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Table 1

Synthetic stellar populations used for SED fitting.

Name Age [Fe/H] Fract.
[Gyr]
(1) (2) (3) (4) (5) (6) (7)

B07-1 0.7 0.40 0.76 0.78 0.72 0.014
B07-3 0.4–1 0.05 0.47 0.50 0.56 0.003
B07-4 7–12 0.03 5.05 3.87 3.12 0.983

M05-1 1 0.00 1.11 1.00 0.85 0.008
M05-2 2 0.00 2.18 1.70 1.43 0.002
M05-3 4 0.00 3.99 3.03 2.56 0.214
M05-4 12 0.00 11.6 8.08 6.47 0.767
M05-5 12 –0.33 9.00 6.60 5.37 0.009

GALEV-1 1, 10 0.04 2.88 3.14 2.92 0.004
GALEV-2 2, 11 0.07 4.35 4.13 3.65 0.011
GALEV-3 4, 13 0.09 7.58 6.20 5.23 0.089
GALEV-4 12 0.12 4.63 4.55 4.05 0.015
GALEV-5 12 0.18 10.9 8.33 6.86 0.881

Notes. The columns contain the following: (1) stellar population model; for B07 models the number is as in the original paper; (2) approximate age of the dominant star-formation epoch(s); (3) average metallicity of the stars; (4)–(6) mass-to-light ratio in the gri filters; (7) total stellar mass fraction in M 31 of the corresponding stellar population.

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