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<ri:Resource created="2026-01-07T12:52:51Z" status="active" updated="2026-07-02T12:00:45Z" 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>LCs of 9 rapidly evolving transients</title><shortName>J/ApJ/955/144</shortName><identifier>ivo://CDS.VizieR/J/ApJ/955/144</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xv-4g</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li W.</name></creator><creator><name>Arcavi I.</name></creator><creator><name>Nakar E.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Brink T.G.</name></creator><creator><name>Zheng W.,Yang Yi</name></creator><creator><name>Lam M.C.</name></creator><creator><name>Keinan I.</name></creator><creator><name>Brennan S.J.</name></creator><creator><name>Shitrit N.</name></creator><date role="Updated">2026-07-02T12:00:45Z</date><date role="Created">2026-01-07T12:52:51Z</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>transient-sources</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>We search the archival Zwicky Transient Facility public survey for rapidly evolving transient (RET) candidates based on well-defined criteria between 2018 May and 2021 December. The search yielded 19 bona fide RET candidates, corresponding to a discovery rate of ~5.2 events per year. Even with a Galactic latitude cut of 20{deg}, eight of the 19 events (~42%) are Galactic, including one with a light-curve shape closely resembling that of the GW170817 kilonova (KN). An additional event is a nova in M31. Four out of the 19 events (~21%) are confirmed extragalactic RETs (one confirmed here for the first time) and the origin of six additional events cannot be determined. We did not find any extragalactic events resembling the GW170817 KN, from which we obtain an upper limit on the volumetric rate of GW170817-like KNe of R&lt;=2400Gpc^-3^/yr (95% confidence). These results can be used for quantifying contaminants to RET searches in transient alert streams, specifically when searching for KNe independently of gravitational-wave and gamma-ray-burst triggers.</description><source format="bibcode">2023ApJ...955..144L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/955/144</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/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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