Table I.1
Values of the systematic parameters for CHEOPS.
Background |
a
bkg [ppm] ![]() |
b bkg [ppm] 695 ± 96 | |
---|---|---|---|
Roll angle | σGP [ppm] ![]() |
ρGP [deg] ![]() |
|
σw [ppm] | f 0 | c 1 [day−1] | |
Visit 01 |
![]() |
{0.999843 ± 0.000054} | – |
Visit 02 |
![]() |
0.999802 ± 0.000053 | – |
Visit 03 |
![]() |
![]() |
![]() |
Visit 04 |
![]() |
0.999791 ± 0.000050 | – |
Visit 05 |
![]() |
0.999806 ± 0.000051 | – |
Visit 06 |
![]() |
![]() |
– |
Visit 07 |
![]() |
![]() |
– |
Visit 08 |
![]() |
0.999775 ± 0.000050 | – |
Visit 09 |
![]() |
![]() |
![]() |
Visit 10 |
![]() |
![]() |
– |
Visit 11 |
![]() |
0.999764 ± 0.000049 | – |
Visit 12 |
![]() |
0.999808 ± 0.000049 | – |
Visit 13 |
![]() |
![]() |
– |
Visit 14 |
![]() |
![]() |
– |
Visit 15 |
![]() |
1.000084 ± 0.000055 | – |
Visit 16 |
![]() |
![]() |
– |
Visit 17 |
![]() |
0.999772 ± 0.000051 | – |
Visit 18 |
![]() |
1.000101 ± 0.000051 | – |
Visit 19 |
![]() |
1.000062 ± 0.000050 | – |
Visit 20 |
![]() |
0.999665 ± 0.000049 | – |
Visit 21 | 145 ± 18 |
![]() |
– |
Visit 22 |
![]() |
![]() |
– |
Visit 23 |
![]() |
![]() |
– |
Visit 24 |
![]() |
0.999891 ± 0.000049 | – |
Visit 25 |
![]() |
![]() |
– |
Visit 26 |
![]() |
0.999664 ± 0.000049 | – |
Visit 27 |
![]() |
1.000069 ± 0.000049 | – |
Visit 28 |
![]() |
![]() |
– |
Visit 29 | 176 ± 17 | 0.999659 ± 0.000049 | – |
Visit 30 |
![]() |
0.999937 ± 0.000056 | – |
Visit 31 |
![]() |
0.999928 ± 0.000049 | 0.00037 ± 0.00012 |
Visit 32 |
![]() |
0.999888 ± 0.000050 |
![]() |
Visit 33 |
![]() |
0.999643 ± 0.000048 | 0.00012 ± 0.00002 |
Visit 34 |
![]() |
![]() |
– |
Visit 35 |
![]() |
![]() |
![]() |
Visit 36 |
![]() |
![]() |
– |
Visit 37 |
![]() |
0.999605 ± 0.000050 | – |
Notes. The background parameters a bkg and b bkg are the ones defined in Eq. 1. The roll-angle GP hyperparameters σGP and ρGP are the standard deviation of the process and the correlation scale in roll-angle unit (deg), respectively (see Section 4.1). The parameters σ w, f0 and c 1 are the additive noise jitter term, the flux normalisation factor and the flux linear slope, respectively. σw is expressed in parts-per-million (ppm) and is added to all error bars quadratically. A negative value of σ w means that the error bars are shrunk. Each f 0 value is fitted after the corresponding data set has been normalised by its median value (i.e. all flux values are close to 1 and without units). The linear slope c 1 is expressed in normalised flux units per day.
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