Limits on the 2.2-μm contrast ratio of the close-orbiting planet HD 189733b

Monthly Notices of the Royal Astronomical Society

Volumn 382, Issue 1, 2007, Pages 473-480

  Barnes, J R ^a   Barman, Travis S ^b   Prato, L ^b   Segransan, D ^c   Jones, H R A ^a   Leigh, C J ^d   Collier Cameron, A ^e   Pinfield, D J ^a  

^a UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^b LOWELL OBSERVATORY   (United States)

^c UNIVERSITÉ DE GENÈVE   (Switzerland)

^d LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^e UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Line: profiles; Methods: data analysis; Planetary systems; Stars: individual: HD 189733; Stars: late type; Techniques: spectroscopic

Indexed keywords

EXTRASOLAR PLANETS; ORBITS; SIGNAL TO NOISE RATIO; STARS;

ABSORPTION SIGNATURE; CONTRAST-RATIO; LINE: PROFILES; METHODS. DATA ANALYSIS; PLANETARY SYSTEM; SPECTRA'S; STAR: INDIVIDUAL: HD 189733; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:LATE TYPE; TECHNIQUES: SPECTROSCOPIC;

INFRARED DEVICES;

EID: 36148983098     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12394.x     Document Type: Article

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