Gaia broad band photometry | Astronomy & Astrophysics (A&A)

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Table 2

Synthetic stellar libraries.

Name	T_eff (K)	log g (dex)	[Fe/H] (dex)	Notes

O, B stars¹	15 000–50 000	1.0–5.0	–5.0–+1.0	TLUSTY code, NLTE, wind, mass loss
Ap/Bp stars²	7000–16 000	4.0	+0.0	LLmodels code, non-solar abundance
B-F stars³	6000–16 000	2.5–4.5	+0.0	LLmodels
MARCS⁴	4000–8000	–0.5–5.5	–5.0–+1.0	Variations in individual α-elements abundances
C stars⁵,⁶	4000–8000	0.0–5.0	–5.0–+0.0	ΔT_eff = 500 K; [C/Fe] = 0, 1, 2, 3; [α/Fe] = +0.0, +0.4
PHOENIX⁷	3000–10 000	–0.5–5.5	–3.5–+0.5	ΔT_eff = 100 K; [α/Fe] = –0.2–+0.8, Δ[α/Fe] = 0.2
Ultra-cool dwarfs⁸	100–6000	0.0–6.0	+0.0	Different dust model implemented;


BaSeL3.1⁹	2000–50 000	–1.0 –5.5	–2.0 – 0.5	Based on Kurucz (1992); Fluks et al. (1994); Bessell et al. (1989, 1991);
				Hauschildt et al. (1999); and Scholz (1997)

References.

Bouret et al. (2008);

Kochukhov & Shulyak (2008);

Shulyak et al. (2004);

⁴

Gustafsson et al. (2008);

⁵

Alvarez & Plez (1998);

⁶

Brott & Hauschildt (2005);

⁷

Allard et al. (2000);

⁸

Martayan et al. (2008);

⁹

Westera et al. (2002).

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