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<ri:Resource created="2014-03-21T14:18:15Z" 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>Rapid optical variability in ultracool dwarfs</title><shortName>J/MNRAS/428/2824</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/428/2824</identifier><altIdentifier>doi:10.26093/cds/vizier.74282824</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Koen C.</name></creator><date role="Updated">2024-07-20T20:13:26Z</date><date role="Created">2014-03-21T14:18:15Z</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>dwarf-stars</subject><subject>photometry</subject><description>In this paper, a summary of optical time-series photometry of 125 ultracool dwarfs is given. The observing strategy was to monitor each object continuously for 2-3h in order to ascertain whether it was rapidly variable. Many of the targets were observed at multiple epochs, to follow up possible short time-scale variability, or to test for slow brightness changes on longer time-scales. The 353 data sets obtained contain nearly 22000 individual measurements. Optical (I_C_) magnitudes, accurate to roughly 0.1-0.2mag, were derived for 21 objects for which there is no optical photometry in the literature. It is shown that photometry is affected by variable seeing in a large percentage of the time-series observations. Since this could give the appearance of variability intrinsic to the objects, magnitudes are modelled as functions of both time and seeing. Several ultracool dwarfs which had not been monitored before are variable, according to certain model-fitting criteria. A number of objects with multi-epoch observations appear to be variable on longer time-scales. Since testing for variability is far from being straightforward, the time-series data are made available so that interested readers can perform their own analyses.</description><source format="bibcode">2013MNRAS.428.2824K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/428/2824</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/J/AJ/126/1526">J/AJ/126/1526 : IR photometry of ultracool dwarfs (Bouy+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2421">J/AJ/126/2421 : 2MASS-Selected sample of ultracool dwarfs (Cruz+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2449">J/AJ/126/2449 : Nearby ultracool dwarfs in galactic plane (Reid+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/446/515">J/A+A/446/515 : Distances of nearby ultracool dwarfs (Phan-Bao+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/382/515">J/MNRAS/382/515 : SDSS ultracool and halo WD candidates (Vidrih+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/439">J/AJ/133/439 : Luminosity function of M7-L8 ultracool dwarfs (Cruz+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2258">J/AJ/133/2258 : Activity and kinematics of ultracool dwarfs (Schmidt+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1290">J/AJ/136/1290 : Ultracool dwarfs from the 2MASS (Reid+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/684">J/ApJ/723/684 : NIRSPEC ultracool dwarf RV survey (Blake+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/404/1817">J/MNRAS/404/1817 : 2MASS/SDSS data for 806 ultracool dwarfs (Zhang+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/522/A112">J/A+A/522/A112 : L5 and later dwarf candidates i'z' photometry (Reyle+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/23">J/ApJ/746/23 : Radio observations of ultracool dwarf stars (McLean+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A131">J/A+A/549/A131 : Radio survey of ultracool dwarfs (Antonova+, 2013)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/428/2824</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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