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<ri:Resource created="2023-04-04T10:17:28Z" status="active" updated="2025-06-13T15:25:00Z" 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>Fast-transients confirmed by ZTFReST &amp; LCs</title><shortName>J/ApJ/918/63</shortName><identifier>ivo://CDS.VizieR/J/ApJ/918/63</identifier><altIdentifier>doi:10.26093/cds/vizier.19180063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andreoni I.</name></creator><creator><name>Coughlin M.W.</name></creator><creator><name>Kool E.C.</name></creator><creator><name>Kasliwal M.M.</name></creator><creator><name>Kumar H.,Bhalerao V.</name></creator><creator><name>Carracedo A.S.</name></creator><creator><name>Ho A.Y.Q.</name></creator><creator><name>Pang P.T.H.</name></creator><creator><name>Saraogi D.</name></creator><creator><name>Sharma K.,Shenoy V.</name></creator><creator><name>Burns E.</name></creator><creator><name>Ahumada T.</name></creator><creator><name>Anand S.</name></creator><creator><name>Singer L.P.</name></creator><creator><name>Perley D.A.</name></creator><creator><name>De K.,Fremling U.C.</name></creator><creator><name>Bellm E.C.</name></creator><creator><name>Bulla M.</name></creator><creator><name>Crellin-quick A.</name></creator><creator><name>Dietrich T.,Drake A.</name></creator><creator><name>Duev D.A.</name></creator><creator><name>Goobar A.</name></creator><creator><name>Graham M.J.</name></creator><creator><name>Kaplan D.L.</name></creator><creator><name>Kulkarni S.R.,Laher R.R.</name></creator><creator><name>Mahabal A.A.</name></creator><creator><name>Shupe D.L.</name></creator><creator><name>Sollerman J.</name></creator><creator><name>Walters R.</name></creator><creator><name>Yao Y.</name></creator><date role="Updated">2023-06-15T09:24:59Z</date><date role="Created">2023-04-04T10:17:28Z</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>photometry</subject><subject>visible-astronomy</subject><subject>redshifted</subject><subject>gamma-ray-astronomy</subject><subject>gamma-ray-bursts</subject><subject>novae</subject><subject>transient-sources</subject><description>The most common way to discover extragalactic fast transients, which fade within a few nights in the optical, is via follow-up of gamma-ray burst and gravitational-wave triggers. However, wide-field surveys have the potential to identify rapidly fading transients independently of such external triggers. The volumetric survey speed of the Zwicky Transient Facility (ZTF) makes it sensitive to objects as faint and fast fading as kilonovae, the optical counterparts to binary neutron star mergers, out to almost 200 Mpc. We introduce an open-source software infrastructure, the ZTF REaltime Search and Triggering, ZTFReST, designed to identify kilonovae and fast transients in ZTF data. Using the ZTF alert stream combined with forced point-spread-function photometry, we have implemented automated candidate ranking based on their photometric evolution and fitting to kilonova models. Automated triggering, with a human in the loop for monitoring, of follow-up systems has also been implemented. In 13 months of science validation, we found several extragalactic fast transients independently of any external trigger, including two supernovae with post-shock cooling emission, two known afterglows with an associated gamma-ray burst (ZTF20abbiixp, ZTF20abwysqy), two known afterglows without any known gamma-ray counterpart (ZTF20aajnksq, ZTF21aaeyldq), and three new fast-declining sources (ZTF20abtxwfx, ZTF20acozryr, ZTF21aagwbjr) that are likely associated with GRB200817A, GRB201103B, and GRB210204A. However, we have not found any objects that appear to be kilonovae. We constrain the rate of GW170817-like kilonovae to R&lt;900Gpc^-3^/yr (95% confidence). A framework such as ZTFReST could become a prime tool for kilonova and fast-transient discovery with the Vera Rubin Observatory.</description><source format="bibcode">2021ApJ...918...63A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/918/63</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/281">VII/281 : GLADE v2.3 catalog (Dalya+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/156">J/ApJ/746/156 : Radio afterglow observations of GRBs (Chandra+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/200/8">J/ApJS/200/8 : AGES: the AGN and Galaxy Evolution Survey (Kochanek+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/52">J/ApJ/806/52 : 8 Fermi GRB afterglows follow-up (Singer+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/110">J/ApJ/818/110 : Short GRBs with Fermi GBM and Swift BAT (Burns+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/828/36">J/ApJ/828/36 : GRB light-curve decay indices with Swift (Del Vecchio+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/593/A68">J/A+A/593/A68 : PTF12os &amp; iPTF13bvn spectra and light curves (Fremling+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/L29">J/ApJ/848/L29 : Opt. follow-up of GW170817 counterpart (Diaz+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/880/7">J/ApJ/880/7 : The Local Universe survey. 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