Table C.2
Polynomial detrending baselines applied to the space-based light curves within the MCMC scheme.
| Time series | Planet | Detrending model |
|---|---|---|
| CH 1 | b c | GP(roll) + t3 + (xy)2 |
| CH 2 | b | GP(roll) + (xy)2 |
| CH 3 | b c | GP(roll) + smear1 + (xy)1 |
| CH 4 | b | GP(roll) + t1 + (xy)1 |
| CH 5 | b | GP(roll) + (xy)2 |
| CH 6 | 0 | GP(roll)+ sky1 |
| CH 7 | b | GP(roll) + (xy)2 |
| CH 8 | b | GP(roll) +t1 + sky1 + (xy)2 |
| CH 9 | b c | GP(roll) + t1 + (xy)2 |
| CH 10 | 0 | GP(roll) + (xy)1 |
| CH 11 | b | GP(roll) + t4 + (xy)2 |
| CH 12 | b | GP(roll) + t1 |
| CH 13 | 0 | GP(roll) + (xy)2 |
| CH 14 | b | GP(roll) +t2 + (xy)2 |
| CH 15 | 0 | GP(roll) + (xy)2 |
| CH 16 | b c | GP(roll) + (xy)2 |
| CH 17 | b | GP(roll) + (xy)2 |
| CH 18 | b | GP(roll) + (xy)2 |
| CH 19 | b | GP(roll) |
| CH 20 | 0 | GP(roll) + t2 |
| CH 21 | b | GP(roll) |
| CH 22 | 0 | GP(roll) |
| CH 23 | b | GP(roll) |
| CH 24 | 0 | GP(roll) + t2 |
| CH 25 | 0 | GP(roll) + t2 |
| TE 1 | b | dx1 |
| TE 2 | b | dx1 |
| TE 3 | b | dx1 |
| TE 4 | b c | dx1 |
| TE 5 | b | dx1 |
| TE 6 | b | c |
| TE 7 | b | dx1 |
| TE 8 | b | dx1 |
| TE 9 | b | dx1 |
| TE 10 | b | c |
| TE 11 | b | c |
| TE 12 | b | c |
| TE 13 | b | c |
| TE 14 | b | dx1 |
| TE 15 | b | t1 |
| TE 16 | b | c |
| TE 17 | b c | dy1 |
| TE 18 | b | dx1 |
| TE 19 | b | c |
| TE 20 | b | c |
| TE 21 | b | c |
| TE 22 | b | c |
| TE 23 | b | c |
| TE 24 | b | c |
| TE 25 | b | c |
| TE 26 | b | dx1 |
| TE 27 | b | c |
| TE 28 | b | c |
| TE 29 | b | dx1 + (xy)1 |
| TE 30 | b | dx1 + (xy)1 |
| TE 31 | b c | t1 + dx1 + (xy)1 |
| TE 32 | b | t1 + dx1 |
| TE 33 | b | t3 + dx1 |
| TE 34 | b | t3 + dx1 + dy1 |
| TE 35 | b | dx1 |
| TE 36 | b | dx1 |
| TE 37 | b | t1 + dx1 + (xy)1 |
| TE 38 | b | t1 + dx2 |
| TE 39 | b | dx1 |
| TE 40 | b | dx1 + (xy)1 |
| TE 41 | b | dx1 |
| TE 42 | b | t2 + dx3 + (xy)1 |
| TE 43 | b | dx1 |
| TE 44 | b | dx1 |
| TE 45 | b | t1 + dx1 |
| TE 46 | b | t1 + dx1 |
| TE 47 | b | dx1 |
| TE 48 | b | dx1 |
| TE 49 | b | t2 + dx1 + (xy)1 |
| TE 50 | b | dx1 |
| TE 51 | b | t2 + dx1 |
| TE 52 | b | dx1 |
| TE 53 | b | t1 + dx1 |
| TE 54 | b | dx1 |
| TE 55 | b | dx1 |
| TE 56 | b c | t1 + dx1 |
| TE 57 | b | dx1 |
| TE 58 | b | t1 + dx1 |
| TE 59 | b | dx1 |
| TE 60 | b | t2 + dx1 |
| TE 61 | b | t1 + dx1 |
| TE 62 | b | t1 + dx1 |
| TE 63 | b | t3 + dx1 |
| TE 64 | b | dx1 |
| TE 65 | b | t1 + dx1 |
| TE 66 | b | dx1 |
| TE 67 | b | t2 + dx1 |
| TE 68 | b | t1 + dx1 |
| TE 69 | b | dx1 |
| TE 70 | b c | t1 + dx1 |
| TE 71 | b | dx1 |
| TE 72 | b | dx1 |
| TE 73 | b | t1 + dx1 + (xy)1 |
| TE 74 | b | dx1 |
| TE 75 | b | t1 + dx1 |
| TE 76 | b | dx1 |
| TE 77 | b | t3 + dx1 |
| TE 78 | b | dx1 |
| TE 79 | b | t1 + dx1 |
| TE 80 | b | t1 + dx1 |
| TE 81 | b | t2 + dx1 |
Notes. CHEOPS LCs furtherrequired a GP-based pre-detrending againstthe roll angle, here denoted with GP(roll). The LC counterrefers to the CHEOPS (CH) and TESS (TE) light curves, extracted as detailed in the text in chronological order of observations. In particular, TE LC from 1 to 28, from 29 to 52, and from 53 to 81 are extracted from Sector 9, 35, and 62, respectively. All the ground-based observations reduced as explained in the text only required a normalisation scalar (c). See text for further details.
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