Doppler beaming factors for white dwarfs, main sequence stars, and giant stars - Limb-darkening coefficients for 3D (DA and DB) white dwarf models

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Table A.1.

Doppler beaming factors for the Kepler, TESS, Gaia, HiPERCAM, Sloan, and UBVRI photometric systems.

Name	Source	Range T_eff	Range log g	log [H/He]	Beaming/Filters
Table 1	DA	3750 K–60 000 K	5.0–9.5	0.00	Kepler/TESS/Gaia/HiPERCAM
Table 2	DB	10 000 K–40 000 K	5.5–9.5	−10.0	Kepler/TESS/Gaia/HiPERCAM
Table 3	DBA	11 000 K–40 000 K	7.0–9.0	−2.0	Kepler/TESS/Gaia/HiPERCAM
Table 4	DA-NLTE	40 000 K–100 000 K	6.0–9.5	0.0	Kepler/TESS/Gaia/HiPERCAM
Table 5	DA	3750 K–60 000 K	5.0–9.5	0.0	Sloan/UBVRI
Table 6	DB	10 000 K–40 000 K	5.5–9.5	−10.0	Sloan/UBVRI
Table 7	DBA	11 000 K–40 000 K	7.0–9.0	−2.0	Sloan/UBVRI
Table 8	DA-NLTE	40 000 K–100 000 K	6.0–9.5	0.0	Sloan/UBVRI
Table 9	ATLAS9	3500 K–50 000 K	0.0–5.0	−2.5–0.5 ^(a)	Kepler/TESS/Gaia/HiPERCAM
Table 10	ATLAS9	3500 K–50 000 K	0.0–5.0	−2.5–0.5 ^(a)	Sloan/UBVRI

Notes.

^(a)

Values of metallicities for the ATLAS9 models.

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