSka/51.78 : Flare stars in nearby Gal. open clusters (Maryeva+ 2021)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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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>[737327/468899939] TESS identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>primary</flag></column><column><name>Teff</name><description>[5103/5998] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[4/4.71] log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[0.69/1.7] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[0.14/25.5] Stellar rotational period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nfl</name><description>[1/63] Number of flares (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nset</name><description>[1/13] Number of Set-n (2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Freq</name><description>[1.19/233.2] Flare frequency, f*, deduced by Equ. 9 (N_*flares_/{tau}*) (3)</description><unit>yr**-1</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flag</name><description>Flare star flag (4)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</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>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/890/46/table2</name><description>Superflares</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TIC</name><description>[737327/468899939] TESS identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>DatePk</name><description>[1325.58/1681.99] Date of superflares' peak</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FluxPk</name><description>[1.29e+31/7.9e+33] Peak Flux (1)</description><unit>1e-07W</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Energy</name><description>[4.75e+33/1.8e+37] Superflare energy</description><unit>1e-07J</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Duration</name><description>[480/15960] Superflare duration</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>