Table 4.
Magnitudes in broad-band filters of the SSPs models.
| IMF | Z | log t | U | B | V | R | u | g | r | i | z |
|---|---|---|---|---|---|---|---|---|---|---|---|
| CHA | 0.02 | 5.00 | −0.340 | 0.674 | 0.905 | 1.031 | 0.773 | 1.122 | 1.559 | 1.967 | 2.247 |
| CHA | 0.02 | 5.48 | −0.380 | 0.635 | 0.868 | 0.995 | 0.732 | 1.084 | 1.522 | 1.931 | 2.213 |
| CHA | 0.02 | 5.70 | −0.422 | 0.594 | 0.826 | 0.953 | 0.691 | 1.044 | 1.480 | 1.889 | 2.171 |
| CHA | 0.02 | 5.85 | −0.465 | 0.550 | 0.781 | 0.907 | 0.647 | 0.999 | 1.435 | 1.843 | 2.124 |
| CHA | 0.02 | 6.00 | −0.526 | 0.493 | 0.726 | 0.853 | 0.586 | 0.943 | 1.380 | 1.789 | 2.071 |
| CHA | 0.02 | 6.10 | −0.635 | 0.387 | 0.619 | 0.745 | 0.477 | 0.836 | 1.273 | 1.682 | 1.964 |
Notes. Column 1 shows the IMF, column 2 corresponds to the stellar metallicity of the SSP, and column 3 is the age. Columns 4 to 7 are the Johnson-Cousins-Glass system magnitudes U, B, V, and R in the Vega system, while columns 8–12 refer to the magnitudes u, g, r, i, and z for the SDSS filters AB system. The whole table is available at the CDS.
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