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<ri:Resource created="2018-12-12T13:23:34Z" 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>Analysis of K2 LCs for members of USco &amp; {rho} Oph</title><shortName>J/AJ/155/196</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/196</identifier><altIdentifier>doi:10.26093/cds/vizier.51550196</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rebull L.M.</name></creator><creator><name>Stauffer J.R.</name></creator><creator><name>Cody A.M.</name></creator><creator><name>Hillenbrand L.A.</name></creator><creator><name>David T.J.,Pinsonneault M.</name></creator><date role="Updated">2019-12-03T07:58:53Z</date><date role="Created">2018-12-12T13:23:34Z</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>stellar-associations</subject><subject>pre-main-sequence-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>infrared-photometry</subject><description>We present an analysis of K2 light curves (LCs) for candidate members of the young Upper Sco (USco) association (~8 Myr) and the neighboring {rho} Oph embedded cluster (~1 Myr). We establish ~1300 stars as probable members, ~80% of which are periodic. The phased LCs have a variety of shapes which can be attributed to physical causes ranging from stellar pulsation and stellar rotation to disk-related phenomena. We identify and discuss a number of observed behaviors. The periods are ~0.2-30 days with a peak near 2 days and the rapid period end nearing breakup velocity. M stars in the young USco region rotate systematically faster than GK stars, a pattern also present in K2 data for the older Pleiades and Praesepe systems. At higher masses (types FGK), the well-defined period-color relationship for slowly rotating stars seen in the Pleiades and Praesepe systems is not yet present in USco. Circumstellar disks are present predominantly among the more slowly rotating M stars in USco, with few disks in the subday rotators. However, M dwarfs with disks rotate faster on average than FGK systems with disks. For four of these disked M dwarfs, we provide direct evidence for disk locking based on the K2 LC morphologies. Our preliminary analysis shows a relatively mass-independent spin-up by a factor of ~3.5 between USco and the Pleiades, then mass-dependent spin-down between Pleiades and Praesepe.</description><source format="bibcode">2018AJ....155..196R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/196</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/II/240">II/240 : The DENIS database first release (Epchtein+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/336">II/336 : AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/479">J/AJ/120/479 : Low-mass stars in the Upper Sco association (Ardila+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/1040">J/AJ/121/1040 : PMS members of upper Scorpius OB association</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/404">J/AJ/124/404 : Upper Scorpius OB association Lithium survey. II.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/630/381">J/ApJ/630/381 : Mid-IR imaging in {rho} Oph (Barsony+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/3016">J/AJ/131/3016 : Low-mass objects in Upper Scorpius (Slesnick+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/651/L49">J/ApJ/651/L49 : Upper Sco OB association IRAC observations</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/688/377">J/ApJ/688/377 : Low-mass objects in Upper Scorpius. II. (Slesnick+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1646">J/ApJ/705/1646 : Debris disks in Upper Sco (Carpenter+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A24">J/A+A/527/A24 : Spectra of low-mass stars in Upper Sco (Lodieu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/140">J/AJ/142/140 : Optical spectroscopy of {rho} Oph stars. II.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/31">J/ApJ/758/31 : IR photometry for members of Upper Sco (Luhman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/448/2737">J/MNRAS/448/2737 : New PMS K/M Stars in Upper Scorpius (Rizzuto+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/113">J/AJ/152/113 : Pleiades members with K2 light curves. I. Periods</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/114">J/AJ/152/114 : Pleiades members with K2 light curves. II. (Rebull+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/115">J/AJ/152/115 : Pleiades members with K2 light curves. III.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/256">J/AJ/154/256 : VLM stars and BDs in Upper Sco using Gaia DR1 (Cook+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/839/92">J/ApJ/839/92 : Praesepe members with K2 light curve data (Rebull+, 2017)</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/155/196</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/196</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/196</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/155/196</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/155/196</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/155/196</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/155/196/table1 (Periods and supporting data for USco and {rho} Oph members with K2 light curves)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/196/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/196/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/196/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>238.6637917</ra><dec>-22.28375</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/155/196/table3 (Periods and supporting data for USco and {rho} Oph non-members with K2 light curves)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/196/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/196/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/196/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>238.6232083</ra><dec>-20.3455278</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>4/1920 2686 2687 2772 5/7336 7337 7338 10715 10727 10733 10735 10736 10737 10738 10741 11077 11079 11092 11093 11094 11096 11097 11100 11101 6/29226 29312 29314 29327 29357 29358 29359 29360 29362 29363 29368 30736 30738 30744 30752 30753 30754 42859 42874 42877 42878 42879 42903 42905 42906 42907 42928 42929 42931 42937 42938 42939 42956 42958 42959 42960 42971 42974 42975 44304 44305 44307 44313 44341 44380 44381 44383 44393 44396 44409 44412 44413 44414</spatial><spectral>7.952274030004205e-20 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/155/196?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/155/196/table1</name><description>Periods and supporting data for USco and {rho} Oph members with K2 light curves</description><column><name>RDist</name><description>[yes no] Resolved distant periods? 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Adopted (V-K_s_) color excess (see Section 2.4)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ksmag0</name><description>[2.1/16.66]? Dereddened K_s_ band Vega magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(V-Ks)0</name><description>[-1.03/9.8]? Dereddened (V-K_s_) color (2)</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_(V-Ks)</name><description>[-9/6] Note on (V-K_s_) (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_(V-Ks)0</name><description>[-9/3] Note on (V-K_s_)_0_ (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Per1</name><description>[0.0476/38.3933]? Primary period (taken to be the rotation period, see text)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Per2</name><description>[0.0458/23.9255]? 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(maybe, yes or no)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>DStart</name><description>Wavelength of start of IR excess (6)</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Multi</name><description>Single or multi-period star</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>DD</name><description>[yes no] Double-dip light curve? (8)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>DDmove</name><description>[yes no] Moving double-dip light curve? (8)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Beat</name><description>[yes no] Full light curve has beating visible? (8)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>CPeak</name><description>[yes no] Complex peak? (8) (9)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RClose</name><description>[yes no] Resolved close periods? (8)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RDist</name><description>[yes no] Resolved distant periods? (8)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Pulse</name><description>[yes no] Pulsator? (8)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>