Table 5
Best-fit results for the planet-to-star radius ratio and limb darkening coefficients, u1 and u2, for the narrowband channel light curves of Run 2.
| Channel | λ [nm] | Rp/R⋆ | Δtransit depth [%] | u1 | u2 | Dilution factor cn[%] | Red noise factor β |
|
|
|||||||
| #1 | 518−538 |
|
|
|
|
0.1574 ± 0.0522 | 1.862 |
| #2 | 538−558 |
|
|
|
|
0.1689 ± 0.0565 | 1.950 |
| #3 | 558−578 |
|
|
|
|
0.1796 ± 0.0541 | 1.612 |
| #4 | 578−598 |
|
|
|
|
0.1710 ± 0.0553 | 1.022 |
| #5 | 598−618 |
|
|
|
|
0.1944 ± 0.0554 | 1.761 |
| #6 | 618−638 |
|
|
|
|
0.1855 ± 0.0525 | 1.950 |
| #7 | 638−658 |
|
|
|
|
0.3335 ± 0.0601 | 1.908 |
| #8 | 658−678 |
|
|
|
|
0.2665 ± 0.0587 | 1.575 |
| #9 | 678−698 |
|
|
|
|
0.2700 ± 0.0606 | 1.702 |
| #10 | 698−718 |
|
|
|
|
0.3621 ± 0.0583 | 1.738 |
| #11 | 718−738 |
|
|
|
|
0.5098 ± 0.0646 | 1.285 |
| #12 | 738−758 |
|
|
|
|
0.7963 ± 0.0613 | 1.626 |
| (#13 | 758−778 |
|
|
|
|
0.6573 ± 0.0588 | 1.731) |
| #13b | 763−778 |
|
|
|
|
0.6211 ± 0.0568 | 1.191 |
| #14 | 778−798 |
|
|
|
|
0.7601 ± 0.0644 | 1.886 |
| #15 | 798−818 |
|
|
|
|
1.0250 ± 0.0684 | 1.212 |
| #16 | 818−838 |
|
|
|
|
1.0954 ± 0.0670 | 1.994 |
| #17 | 838−858 |
|
|
|
|
1.0714 ± 0.0688 | 1.230 |
| #18 | 858−878 |
|
|
|
|
1.1793 ± 0.0703 | 1.380 |
| #19 | 878−898 |
|
|
|
|
1.2985 ± 0.0643 | 1.633 |
| #20 | 898−918 |
|
|
|
|
1.4459 ± 0.0701 | 1.789 |
Notes. For every channel the red noise factor β that was used to inflate the MCMC derived error bars of the results is given. Also the respective dilution factor cn that was given as prior information for every channel is listed. Listed separately are changes in the transit depth with respect to the white light transit depth, i.e., Δtransit depth 
. These values are independent from the absolute value of the white light radius ratio assumed during the analysis.
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