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<ri:Resource created="2026-08-12T13:26:20Z" status="active" updated="2026-08-12T12:43:56Z" 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>Flare events in TESS 2min cadence light curves</title><shortName>J/ApJS/281/52</shortName><identifier>ivo://CDS.VizieR/J/ApJS/281/52</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang Y.</name></creator><creator><name>Zhang L.-Y.</name></creator><creator><name>Su T.</name></creator><creator><name>Misra P.</name></creator><creator><name>Han X.L.</name></creator><date role="Updated">2026-08-12T12:43:56Z</date><date role="Created">2026-08-12T13:26:20Z</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>photometry</subject><subject>visible-astronomy</subject><subject>giant-stars</subject><subject>stellar-spectral-types</subject><subject>effective-temperature</subject><description>Stellar flares are important indicators of stellar magnetic activity and have been widely studied. Detailed studies of flares have raised new questions. For example, the quasiperiodic pulsation (QPP) phenomenon in flares challenges standard flare models, yet the underlying mechanism of this phenomenon remains poorly understood. We utilize the 2 minute cadence light-curve data from TESS Sectors 1-74 prior to 2024 January 30. By combining the previously published convolutional neural network-based machine learning flare identification method with traditional flare detection techniques, we have obtained a flare sample consisting of 208,280 flare events from 29,280 flare stars. In our flare events sample, flares with rise times within 10 minutes and decay times within 50 minutes account for more than 90% of the total number of flares. The proportion of flare stars is higher in binaries, the main sequence, and stars with KM spectral types compared to single stars, giants, and stars with spectral types other than KM. The fitted {alpha} index results for the flare frequency distributions across different evolutionary stages indicate a general trend of decreasing {alpha} index from main-sequence stars to giants. Except for M-type stars, the {alpha} index also gradually decreases from K-type to O-type stars. Using the flare QPP identification method, based on the fully convolutional networks published by previous researchers, we have also identified flare events with QPP, and through flare parameter constraints, we selected 10,465 flares with QPP features from M-type stars and qualitatively investigated their correlations with stellar parameters.</description><source format="bibcode">2025ApJS..281...52W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/281/52</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/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/139/555">J/A+AS/139/555 : Catalogue and Bibliography of UV Cet stars (Gershberg+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/649">J/ApJ/699/649 : Young M dwarfs within 25pc. 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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>Nfl</name><description>Number of flares for this star (link to Table 2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>TIC</name><description>[101/10005000540] TESS identifier</description><ucd>meta.id;meta.main</ucd><flag>primary</flag></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>TESSmag</name><description>[-1.8/21] TESS apparent magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[2578.6/75050]? Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(g)</name><description>[-0.5/6.6]? Log of surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Period</name><description>[0/25960]? Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Dist</name><description>[1.3/34785]? 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Contamination ratio provided by TESS Input Catalogue</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/281/52/table2</name><description>Parameters of flare events sourced from 29280 stars from TESS sample</description><column><name>TIC</name><description>[11182/2055585779] TESS identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>QPP-per</name><description>[29.3/299]? QPP period</description><unit>s</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_QPP-per</name><description>[0/127]? Uncertainty in QPP-period</description><unit>s</unit><ucd>stat.error;time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>QPP-eye</name><description>[0/1] QPP sample checked by eye (labeled with 1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>Sector</name><description>[1/74] TESS sector</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Begin</name><description>[1325.3/3339.49] Flare start time from BJD2457000</description><unit>d</unit><ucd>time.epoch;time.start</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Peak</name><description>[1325.3/3339.49] Flare peak time from BJD2457000</description><unit>d</unit><ucd>time.epoch;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>End</name><description>[1325.31/3339.52] Flare end time from BJD2457000</description><unit>d</unit><ucd>time.epoch;time.end</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dur</name><description>[7.99/8684.1] Flare duration</description><unit>min</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Amp</name><description>[0.0009/2718.4] Flare amplitude</description><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ebol</name><description>[3.5e+29/1.3e+40]? Bolometric flare energy; in erg units</description><unit>1e-07J</unit><ucd>phot.flux.bol;em.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>ED</name><description>[-242.2/6685232]? Equivalent Duration</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>QPP-prob</name><description>[7.26e-05/1]? Quasiperiodic pulsation (QPP) confidence predicted by FCN model</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>