J/A+A/586/A47ivo://CDS.VizieR/J/A+A/586/A47doi:10.26093/cds/vizier.35860047CDSSousa A.P.Alencar S.H.P.Bouvier J.Stauffer J.R.Venuti L.,Flaccomio E.Hillenbrand L.Cody A.M.Teixeira P.S.Guimaraes M.M.,McGinnis P.T.Rebull L.Flaccomio E.Fueresz G.Micela G.Gameiro J.F.2017-10-02T19:28:58Z2016-01-25T08:17:23ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fropen-star-clusterspre-main-sequence-starsline-intensitiesNGC 2264 is a young stellar cluster (~3Myr) with hundreds of low-mass accreting stars that allow a detailed analysis of the accretion process taking place in the pre-main sequence. Our goal is to relate the photometric and spectroscopic variability of classical T Tauri stars to the physical processes acting in the stellar and circumstellar environment, within a few stellar radii from the star. NGC 2264 was the target of a multiwavelength observational campaign with CoRoT, MOST, Spitzer, and Chandra satellites and photometric and spectroscopic observations from the ground. We classified the CoRoT light curves of accreting systems according to their morphology and compared our classification to several accretion diagnostics and disk parameters.2016A&A...586A..47Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/586/A47CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/147/82 : Monitoring of disk-bearing stars in NGC 2264 (Cody+, 2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/586/A47https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/586/A47http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/586/A47https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/586/A47https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/586/A47http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/586/A47GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/586/A47/table2 (Parameters of the CTTSs observed by CoRoT and/or FLAMES/VLT)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/586/A47/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/586/A47/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/586/A47/table2?GETtext/xml+votable180.050000true100.4719.96744440.005555555555555556Cone search capability for table J/A+A/586/A47/table3 (Parameters of the WTTSs observed by CoRoT and/or FLAMES/VLT)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/586/A47/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/586/A47/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/586/A47/table3?GETtext/xml+votable180.050000true100.45245839.90319440.0055555555555555566/23636-23637 23639https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/586/A47?format=asciidefaultJ/A+A/586/A47/table2Parameters of the CTTSs observed by CoRoT and/or FLAMES/VLTPer2011? CoRoT photometric perioddtime.periodfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCSIMonInternal identification of CSI 2264 campaignmeta.id;meta.mainint2MASS2MASS identification (HHMMSSss+DDMMSSs)meta.idcharSpTypeSpectral type (G1)src.spTypecharEWHa? Halpha equivalent width measured using FLAMES spectra (G2)0.1nmspect.line.eqWidth;em.line.Halphafloatnullablee_EWHa? EWHa uncertainties obtained assuming a Poisson distribution0.1nmstat.errorfloatnullableW10? Halpha width at 10% of maximum intensitykm/sspect.line.widthintnullableEWHal? Halpha equivalent width obtained by Dahm et al., 2005AJ....129..829D, Cat. J/AJ/129/8290.1nmspect.line.eqWidth;em.line.Halpha;meta.modelledfloatnullableFUR06[cw] Classification as CTTS (c) or WTTS (w) (G3)meta.code.classcharalphaIRAC? Slope of the spectral energy distribution between 3.6 and 8um (G4)spect.indexfloatnullableLC2008Note on 2008 light curves (5)meta.codecharPer2008? CoRoT photometric perioddtime.periodfloatnullableLC2011Note on 2008 light curves (5)meta.codecharQ? Parameter defined by Cody et al., 2014AJ....147...82C to distinguish periodic from aperiodic light curvesphot.color.reddFreefloatnullableSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from 2MASS or CSIMon names (right ascension part)degpos.eq.ra;meta.main_DEPositions from 2MASS or CSIMon names (declination part)degpos.eq.dec;meta.mainJ/A+A/586/A47/table3Parameters of the WTTSs observed by CoRoT and/or FLAMES/VLTrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCSIMonInternal identification of CSI 2264 campaignmeta.id;meta.mainint2MASS2MASS identification (HHMMSSss+DDMMSSs)meta.idcharSpTypeSpectral type (G1)src.spTypecharEWHa? Halpha equivalent width measured using FLAMES spectra (G2)0.1nmspect.line.eqWidth;em.line.Halphafloatnullablee_EWHa? EWHa uncertainties obtained assuming a Poisson distribution0.1nmstat.errorfloatnullableW10? Halpha width at 10% of maximum intensitykm/sspect.line.widthintnullableEWHal? Halpha equivalent width obtained by Dahm et al., 2005AJ....129..829D, Cat. J/AJ/129/8290.1nmspect.line.eqWidth;em.line.Halpha;meta.modelledfloatnullableFUR06[cw] Classification as CTTS (c) or WTTS (w) (G3)meta.code.classcharalphaIRAC? Slope of the spectral energy distribution between 3.6 and 8um (G4)spect.indexfloatnullableSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from 2MASS or CSIMon names (right ascension part)degpos.eq.ra;meta.main_DEPositions from 2MASS or CSIMon names (declination part)degpos.eq.dec;meta.main