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Table 16.
Best-fit parameters for the GCLF.
| Band | mag | A | μ | σ | MTO | d |
|---|---|---|---|---|---|---|
| (mag) | (mag) | (mag) | (mag) | (Mpc) | ||
| g′ | 26.589 | 598.89 ± 17.37 | 25.88 ± 0.13 | 1.34 ± 0.09 | −7.2 ± 0.20 | 41.39 ± 4.54 |
| r′ | 26.166 | 553.62 ± 14.74 | 25.27 ± 0.13 | 1.43 ± 0.08 | −7.56 ± 0.20 | 36.81 ± 4.01 |
| i′ | 25.911 | 558.95 ± 19.74 | 25.04 ± 0.16 | 1.39 ± 0.11 | −7.82 ± 0.20 | 37.35 ± 4.41 |
Notes. The columns show the band, the magnitude up to which the LF was fitted (mag), the amplitude (A), the mean (μ), and the standard deviation (σ). The last two columns show the absolute turnover magnitude for the filter considered and the calculated distance of NGC 4696.
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