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CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM

dc.contributor.authorLatham, D. W.
dc.contributor.authorGilbert, H.
dc.contributor.authorMugrauer, M.
dc.contributor.authorMaciejewski, G.
dc.contributor.authorNiedzielski, A.
dc.contributor.authorWolszczan, A.
dc.contributor.authorNowak, G.
dc.contributor.authorNeuhaeuser, R.
dc.contributor.authorWinn, J. N.
dc.contributor.authorDeka, B.
dc.contributor.authorAdamow, M.
dc.contributor.authorGorecka, M.
dc.contributor.authorFernandez, M.
dc.contributor.authorAceituno, F. J.
dc.contributor.authorOhlert, J.
dc.contributor.authorErrmann, R.
dc.contributor.authorSeeliger, M.
dc.contributor.authorDimitrov, D.
dc.contributor.authorEsquerdo, G. A.
dc.contributor.authorMcKnight, L.
dc.contributor.authorHolman, M. J.
dc.contributor.authorJensen, E. L. N.
dc.contributor.authorKramm, U.
dc.contributor.authorPribulla, T.
dc.contributor.authorRaetz, St.
dc.contributor.authorSchmidt, T. O. B.
dc.contributor.authorGinski, Ch.
dc.contributor.authorSaral, G.
dc.contributor.authorPopov, V.
dc.contributor.authorRaetz, M.
dc.contributor.authorMottola, S.
dc.contributor.authorHellmich, S.
dc.contributor.authorAdam, Ch.
dc.date.accessioned2021-03-05T08:06:34Z
dc.date.available2021-03-05T08:06:34Z
dc.date.issued2013
dc.identifier.citationMaciejewski G., Niedzielski A., Wolszczan A., Nowak G., Neuhaeuser R., Winn J. N. , Deka B., Adamow M., Gorecka M., Fernandez M., et al., "CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM", ASTRONOMICAL JOURNAL, cilt.146, 2013
dc.identifier.issn0004-6256
dc.identifier.othervv_1032021
dc.identifier.otherav_97312e4d-22e0-4969-8103-dd04660023a2
dc.identifier.urihttp://hdl.handle.net/20.500.12627/101782
dc.identifier.urihttps://doi.org/10.1088/0004-6256/146/6/147
dc.description.abstractThere have been previous hints that the transiting planet WASP-3b is accompanied by a second planet in a nearby orbit, based on small deviations from strict periodicity of the observed transits. Here we present 17 precise radial velocity (RV) measurements and 32 transit light curves that were acquired between 2009 and 2011. These data were used to refine the parameters of the host star and transiting planet. This has resulted in reduced uncertainties for the radii and masses of the star and planet. The RV data and the transit times show no evidence for an additional planet in the system. Therefore, we have determined the upper limit on the mass of any hypothetical second planet, as a function of its orbital period.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.titleCONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
dc.typeMakale
dc.relation.journalASTRONOMICAL JOURNAL
dc.contributor.departmentNicolaus Copernicus University , ,
dc.identifier.volume146
dc.identifier.issue6
dc.contributor.firstauthorID212098


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