Detection limits for close eclipsing and transiting substellar and planetary companions to white dwarfs in the WASP survey

Monthly Notices of the Royal Astronomical Society

Volumn 410, Issue 2, 2011, Pages 899-911

  Faedi, F ^a,b   West, R G ^a   Burleigh, M R ^a   Goad, M R ^a   Hebb, L ^c,d  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

^b QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

^d VANDERBILT UNIVERSITY   (United States)

Author keywords

Methods: data analysis; Occultations; Planetary systems; White dwarfs

Indexed keywords

ORBITS; SIGNAL TO NOISE RATIO; SURVEYS;

DETECTION LIMITS; DETECTION RATES; EXTENSIVE SIMULATIONS; LIGHT CURVES; METHODS. DATA ANALYSIS; OCCULTATION; ORBITAL PERIODS; ORBITAL RADIUS; PLANETARY SYSTEM; WIDE ANGLE;

WHITE DWARFS;

EID: 78650711580     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17488.x     Document Type: Article

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