Thermal emission at 4.5 and 8μm of WASP-17b, an extremely large planet in a slightly eccentric orbit

Monthly Notices of the Royal Astronomical Society

Volumn 416, Issue 3, 2011, Pages 2108-2122

  Anderson, D R ^a   Smith, A M S ^a   Lanotte, A A ^b   Barman, T S ^c   Cameron, A Collier ^d   Campo, C J ^e   Gillon, M ^b   Harrington, J ^e   Hellier, C ^a   Maxted, P F L ^a   Queloz, D ^f   Triaud, A H M J ^f   Wheatley, P J ^g  

^a KEELE UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c LOWELL OBSERVATORY   (United States)

^d UNIVERSITY OF ST ANDREWS   (United Kingdom)

^e UNIVERSITY OF CENTRAL FLORIDA   (United States)

^f UNIVERSITÉ DE GENÈVE   (Switzerland)

^g UNIVERSITY OF WARWICK   (United Kingdom)

Author keywords

Methods: data analysis; Occultations; Planets and satellites: atmospheres; Planets and satellites: individual: WASP 17b; Stars: individual: WASP 17; Techniques: photometric

Indexed keywords

LUMINANCE; ORBITS; SATELLITES; STARS;

LIGHT CURVES; METHODS. DATA ANALYSIS; OCCULTATION; PLANET AND SATELLITE: INDIVIDUAL: WASP-17B; PLANETS AND SATELLITES: ATMOSPHERES; PLANETS AND SATELLITES: INDIVIDUAL; STAR: INDIVIDUAL: WASP-17; STARS: INDIVIDUAL: PROXIMA CENTAURI; TECHNIQUES: PHOTOMETRIC; THERMAL EMISSIONS;

PLANETS;

EID: 80052639327     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19182.x     Document Type: Article

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