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<ri:Resource created="2026-04-14T15:40:56Z" status="active" updated="2026-04-14T15:02:07Z" 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>ZTF light curves of 29 BTS supernovae</title><shortName>J/ApJ/960/72</shortName><identifier>ivo://CDS.VizieR/J/ApJ/960/72</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Strotjohann N.L.</name></creator><creator><name>Ofek E.O.</name></creator><creator><name>Gal-Yam A.</name></creator><creator><name>Sollerman J.</name></creator><creator><name>Chen P.</name></creator><creator><name>Yaron O.,Zackay B.</name></creator><creator><name>Rehemtulla N.</name></creator><creator><name>Gris P.</name></creator><creator><name>Masci F.J.</name></creator><creator><name>Rusholme B.</name></creator><creator><name>Purdum J.</name></creator><date role="Updated">2026-04-14T15:02:07Z</date><date role="Created">2026-04-14T15:40:56Z</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>photometry</subject><subject>visible-astronomy</subject><subject>surveys</subject><description>The direct detection of core-collapse supernova (SN) progenitor stars is a powerful way of probing the last stages of stellar evolution. However, detections in archival Hubble Space Telescope images are limited to about one detection per year. Here, we explore whether we can increase the detection rate by using data from ground-based wide-field surveys. Due to crowding and atmospheric blurring, progenitor stars can typically not be identified in preexplosion images alone. Instead, we combine many pre-SN and late-time images to search for the disappearance of the progenitor star. As a proof of concept, we implement our search of ZTF data. For a few hundred images, we achieve limiting magnitudes of ~23mag in the g and r bands. However, no progenitor stars or long-lived outbursts are detected for 29 SNe within z&lt;=0.01, and the ZTF limits are typically several magnitudes less constraining than detected progenitors in the literature. Next, we estimate progenitor detection rates for the Legacy Survey of Space and Time (LSST) with the Vera C. Rubin telescope by simulating a population of nearby SNe. The background from bright host galaxies reduces the nominal LSST sensitivity by, on average, 0.4 mag. Over the 10 yr survey, we expect the detection of ~50 red supergiant progenitors and several yellow and blue supergiants. The progenitors of Type Ib and Ic SNe will be detectable if they are brighter than -4.7 or -4.0 mag in the LSST i band, respectively. In addition, we expect the detection of hundreds of pre-SN outbursts depending on their brightness and duration.</description><source format="bibcode">2024ApJ...960...72S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/960/72</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/VII/291">VII/291 : GLADE+ (Galaxy List for the Advanced Detector Era) (Dalya+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/395/1409">J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/412/1441">J/MNRAS/412/1441 : SNe luminosity functions (Li+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/789/104">J/ApJ/789/104 : SNe IIn observations and properties (Ofek+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A142">J/A+A/580/A142 : SN 2011dh. 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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>SN</name><description>IAU identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType><flag>primary</flag></column><column><name>ZTF</name><description>ZTF identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>RAJ2000</name><description>[34/310.5] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-26/71.1] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Type</name><description>Supernova type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>f_Type</name><description>Flag on Type (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Host</name><description>Host galaxy identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">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>JD</name><description>Julian date of the approximate explosion</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>t23</name><description>[305/772] Time after explosion when SN likely faded to 23rd mag in r band</description><unit>d</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dist</name><description>[14.7/44.6] Distance</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_Dist</name><description>[i] No host galaxy redshift available</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_mag</name><description>Limit flag on mag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>mag</name><description>[24.8/28.7]? Detected progenitor magnitude in Band</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_mag</name><description>[0.02/0.07]? Uncertainty in mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Band</name><description>Observation band of progenitor (F555W, F606W, F635W or F814W)</description><ucd>instr.bandpass;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>f_mag</name><description>Flag on mag (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Np</name><description>Number of ZTF measurements for this SN (link to Table 2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>LC</name><description>Interactive LC Plot</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/960/72/table2</name><description>*Unbinned ZTF forced-photometry light curves for 29 nearby SNe</description><column><name>SN</name><description>IAU identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</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>JD</name><description>Julian Date of the observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>Field</name><description>[277/1876] The ZTF field (1)</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CCID</name><description>[1/16] The ZTF CCD ID (1)</description><ucd>meta.id;instr.det</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>QID</name><description>[1/4] The ZTF quadrant ID (1)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Filt</name><description>[1/2] The ZTF filter code (1=g, 2=r) (1)</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flux</name><description>[-452/3060] Observed flux, in 10-9maggy (2)</description><unit>3.63uJy</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[0.04/114] Uncertainty in Flux (2)</description><unit>3.63uJy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>