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<ri:Resource created="2021-10-04T08:12:34Z" 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>Zwicky Transient Facility BTS. I.</title><shortName>J/ApJ/895/32</shortName><identifier>ivo://CDS.VizieR/J/ApJ/895/32</identifier><altIdentifier>doi:10.26093/cds/vizier.18950032</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fremling C.</name></creator><creator><name>Miller A.A.</name></creator><creator><name>Sharma Y.</name></creator><creator><name>Dugas A.</name></creator><creator><name>Perley D.A.</name></creator><creator><name>Taggart K.,Sollerman J.</name></creator><creator><name>Goobar A.</name></creator><creator><name>Graham M.L.</name></creator><creator><name>Neill J.D.</name></creator><creator><name>Nordin J.</name></creator><creator><name>Rigault M.,Walters R.</name></creator><creator><name>Andreoni I.</name></creator><creator><name>Bagdasaryan A.</name></creator><creator><name>Belicki J.</name></creator><creator><name>Cannella C.,Bellm E.C.</name></creator><creator><name>Cenko S.B.</name></creator><creator><name>De K.</name></creator><creator><name>Dekany R.</name></creator><creator><name>Frederick S.</name></creator><creator><name>Golkhou V.Z.,Graham M.J.</name></creator><creator><name>Helou G.</name></creator><creator><name>Ho A.Y.Q.</name></creator><creator><name>Kasliwal M.M.</name></creator><creator><name>Kupfer T.</name></creator><creator><name>Laher R.R.,Mahabal A.</name></creator><creator><name>Masci F.J.</name></creator><creator><name>Riddle R.</name></creator><creator><name>Rusholme B.</name></creator><creator><name>Schulze S.</name></creator><creator><name>Shupe D.L.,Smith R.M.</name></creator><creator><name>Van Velzen S.</name></creator><creator><name>Yan L.</name></creator><creator><name>Yao Y.</name></creator><creator><name>Zhuang Z.</name></creator><creator><name>Kulkarni S.R.</name></creator><date role="Updated">2022-03-16T12:25:08Z</date><date role="Created">2021-10-04T08:12:34Z</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>galaxies</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>redshifted</subject><description>The Zwicky Transient Facility (ZTF) is performing a three-day cadence survey of the visible northern sky (~3{pi}) with newly found transient candidates announced via public alerts. The ZTF Bright Transient Survey (BTS) is a large spectroscopic campaign to complement the photometric survey. BTS endeavors to spectroscopically classify all extragalactic transients with m_peak_&lt;~18.5mag in either the g_ZTF_ or r_ZTF_ filters, and publicly announce said classifications. BTS discoveries are predominantly supernovae (SNe), making this the largest flux-limited SN survey to date. Here we present a catalog of 761 SNe, classified during the first nine months of ZTF (2018 April 1-2018 December 31). We report BTS SN redshifts from SN template matching and spectroscopic host-galaxy redshifts when available. We analyze the redshift completeness of local galaxy catalogs, the redshift completeness fraction (RCF; the ratio of SN host galaxies with known spectroscopic redshift prior to SN discovery to the total number of SN hosts). Of the 512 host galaxies with SNe Ia, 227 had previously known spectroscopic redshifts, yielding an RCF estimate of 44%{+/-}4%. The RCF decreases with increasing distance and decreasing galaxy luminosity (for z&lt;0.05, or ~200Mpc, RCF~0.6). Prospects for dramatically increasing the RCF are limited to new multifiber spectroscopic instruments or wide-field narrowband surveys. Existing galaxy redshift catalogs are only ~50% complete at r~16.9mag. Pushing this limit several magnitudes deeper will pay huge dividends when searching for electromagnetic counterparts to gravitational wave events or sources of ultra-high-energy cosmic rays or neutrinos.</description><source format="bibcode">2020ApJ...895...32F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/895/32</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/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</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/886/152">J/ApJ/886/152 : ZTF early observations of Type Ia SNe. I. 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Observed time, maximum brightness, g-band, JD-2458000 (4)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>gmag</name><description>[13.9/20.6]? g-ZTF band magnitude, maximum brightness (4)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_gmag</name><description>[0.01/0.3]? Uncertainty in gmag (4)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>JDr</name><description>[214/706]? 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