A comparison of spectroscopic methods for detecting the starlight scattered by transiting hot Jupiters, with an application to Subaru data for HD 209458b and HD 189733b

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 1, 2011, Pages 673-686

  Langford, Sally V ^a,b   Wyithe, J Stuart B ^a   Turner, Edwin L ^b,c   Jenkins, Edward B ^b   Narita, Norio ^d   Liu, Xin ^b   Suto, Yasushi ^b,c,e   Yamada, Toru ^f  

^a UNIVERSITY OF MELBOURNE   (Australia)

^b PRINCETON UNIVERSITY OBSERVATORY   (United States)

^c UNIVERSITY OF TOKYO   (Japan)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^e UNIVERSITY OF TOKYO   (Japan)

^f TOHOKU UNIVERSITY   (Japan)

Author keywords

Planetary systems; Techniques: radial velocities

Indexed keywords

EXTRASOLAR PLANETS; FOURIER ANALYSIS; INTELLIGENT SYSTEMS; ORBITS; SIGNAL TO NOISE RATIO; SPECTROSCOPIC ANALYSIS; STARS;

ECHELLE; FLUX RATIO; FOURIER ANALYSIS METHODS; JUPITERS; LIGHT SCATTERED; MEASUREMENTS OF; PLANETARY SYSTEM; SPECTRA'S; TECHNIQUES: RADIAL VELOCITIES; UPPER LIMITS;

MONTE CARLO METHODS;

EID: 79960114335     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18739.x     Document Type: Article

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