J/A+A/526/A150ivo://CDS.VizieR/J/A+A/526/A150doi:10.26093/cds/vizier.35260150CDSRibeiro T.Baptista R.2017-06-27T06:37:55Z2011-01-13T08:50:36ZCDS support team

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

cds-question@unistra.frvariable-starsinfrared-photometryFrom a number of known post common envelopes binaries (PCEB) only a handful have yet been observed at near-infrared (NIR) wavelengths, and even fewer have modeled NIR light curves. At shorter wavelengths one has access to the cooler and larger components of these systems and has a chance to detect emission from its faint and heavily irradiated atmospheres. By modeling NIR light curves of PCEBs, we intend to constrain their system parameters and study the properties of the system components.2011A&A...526A.150Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/526/A150CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/526/A150https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/526/A150http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/526/A150https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/526/A150https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/526/A150http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/526/A150GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/A+A/526/A150/photomLight curves of KV Vel (JHK) and TW Crv (JH)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar namemeta.id;meta.maincharBand[JHK] Observed bandinstr.bandpasscharPhaseOrbital phasetime.phasefloatFluxFlux in BandmJyphot.flux.density;em.IRfloate_FluxFlux errormJystat.error;phot.fluxfloat