A transit timing analysis of seven RISE light curves of the exoplanet system HAT-P-3

Monthly Notices of the Royal Astronomical Society

Volumn 401, Issue 3, 2010, Pages 1917-1923

  Gibson, N P ^a   Pollacco, D L ^a   Barros, S ^a   Benn, C ^b   Christian, D ^c   Hrudkova M ^d   Joshi, Y C ^a,e   Keenan, F P ^a   Simpson, E K ^a   Skillen, I ^b   Steele, I A ^f   Todd, I ^a  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^c CALIFORNIA STATE UNIVERSITY   (United States)

^d CHARLES UNIVERSITY   (Czech Republic)

^e ARYABHATTA RESEARCH INSTITUTE OF OBSERVATIONAL SCIENCES ARIES   (India)

^f LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

Author keywords

Methods: data analysis; Planetary systems; Stars: individual: HAT P 3; Techniques: photometric

Indexed keywords

EXTRASOLAR PLANETS; ORBITS; SEARCH ENGINES; STARS; TIMING CIRCUITS;

EXO-PLANETS; LIGHT CURVES; METHODS. DATA ANALYSIS; PLANETARY SYSTEM; STAR: INDIVIDUAL: HAT-P-3; STARS: INDIVIDUAL: PROXIMA CENTAURI; TECHNIQUES: PHOTOMETRIC; TIMING ANALYSIS; TRANSIT TIMING; TRANSIT-TIME;

MARKOV PROCESSES;

EID: 73949108651     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15770.x     Document Type: Article

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