J/A+A/524/A97ivo://CDS.VizieR/J/A+A/524/A97doi:10.26093/cds/vizier.35240097CDSLopez-Santiago J.Albacete-Colombo J.F.Lopez-Garcia M.A.2017-12-06T07:37:59Z2011-04-07T08:54:40ZCDS support team

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

cds-question@unistra.fropen-star-clustersx-ray-sourcesThe members of the {eta} Chamaleontis cluster are in an evolutionary stage in which disks are rapidly evolving. It also exhibits some peculiarities, such as the large fraction of binaries and accretion disks, probably related to the cluster formation process. Its proximity makes this stellar group an ideal target for studying the relation between X-ray emission and those stellar parameters. Our main objective is to determine the general X-ray properties of the cluster members in terms of coronal temperature, column density, emission measure, X-ray luminosity, and variability. We also aim to establish the relation between the X-ray luminosity of these stars and other stellar parameters, such as effective temperature, binarity, and the presence of accretion disks. Finally, a study of flare energies in each flare event detected during the observations and their relation with some stellar parameters is also performed.2010A&A...524A..97Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/524/A97CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2009)IX/37 : XMM-Newton Serendipitous Source Catalogue (1XMM) (XMM-SSC, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/524/A97https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/524/A97http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/524/A97https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/524/A97https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/524/A97http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/524/A97GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/524/A97/tablea1 (Sources detected in the 0.3-7.5keV energy band using PWDetect with detection threshold SNR=5)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/524/A97/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/524/A97/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/524/A97/tablea1?GETtext/xml+votable180.050000true131.39125-79.2259720.0055555555555555566/36926-36927 37012-37013https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/524/A97?format=asciiX-raydefaultJ/A+A/524/A97/tablea1Sources detected in the 0.3-7.5keV energy band using PWDetect with detection threshold SNR=5NoteRemarkmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[01/86] Source sequential numbermeta.id;meta.mainintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainSigniSignificance of the detectionstat.fit.goodness;instr.saturationfloatCountsObserved counts in 0.3-7.5keV band (in units of 10^-3^s^-1^)ct/ksphot.count;em.X-rayfloate_CountsError in the observed counts (in 10^-3^s^-1^)ct/ksstat.error;phot.countfloatFluxObserved flux in 0.3-7.5keV band (in units of 10^-13^erg/cm^2^/s)1e-16W.m**-2phot.flux;em.X-rayfloate_FluxError in the flux (in 10^-13^erg/cm^2^/s)1e-16W.m**-2stat.error;phot.fluxfloatONameOther namemeta.idcharSimbadSimbad column added by the CDSmeta.refchar