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<ri:Resource created="2018-03-23T12:40:24Z" 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>White dwarf candidates in DECam first field</title><shortName>J/MNRAS/462/2506</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/462/2506</identifier><altIdentifier>doi:10.26093/cds/vizier.74622506</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Belardi C.</name></creator><creator><name>Kilic M.</name></creator><creator><name>Munn J.A.</name></creator><creator><name>Gianninas A.</name></creator><creator><name>Barber S.D.</name></creator><creator><name>Dey A.,Stetson P.B.</name></creator><date role="Updated">2024-08-16T20:18:22Z</date><date role="Created">2018-03-23T12:40:24Z</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>surveys</subject><subject>white-dwarf-stars</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>stellar-ages</subject><subject>stellar-distance</subject><description>We present the first results from a minute cadence survey of a 3deg^2^ field obtained with the Dark Energy Camera. We imaged part of the Canada-France-Hawaii Telescope Legacy Survey area over eight half-nights. We use the stacked images to identify 111 high proper motion white dwarf candidates with g&lt;=24.5mag and search for eclipse-like events and other sources of variability. We find a new g=20.64mag pulsating ZZ Ceti star with pulsation periods of 11-13min. However, we do not find any transiting planetary companions in the habitable zone of our target white dwarfs. Given the probability of eclipses of 1 per cent and our observing window from the ground, the non-detection of such companions in this first field is not surprising. 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