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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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