Physical properties of the planetary systems WASP-45 and WASP-46 from simultaneous multi-band photometry

S Ciceri,L Mancini, J Southworth,M Lendl,J Tregloanreed,R Brahm,Gang Chen, G Dago,M Dominik,R Figuera Jaimes, P Galianni,K Harpsoe,T C Hinse,U G Jorgensen,D Juncher,H Korhonen,C Liebig,M Rabus,A S Bonomo, Kaspar Bott,Th Henning,A Jordan,A Sozzetti,K A Alsubai, J M Andersen,D Bajek,V Bozza,D M Bramich,P Browne,S Calchi Novati,Y Damerdji,C Diehl,A Elyiv,E Giannini,Sh Gu,M Hundertmark,N Kains,M T Penny,A Popovas,S Rahvar,G Scarpetta,R W Schmidt,J Skottfelt,C Snodgrass,Jean Surdej,C Vilela, Xb Wang,O Wertz

Monthly Notices of the Royal Astronomical Society（2016）

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Abstract

Accurate measurements of the physical characteristics of a large number of exoplanets are useful to strongly constrain theoretical models of planet formation and evolution, which lead to the large variety of exoplanets and planetary-system configurations that have been observed. We present a study of the planetary systems WASP-45 and WASP-46, both composed of a main-sequence star and a close-in ho...

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Key words

planets and satellites: fundamental parameters,stars: fundamental parameters,stars: individual: WASP-45,stars: individual: WASP-46

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