Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission

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Table I.2

Values of the systematic parameters for TESS.

	σ_w [ppm]	f ₀
Orbit 011	$113_{- 23}^{+ 19}$ ${113}_{-{23}}^{+{19}}$	${0.9996806}_{- 0.0000069}^{+ 0.0000070}$ ${0.9996806}_{-{0.0000069}}^{+{0.0000070}}$
Orbit 012	$89_{- 40}^{+ 25}$ ${89}_{-{40}}^{+{25}}$	0.9996605 ± 0.0000070
Orbit 013	$39_{- 63}^{+ 46}$ ${39}_{-{63}}^{+{46}}$	${0.9998882}_{- 0.0000078}^{+ 0.0000079}$ ${0.9998882}_{-{0.0000078}}^{+{0.0000079}}$
Orbit 014	$150_{- 18}^{+ 17}$ ${150}_{-{18}}^{+{17}}$	${0.9994915}_{- 0.0000077}^{+ 0.0000076}$ ${0.9994915}_{-{0.0000077}}^{+{0.0000076}}$
Orbit 065	203 ± 16	0.9997122 ± 0.0000088
Orbit 066	261 ± 12	${0.9996716}_{- 0.0000084}^{+ 0.0000085}$ ${0.9996716}_{-{0.0000084}}^{+{0.0000085}}$
Orbit 067	$210_{- 13}^{+ 12}$ ${210}_{-{13}}^{+{12}}$	0.9996800 ± 0.0000075
Orbit 068	267 ± 11	0.9996845 ± 0.0000078
Orbit 145	$198_{- 17}^{+ 16}$ ${198}_{-{17}}^{+{16}}$	0.9996415 ± 0.0000090
Orbit 146	$150_{- 26}^{+ 22}$ ${150}_{-{26}}^{+{22}}$	0.9997236 ± 0.0000095

Notes. The parameters σ_w and f₀ are the additive noise jitter term and the flux normalisation factor, respectively. σ_w is expressed in parts-permillion (ppm) and is added to all error bars quadratically. A negative value of σ_w means that the error bars are shrunk. Each f₀ 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).

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