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Table 2

Model comparison for the white light curve of Run 1.

Model ΔBIC ΔRp/R

xpos0 ypos0 airm0 fwhm3 5.76 0.000586
xpos0 ypos0 airm1 fwhm3 4.28 0.000292
xpos0 ypos0 airm1 fwhm4 9.63 0.000332
xpos0 ypos1 airm0 fwhm3 7.96 0.000399
xpos0 ypos1 airm1 fwhm2 6.92 0.000050
xpos0 ypos1 airm1 fwhm3 0.00 0.000000
xpos0 ypos1 airm1 fwhm4 5.70 0.000125
xpos0 ypos2 airm1 fwhm3 4.63 0.000019
xpos1 ypos0 airm0 fwhm3 7.23 0.000300
xpos1 ypos0 airm1 fwhm3 9.77 0.000443
xpos1 ypos0 airm2 fwhm3 7.46 0.000492
xpos1 ypos1 airm0 fwhm3 5.54 0.000456
xpos1 ypos1 airm1 fwhm3 5.69 0.000046
xpos1 ypos2 airm0 fwhm3 9.77 0.000346

Notes. Different model approaches for the systematic noise and the respective values for ΔBIC = BIC − BICmin and the respective change in best-fitting planet-to-star radius ratio .

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