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<ri:Resource created="2024-12-30T09:10:49Z" 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>LCs and sp. of 30 ZTF TDEs</title><shortName>J/ApJ/942/9</shortName><identifier>ivo://CDS.VizieR/J/ApJ/942/9</identifier><altIdentifier>doi:10.26093/cds/vizier.19420009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hammerstein E.</name></creator><creator><name>van Velzen S.</name></creator><creator><name>Gezari S.</name></creator><creator><name>Cenko S.B.</name></creator><creator><name>Yao Y.</name></creator><creator><name>Ward C.,Frederick S.</name></creator><creator><name>Villanueva N.</name></creator><creator><name>Somalwar J.J.</name></creator><creator><name>Graham M.J.</name></creator><creator><name>Kulkarni S.R.,Stern D.</name></creator><creator><name>Andreoni I.</name></creator><creator><name>Bellm E.C.</name></creator><creator><name>Dekany R.</name></creator><creator><name>Dhawan S.</name></creator><creator><name>Drake A.J.,Fremling C.</name></creator><creator><name>Gatkine P.</name></creator><creator><name>Groom S.L.</name></creator><creator><name>Ho A.Y.Q.</name></creator><creator><name>Kasliwal M.M.,Karambelkar V.</name></creator><creator><name>Kool E.C.</name></creator><creator><name>Masci F.J.</name></creator><creator><name>Medford M.S.</name></creator><creator><name>Perley D.A.,Purdum J.</name></creator><creator><name>van Roestel J.</name></creator><creator><name>Sharma Y.</name></creator><creator><name>Sollerman J.</name></creator><creator><name>Taggart K.</name></creator><creator><name>Yan L.</name></creator><date role="Updated">2025-02-24T20:13:52Z</date><date role="Created">2024-12-30T09:10:49Z</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>black-holes</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>transient-sources</subject><description>Tidal disruption events (TDEs) offer a unique way to study dormant black holes. While the number of observed TDEs has grown thanks to the emergence of wide-field surveys in the past few decades, questions regarding the nature of the observed optical, UV, and X-ray emission remain. We present a uniformly selected sample of 30 spectroscopically classified TDEs from the Zwicky Transient Facility Phase I survey operations with follow-up Swift UV and X-ray observations. Through our investigation into correlations between light-curve properties, we recover a shallow positive correlation between the peak bolometric luminosity and decay timescales. We introduce a new spectroscopic class of TDE, TDE-featureless, which are characterized by featureless optical spectra. The new TDE-featureless class shows larger peak bolometric luminosities, peak blackbody temperatures, and peak blackbody radii. We examine the differences between the X-ray bright and X-ray faint populations of TDEs in this sample, finding that X-ray bright TDEs show higher peak blackbody luminosities than the X-ray faint subsample. This sample of optically selected TDEs is the largest sample of TDEs from a single survey yet, and the systematic discovery, classification, and follow-up of this sample allows for robust characterization of TDE properties, an important stepping stone looking forward toward the Rubin era.</description><source format="bibcode">2023ApJ...942....9H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/942/9</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/273">VII/273 : The Half Million Quasars (HMQ) catalogue (Flesch, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/290">VII/290 : The Million Quasars (Milliquas) catalogue, version 7.2 (Flesch, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/1177">J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/38">J/ApJ/793/38 : Palomar Transient Factory photometric obs. 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