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High-precision Photometry by Telescope Defocussing. VI. WASP-24, WASP-25 and WASP-26

John Southworth,T. C. Hinse,M. Burgdorf,S. Calchi Novati,M. Dominik,P. Galianni,T. Gerner,E. Giannini,S. -H. Gu,M. Hundertmark,U. G. Jorgensen,D. Juncher,E. Kerins,L. Mancini,M. Rabus,D. Ricci,S. Schaefer,J. Skottfelt,J. Tregloan-Reed,X. -B. Wang,O. Wertz,K. A. Alsubai,J. M. Andersen,V. Bozza,D. M. Bramich,P. Browne,S. Ciceri,G. D'Ago,Y. Damerdji,C. Diehl,P. Dodds,A. Elyiv,X. -S. Fang,F. Finet,R. Figuera Jaimes,S. Hardis,K. Harpsoe,J. Jessen-Hansen,N. Kains,H. Kjeldsen,H. Korhonen,C. Liebig,M. N. Lund,M. Lundkvist,M. Mathiasen,M. T. Penny,A. Popovas, S. Prof,S. Rahvar,K. Sahu,G. Scarpetta,R. W. Schmidt,F. Schoenebeck,C. Snodgrass,R. A. Street,J. Surdej,Y. Tsapras,C. Vilela

Monthly Notices of the Royal Astronomical Society（2014）

Cited 74|Views42
Key words
stars: fundamental parameters,planetary systems,stars: individual: WASP-24,stars: individual: WASP-25,stars: individual: WASP-26
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