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Table A.3

Optimum parameters used for our pipeline which minimise the χ2 of a least-squares fit to the systematic errors and the transit.

Planet Channel Aperture size Background method Background params Centroiding method Centroiding params
pixels pixels pixels
HAT-P-32 b ch1 2.50 Annulus –, 6, 4 Barycenter 3.0
HAT-P-32 b ch2 2.50 Annulus –, 6, 4 Barycenter 5.0
XO-1 b ch1 2.50 Annulus –, 6, 4 Moffat
XO-1 b ch2 2.50 Annulus –, 6, 4 Gaussian
HAT-P-1 b ch1 3.00 Box 4, –, – Barycenter 5.0
HAT-P-1 b ch2 3.50 Box 4, –, – Barycenter 5.0
WASP-17 b ch1 2.50 Annulus –, 6, 4 Barycenter 5.0
WASP-17 b ch2 2.50 Annulus –, 6, 4 Barycenter 3.0
WASP-39 b ch1 2.50 Annulus –, 6, 4 Barycenter 3.0
WASP-39 b ch2 2.50 Annulus –, 6, 4 Barycenter 7.0
HAT-P-12 b ch1 2.50 Annulus –, 6, 4 Moffat
HAT-P-12 b ch2 2.50 Annulus –, 6, 4 Moffat
HAT-P-18 b ch1 2.50 Annulus –, 6, 4 Barycenter 5.0
HAT-P-18 b ch2 2.50 Annulus –, 6, 4 Moffat
TrES-2 b ch1 2.50 Annulus –, 6, 4 Barycenter 5.0
TrES-2 b ch2 2.50 Histogram –, –, – Barycenter 3.0
WASP-4 b ch1 2.50 Annulus –, 6, 4 Moffat
WASP-4 b ch2 2.50 Annulus –, 6, 4 Barycenter 5.0
XO-2 b ch1 2.50 Annulus –, 6, 4 Moffat
XO-2 b ch2 2.50 Annulus –, 6, 4 Barycenter 7.0
GJ3470 b ch1 2.50 Annulus –, 6, 4 Barycenter 3.0
GJ3470 b ch2 2.50 Annulus –, 6, 4 Barycenter 3.0
WASP-21 b ch1 2.50 Annulus –, 6, 4 Barycenter 5.0
WASP-21 b ch2 2.50 Annulus –, 6, 4 Barycenter 5.0
WASP-31 b ch1 2.50 Annulus –, 6, 4 Barycenter 7.0
WASP-31 b ch2 2.50 Annulus –, 6, 4 Barycenter 7.0
WASP-1 b ch1 2.50 Annulus –, 6, 4 Barycenter 7.0
WASP-1 b ch2 2.50 Annulus –, 6, 4 Barycenter 3.0
HAT-P-26 b ch1 2.50 Annulus –, 6, 4 Barycenter 7.0
HAT-P-26 b ch2 2.50 Annulus –, 6, 4 Barycenter 5.0
WASP-107 b ch1 2.25 Histogram –, –, – Barycenter 5.0
WASP-107 b ch2 2.25 Histogram –, –, – Barycenter 3.0
WASP-13 b ch1 2.25 Histogram –, –, – Gaussian
WASP-13 b ch2 2.50 Histogram –, –, – Barycenter 3.0
WASP-121 b ch1 1.00 Histogram –, –, – Barycenter 3.0
WASP-121 b ch2 1.00 Box 4, –, – Barycenter 3.0
WASP-69 b ch1 2.00 Histogram –, –, – Gaussian
WASP-69 b ch2 2.25 Histogram –, –, – Barycenter 3.0
WASP-67 b ch1 2.00 Histogram –, –, – Moffat
WASP-67 b ch2 2.00 Histogram –, –, – Moffat
HATS-7 b ch1 2.00 Histogram –, –, – Barycenter 3.0
HATS-7 b ch2 2.00 Histogram –, –, – Gaussian
WASP-29 b ch1 2.25 Histogram –, –, – Gaussian
WASP-29 b ch2 2.25 Histogram –, –, – Barycenter 3.0
HAT-P-41 b ch1 2.25 Histogram –, –, – Barycenter 3.0
HAT-P-41 b ch2 2.25 Histogram –, –, – Gaussian
WASP-101 b ch1 2.25 Histogram –, –, – Barycenter 5.0
WASP-101 b ch2 2.25 Histogram –, –, – Barycenter 3.0
WASP-131 b ch1 2.25 Histogram –, –, – Barycenter 5.0
WASP-131 b ch2 2.25 Histogram –, –, – Barycenter 3.0
WASP-36 b ch1 2.00 Histogram –, –, – Gaussian
WASP-36 b ch2 2.00 Histogram –, –, – Barycenter 3.0
WASP-63 b ch1 2.25 Histogram –, –, – Barycenter 5.0
WASP-63 b ch2 2.25 Histogram –, –, – Gaussian
WASP-79 b ch1 2.50 Histogram -, -, - Barycenter 5.0
WASP-79 b ch2 2.25 Histogram -, -, - Barycenter 3.0
WASP-94 Ab ch1 2.50 Histogram -, -, - Moffat
WASP-94 Ab ch2 2.25 Histogram -, -, - Barycenter 3.0
WASP-74 b ch1 2.25 Histogram -, -, - Barycenter 3.0
WASP-74 b ch2 2.00 Histogram -, -, - Barycenter 3.0
WASP-62 b ch1 2.25 Histogram -, -, - Barycenter 3.0
WASP-62 b ch2 2.25 Box 4, -, - Barycenter 3.0
KELT-7 b ch1 2.25 Histogram -, -, - Moffat
KELT-7 b ch2 2.00 Histogram -, -, - Barycenter 3.0
Kepler-45 b ch1 1.00 Histogram -, -, - Barycenter 3.0
Kepler-45 b ch1 1.00 Histogram -, -, - Gaussian
Kepler-45 b ch1 1.00 Histogram -, -, - Gaussian
Kepler-45 b ch1 1.00 Histogram -, -, - Gaussian
Kepler-45 b ch2 1.00 Histogram -, -, - Gaussian
Kepler-45 b ch2 1.00 Histogram -, -, - Barycenter 3.0
Kepler-45 b ch2 1.00 Histogram -, -, - Moffat
Kepler-45 b ch2 1.00 Box 2, -, - Gaussian

Notes. If background method is “Annulus”, then the two parameters are the radius and width of a circular annulus; if it is “box” then the parameter is the size of the box taken in all of the four corners of the image. If the centroiding method is “baycenter” then the parameter is the number of pixels over which to create a box over the star for the flux weighting.

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