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<ri:Resource created="2022-07-27T12:30:53Z" status="active" updated="2026-01-13T14:27:05Z" 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>TESS early light curves of type Ia Supernovae</title><shortName>J/ApJ/908/51</shortName><identifier>ivo://CDS.VizieR/J/ApJ/908/51</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fausnaugh M.M.</name></creator><creator><name>Vallely P.J.</name></creator><creator><name>Kochanek C.S.</name></creator><creator><name>Shappee B.J.</name></creator><creator><name>Stanek K.Z.,Tucker M.A.</name></creator><creator><name>Ricker G.R.</name></creator><creator><name>Vanderspek R.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Seager S.</name></creator><creator><name>Winn J.N.,Jenkins J.M.</name></creator><creator><name>Berta-Thompson Z.K.</name></creator><creator><name>Daylan T.</name></creator><creator><name>Doty J.P.</name></creator><creator><name>Furesz G.,Levine A.M.</name></creator><creator><name>Morris R.</name></creator><creator><name>Pal A.</name></creator><creator><name>Sha L.</name></creator><creator><name>Ting E.B.</name></creator><creator><name>Wohler B.</name></creator><date role="Updated">2026-01-13T14:27:05Z</date><date role="Created">2022-07-27T12:30:53Z</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>supernovae</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>We present the early-time light curves of Type Ia supernovae (SNeIa) observed in the first six sectors of Transiting Exoplanet Survey Satellite (TESS) data. Ten of these SNe were discovered by ASAS-SN, seven by ATLAS, six by ZTF, and one by Gaia. For nine of these objects with sufficient dynamic range (&gt;3.0mag from detection to peak), we fit power-law models and searched for signatures of companion stars. We found a diversity of early-time light-curve shapes, although most of our sources are consistent with fireball models where the flux increases as {prop}t2. Three SNe displayed a flatter rise with flux {prop}t. We did not find any obvious evidence for additional structures, such as multiple power-law components, in the early rising light curves. For assumptions about the SN properties and the observer viewing angle (ejecta mass of 1.4M{sun}, expansion velocity of 104km/s, opacity of 0.2cm^2^/g, and viewing angle of 45{deg}) and a further assumption that any companion stars would be in Roche lobe overflow, it is possible to place upper limits on the radii of any companion stars. Six of the nine SNe had complete coverage of the early-time light curves, and we placed upper limits on the radii of companion stars of &lt;~32R{sun} for these SNe, &lt;~20R{sun} for five of the six, and &lt;~4R{sun} for two of the six. The small sample size did not allow us to put limits on the occurrence rate of companion stars in the progenitors of SNe Ia. However, we expect that TESS observed enough SNe in its two-year primary mission (26 sectors) to either detect the signature of a large companion (R&gt;20R{sun}) or constrain the occurrence rate of such systems, at least for the fiducial SN properties adopted here. We also show that TESS is capable of detecting emission from a 1R{sun} companion for an SN Ia within 50Mpc and has a reasonable chance of doing so after about six years.</description><source format="bibcode">2021ApJ...908...51F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/908/51</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/48">J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/446/3895">J/MNRAS/446/3895 : The rising light curves of Type Ia supernovae (Firth+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/105">J/ApJ/799/105 : KELT light curve of the M82 SN 2014J (Siverd+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/853/62">J/ApJ/853/62 : Optical and NIR spectra and LCs of SN2016ija (Tartaglia+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/L1">J/ApJ/870/L1 : K2 observations type Ia supernova SN2018oh (Dimitriadis+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/111">J/ApJ/883/111 : UV-Opt LCs of ASASSN-19bt detected by TESS (Holoien+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/13">J/ApJ/870/13 : K2 light curve analysis of ASASSN-18bt (Shappee+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/886/152">J/ApJ/886/152 : ZTF early observations of Type Ia SNe. 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Luminosity</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>z</name><description>[0.01/0.09] Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>[0.005/0.3] E(B-V) color</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Discov</name><description>Discorvery reference</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Class</name><description>Classification reference</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Note1</name><description>X = fit with a power law to characterize the early light curve (see section 4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Note2</name><description>X = searched for signatures of companion stars (section 5)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Note3</name><description>X = flux calibrated across two sectors using a joint fit to both data sets (section 3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Note4</name><description>X = near strong scattered light backgrounds at the time of first light</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Note5</name><description>X = affected by pixels with enhanced sensitivity from "straps"</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Note6</name><description>X = near bright stars and required detrending</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Nobs</name><description>Number of observations for the light curve</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>LC</name><description>Interactive Plot</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column></table><table><name>J/ApJ/908/51/table2</name><description>TESS supernova light curves</description><column><name>SN</name><description>Supernova identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Flux</name><description>[-30/168] Observed flux</description><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>[0.8/5] Uncertainty in Flux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Asteroid</name><description>[0/1] Asteroid flag (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>TNS</name><description>Discovery survey identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>BJD</name><description>[1325/1491] Barycentric Julian Date JD-2457000.0</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column></table><table><name>J/ApJ/908/51/table5</name><description>*TESS light curves</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>Time</name><description>[0.001/17] Time since explosion</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux50</name><description>[0.006/21.7] 50R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag50</name><description>[17/25.9] 50R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux25</name><description>[0.005/12.9] 25R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag25</name><description>[17.6/26.1] 25R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux10</name><description>[0.004/6.42] 10R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag10</name><description>[18.4/26.3] 10R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux5</name><description>[0.003/3.78] 5R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag5</name><description>[18.9/26.5] 5R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux1</name><description>[0.002/1.13] 1R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag1</name><description>[20.3/27] 1R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux0.5</name><description>[0.002/0.67] 0.5R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag0.5</name><description>[20.8/27.2] 0.5R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux0.1</name><description>[0.0004/0.2] 0.1R* companion model flux</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag0.1</name><description>[22.2/28.9] 0.1R* companion model apparent magnitude</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/908/51/refs</name><description>References used for table1</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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