J/PASP/121/699ivo://CDS.VizieR/J/PASP/121/699doi:10.26093/cds/vizier.61210699CDSYang Y.-G.2025-09-09T14:13:40Z2010-02-24T15:02:26ZCDS support team

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

cds-question@unistra.frvariable-starsinfrared-photometryvisible-astronomybroad-band-photometryBVR light curves of V343 Orionis were observed with the 85cm telescope at Xinglong Station of the National Astronomical Observatories of the Chinese Academy of Sciences, in 2007 and 2008. Using the Wilson-Devinney program, the photometric solution of V343 Ori was first deduced from those observations. Photometric results indicated that V343 Ori is an A-subtype W Ursae Majoris binary, whose mass ratio and overcontact degree are q=0.253(+/-0.004) and f=86.9%(+/-2.1%), respectively.2009PASP..121..699Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/121/699CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/121/699https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/121/699http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/121/699https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASP/121/699https://vizier.iucaa.in/viz-bin/votable?-source=J/PASP/121/699http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASP/121/699GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/PASP/121/699/table2BVR-band observations for eclipsing binary V343 OrirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBand[BVR] Observed bandinstr.bandpasscharHJDHeliocentric Julian datedtime.epochdoubleDmagDifferential magnitude in Band (1)magphot.mag;arith.difffloat