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<ri:Resource created="2025-06-16T14:36:46Z" status="active" updated="2026-08-03T07:31:22Z" 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 detections of TOI host stars</title><shortName>J/MNRAS/512/L60</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/512/L60</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-g0/wga</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Howard W.S.</name></creator><date role="Updated">2026-08-03T07:31:22Z</date><date role="Created">2025-06-16T14:36:46Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>stellar-flares</subject><subject>stellar-atmospheres</subject><subject>transient-sources</subject><subject>orbits</subject><subject>astronomical-object-identification</subject><subject>astrometry</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>stellar-distance</subject><subject>stellar-masses</subject><description>Although more than 5000 TESS Objects of Interest have been catalogued, no comprehensive survey of the flare rates of their host stars exists. We perform the first flare survey of all 2250 non-retired TOIs with 2-min cadence light curves to measure or place upper limits on their flare rates. We find 93 candidates orbit flare stars and measure their flare frequency distributions. Across the sample, TOIs of &lt;= 1.5R_{Earth}_ orbit flare stars more frequently than do TOIs of 1.5 &lt; R &lt; 2.75R_{Earth}_, 2.75 &lt; R&lt; 4R_{Earth}_, or R =&gt; 4R_{Earth}_. We sort all TOI host stars by their flare rate/upper limit, stellar mass, and distance to create a flare ranking metric (FRM) to determine suitability for follow-up. The FRM of each TOI is then checked against the expected signal-to-noise of atmospheric features in transmission spectroscopy to locate the most promising targets. We find 1/4 of terrestrial M-dwarf planets amenable to transmission spectroscopy orbit flare stars. However, none of the M-dwarf hosts to terrestrial planets are currently flaring at sufficient levels for &gt; 99.9 per cent atmospheric ozone depletion. We give the first upper limits on the flare rate of the host star to TOI 700 d and explore the flare rates incident on young planets such as DS Tuc Ab.</description><source format="bibcode">2022MNRAS.512L..60H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/512/L60</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/J/ApJS/254/39">J/ApJS/254/39 : Exoplanet candidates from TESS first 2yr obs (Guerrero+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/926/204">J/ApJ/926/204 : TESS monitoring campaign of low-mass flare stars (Howard+,2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/623/A72">J/A+A/623/A72 : Binarity of Hipparcos stars from Gaia pm anomaly</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/188">J/AJ/160/188 : Spectroscopic transit depths of LHS 3844b (Diamond-Lowe+, 2020)</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/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2</relatedResource><relatedResource>https://exofop.ipac.caltech.edu/tess/ : ExoFOP data</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>TOI</name><description>TESS Objects of Interest identifier number (TOI)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rp</name><description>Planet radius (planet_radius_Re) (1)</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rp</name><description>? Mean uncertainty of Rp (e_planet_radius_Re)</description><unit>(6.3781x10+6m)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Orb</name><description>? Planet orbital distance (orb_dist_au)</description><unit>au</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Orb</name><description>? Mean uncertainty of Orb (e_orb_dist_au)</description><unit>au</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Per</name><description>? Planet orbital period (orb_period_d) (2)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Per</name><description>? Mean uncertainty of Per (e_orb_period_d)</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Priority</name><description>TOI flare order of priority from 1 to 5 ranks (master_priority)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TIC</name><description>TESS input catalog identifier (TICID)</description><ucd>meta.id</ucd></column><column><name>Bin</name><description>Binary flag takes whether 2 for 2167 sources or 3 for 83 sources (table_bool) (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GaiaDR2</name><description>Gaia DR2 unique identifier number (GAIA_ID)</description><ucd>meta.id.assoc</ucd></column><column><name>RA_ICRS</name><description>Barycentric right ascension (ICRS) at Ep=2015.5 (coord_RA)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Barycentric declination (ICRS) at Ep=2015.5 (coord_Dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Tmag</name><description>TESS magnitude from TIC Stassun et al. 2019AJ....158..138S, Cat. IV/38 (Tmags)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>D*</name><description>? Stellar distance from TIC Stassun et al. 2019AJ....158..138S, Cat. IV/38 (stellar_distance_pc)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_D*</name><description>[0/1] Stellar distance availability flag, 0 for 2246 sources and 1 for 4 sources (stellar_distance_bool)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M*</name><description>? Stellar mass from TIC Stassun et al. 2019AJ....158..138S, Cat. IV/38 (stellar_mass)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_M*</name><description>Mean uncertainty of M* (e_stellar_mass)</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Binarity</name><description>Binarity boolean takes whether 0 for 2212 sources or 1 for 38 sources (binarity_bool) (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Contam</name><description>Flag which tags source contamination is likely present, takes 0 for 2079 sources or 1 for 171 sources (contam_bool)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ExpBin</name><description>Exposed binarity boolean takes whether 0 for 2247 sources or 1 for 3 sources (expbinarity_bool)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Obs</name><description>Observation time (obs_time_d)</description><unit>s</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nfl</name><description>Number of flares observed (N_flares)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EminU</name><description>Smallest energy flare used to detect flares (MinUse_Erg)</description><unit>1e-07J</unit><ucd>phys.energy;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Emin100</name><description>Smallest energy flare that would be recovered 100 per cent of the time (MinCompl_Erg)</description><unit>1e-07J</unit><ucd>phys.energy;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EDU</name><description>Smallest the equivalent duration used for detection of each flare obtained by integrating the fractional flux between the start and stop times in seconds (MinUse_ED)</description><unit>s</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ED100</name><description>Smallest the equivalent duration would be recovered 100 per cent of the time (MinCompl_ED)</description><unit>s</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ED</name><description>The equivalent duration flare rate (ED_flare_rate)</description><unit>yr**-1</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>1-alpha</name><description>Fit parameter 1-{alpha} from flare frequency distribution FFD computations (one_min_alpha_ffd) (5)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_1-alpha</name><description>? Lower uncertainty of 1-{alpha} from 1{sigma} confidence interval (e_one_min_alpha_ffd)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_1-alpha</name><description>? Upper uncertainty of 1-{alpha} from 1{sigma} confidence interval (E_one_min_alpha_ffd)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>beta</name><description>Fit parameter {beta} from flare frequency distribution FFD computations (beta_ffd) (5)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_beta</name><description>? Lower uncertainty of {beta} from 1{sigma} confidence interval (e_beta_ffd)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_beta</name><description>? Upper uncertainty of {beta} from 1{sigma} confidence interval (E_beta_ffd)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nsuper</name><description>The superflare rate number for energy flare equal or greater than 10^34^ erg (superflare_rate)</description><unit>yr**-1</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Nsuper</name><description>? Lower uncertainty of Nsuper from 1{sigma} confidence interval (e_superflare_rate)</description><unit>yr**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_Nsuper</name><description>? Upper uncertainty of Nsuper from 1{sigma} confidence interval (E_superflare_rate)</description><unit>yr**-1</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FRM</name></column></table></schema></tableset></ri:Resource>