A new method to compute limb-darkening coefficients for stellar atmosphere models with spherical symmetry: the space missions TESS, Kepler, CoRoT, and MOST

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Volume 618 (October 2018)

A&A, 618 (2018) A20

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Table 1.

Limb-darkening coefficients for the space mission photometric system FSM.

Name	Source	Range T_eff	Range log g	Vel Turb.	Filter	Fit/equation/model
Table2	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	TESS	LSM/Eq. (1), FSM
Table3	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	TESS	LSM/Eq. (1), FSM
Table4	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	TESS	LSM/Eq. (2), FSM
Table5	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	TESS	LSM/Eq. (2), FSM
Table6	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	Kepler	LSM/Eq. (1), FSM
Table7	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	Kepler	LSM/Eq. (1), FSM
Table8	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	Kepler	LSM/Eq. (2), FSM
Table9	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	Kepler	LSM/Eq. (2), FSM
Table10	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	CoRoT	LSM/Eq. (1), FSM
Table11	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	CoRoT	LSM/Eq. (1), FSM
Table12	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	CoRoT	LSM/Eq. (2), FSM
Table13	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	CoRoT	LSM/Eq. (2), FSM
Table14	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	MOST	LSM/Eq. (1), FSM
Table15	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	MOST	LSM/Eq. (1), FSM
Table16	PHOENIX-DRIFT	1500 K–3000 K	2.5–5.5	2 km s⁻¹	MOST	LSM/Eq. (2), FSM
Table17	PHOENIX-COND	2300 K–12 000 K	2.5–6.0	2 km s⁻¹	MOST	LSM/Eq. (2), FSM

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