J/A+A/590/A100ivo://CDS.VizieR/J/A+A/590/A100doi:10.26093/cds/vizier.35900100CDSMallonn M.Strassmeier K.G.2021-03-11T16:52:45Z2016-05-25T13:22:48ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsccd-photometrynarrow-band-photometryWe obtained low-resolution, multi-object spectra of the planet host star HAT-P-32 and multiple comparison stars during a transit event of HAT-P-32b. The spectral flux was binned in 62 narrow channels from 3300 to 10000{AA} and used to create differential photometric light curves. These light curves were analysed for a wavelength dependence of the effective planetary radius.2016A&A...590A.100Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/590/A100CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/590/A100https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/590/A100http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/590/A100https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/590/A100https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/590/A100http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/590/A100GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/590/A100/tablea1Characteristics of the 62 chromatic light curves and the derived values of k with relative uncertaintiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintb_lambdaLower value of wavelength interval0.1nmem.wl;stat.minintB_lambdaUpper value of wavelength interval0.1nmem.wl;stat.maxintlambdaCentral wavelength0.1nmem.wl.centralintWidthWidth of wavelength interval0.1nmem.wlintCompComparison star numbersmeta.id;meta.maincharrmsPoint-to-point scatter valuemmagstat.error;phot.magfloatbeta{beta} factor (1)stat.errorfloatPolyOrder of the time-dependent polynomials usedstat.fit.paramintuLDC u value of the quadratic limb-darkening lawphot.limbDarkfloate_urms uncertainty on u valuestat.errorfloatvLDC v value of the quadratic limb-darkening lawphot.limbDarkfloatkPlanet to star radius ration, k=r_p_/r*phys.size.radiusdoublee_krms uncertainty on kstat.errordoubleLCShow the light curvemeta.ref.urlchar