Table 3.
Results from the three-Gaussian fit method.
| mF322W2 | rMS | gMS | bMS | rMS/N | gMS/N | bMS/N | σrMS | σgMS | σbMS |
 |
 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [%] | [%] | [%] | |||||||||
| 20.0 − 20.5 | 632 ± 25 | 259 ± 16 | 216 ± 15 | 57 ± 3 | 23 ± 2 | 20 ± 1 | 0.16 | 0.18 | 0.18 | 0.02 | 0.02 |
| 20.5 − 21.0 | 524 ± 23 | 263 ± 16 | 307 ± 18 | 48 ± 3 | 24 ± 2 | 28 ± 2 | 0.12 | 0.16 | 0.19 | 0.02 | 0.02 |
| 21.0 − 21.5 | 382 ± 20 | 231 ± 15 | 183 ± 14 | 48 ± 3 | 29 ± 2 | 23 ± 2 | 0.12 | 0.14 | 0.18 | 0.03 | 0.03 |
| 21.5 − 22.0 | 291 ± 17 | 190 ± 14 | 136 ± 12 | 47 ± 3 | 31 ± 3 | 22 ± 2 | 0.11 | 0.16 | 0.16 | 0.03 | 0.04 |
| 22.0 − 22.5 | 223 ± 15 | 121 ± 11 | 101 ± 10 | 50 ± 4 | 27 ± 3 | 23 ± 3 | 0.10 | 0.16 | 0.19 | 0.05 | 0.05 |
| 22.5 − 23.0 | 159 ± 13 | 95 ± 10 | 44 ± 7 | 53 ± 5 | 32 ± 4 | 15 ± 2 | 0.14 | 0.15 | 0.15 | 0.07 | 0.07 |
| 23.0 − 23.5 | 95 ± 10 | 33 ± 6 | 18 ± 4 | 65 ± 9 | 23 ± 4 | 12 ± 3 | 0.20 | 0.23 | 0.13 | 0.08 | 0.11 |
| 23.5 − 24.0 | 51 ± 7 | 22 ± 5 | 0 ± 0 | 70 ± 13 | 30 ± 7 | 0 ± 0 | 0.21 | 0.16 | 0.00 | 0.08 | 0.14 |
| 2357 ± 49 | 1214 ± 35 | 1005 ± 32 | 52 ± 2 | 26 ± 1 | 22 ± 2 | ||||||
Notes. Values are derived using the method illustrated in panels (1c) to (1l) of Fig. 13 for the three sequences. The table also includes the dispersion values (σ) for each Gaussian component for both the real and artificial stars. The final row presents the total number of stars and the weighted average of the ratios for the three sequences.
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