The impact of correlated noise on Super WASP detection rates for transiting extrasolar planets

Monthly Notices of the Royal Astronomical Society

Volumn 373, Issue 3, 2006, Pages 1151-1158

  Smith, A M S ^a   Collier Cameron, A ^a   Christian, D J ^b   Clarkson, W I ^c,d   Enoch, B ^c   Evans, A ^e   Haswell, C A ^c   Hellier, C ^e   Horne, K ^a   Irwin, J ^f   Kane, S R ^g   Lister, T A ^a,e   Norton, A J ^c   Parley, N ^c   Pollacco, D L ^b   Ryans, R ^b   Skillen, I ^h   Street, R A ^b   Triaud, A H M J ^a   West, R G ⁱ   Wheatley, P J ^j   Wilson, D M ^e   more..

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^c OPEN UNIVERSITY   (United Kingdom)

^d AURA for the European Space Agency   (United States)

^e KEELE UNIVERSITY   (United Kingdom)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^g 211 Bryant Space Science Center ^*  (United States)

^h ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

ⁱ UNIVERSITY OF LEICESTER   (United Kingdom)

^j UNIVERSITY OF WARWICK   (United Kingdom)

more..

Author keywords

Planetary systems; Techniques: photometric

Indexed keywords

ASTROPHYSICS; CAMERAS; EXTRASOLAR PLANETS; STARS;

CORRELATED NOISE; DETECTION RATES; METALLICITIES; ONE CAMERA; PLANETARY SYSTEM; RED NOISE; STELLAR POPULATIONS; STELLARS; SYSTEMATIC NOISE; TECHNIQUES: PHOTOMETRIC;

SIGNAL TO NOISE RATIO;

EID: 33845316427     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11095.x     Document Type: Article

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