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<ri:Resource created="2024-04-22T07:09:32Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Ha emission from FU Tau B brown dwarf companion</title><shortName>J/AJ/166/143</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/143</identifier><altIdentifier>doi:10.26093/cds/vizier.51660143</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wu Y.-L.</name></creator><creator><name>Cheng Y.-C.</name></creator><creator><name>Huang L.-C.</name></creator><creator><name>Bowler B.P.</name></creator><creator><name>Close L.M.</name></creator><creator><name>Tseng W.-L.,Chen N.</name></creator><creator><name>Chen D.-W.</name></creator><date role="Updated">2024-11-06T20:17:48Z</date><date role="Created">2024-04-22T07:09:32Z</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>exoplanets</subject><subject>brown-dwarfs</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><description>Monitoring mass accretion onto substellar objects provides insights into the geometry of the accretion flows. We use the Lulin One-meter Telescope to monitor H{alpha} emission from FUTauB, a ~19MJup brown-dwarf companion at 5.7" (719au) from the host star, for six consecutive nights. This is the longest continuous H{alpha} monitoring for a substellar companion near the deuterium-burning limit. We aim to investigate if accretion near the planetary regime could be rotationally modulated as suggested by magnetospheric accretion models. We find tentative evidence that H{alpha} mildly varies on hourly and daily timescales, though our sensitivity is not sufficient to definitively establish any rotational modulation. No burst-like events are detected, implying that accretion onto FUTauB is overall stable during the time baseline and sampling windows over which it was observed. The primary star FUTauA also exhibits H{alpha} variations over timescales from minutes to days. This program highlights the potential of monitoring accretion onto substellar objects with small telescopes.</description><source format="bibcode">2023AJ....166..143W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/143</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances 1.47 billion stars Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/349/619">J/A+A/349/619 : UBVRI light curves of AA Tau in 1995 (Bouvier+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/548/A56">J/A+A/548/A56 : X-shooter spectra 12 young stellar objects (Rigliaco+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A107">J/A+A/551/A107 : X-shooter spectra of 24 young stellar objects (Manara+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/82">J/AJ/147/82 : Monitoring of disk-bearing stars in NGC 2264 (Cody+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/40">J/ApJ/788/40 : Late-type targets in Taurus, Cha I &amp; UpperSco (Todorov+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/605/A86">J/A+A/605/A86 : Pre-main sequence stars VLT/X-Shooter spectra (Manara+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/71">J/AJ/156/71 : K2 Campaign2 young disk-bearing stars in Sco&amp;Oph (Cody+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/164">J/AJ/165/164 : Tull RVels, rotation periods and Inclinations (Bowler+, 2023)</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/AJ/166/143</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/166/143</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/166/143</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/166/143</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/166/143</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/166/143</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/166/143/table2</name><description>Relative photometry between FU Tau A and 2MASS J04241447+2506106</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HJD</name><description>Heliocentric Julian date at exposure midpoint</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dmag</name><description>Magnitude difference at H{alpha}</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dmag</name><description>Uncertainty in dmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/166/143/table3</name><description>Relative photometry between FU Tau B and 2MASS J04241447+2506106</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HJD</name><description>Heliocentric Julian date at exposure midpoint</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dmag</name><description>Magnitude difference at H{alpha}</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dmag</name><description>Uncertainty in dmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>