A song of interactions and mergers: The case of NGC 4709

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Table 5.

Best-fit parameters for the GCLF of NGC 4709.

Band	mag	A	μ	σ	M_TO	d	(m − M)
	(mag)		(mag)	(mag)	(mag)	(Mpc)	(mag)
g′₀	25.457	84.08 ± 0.09	25.22 ± 0.02	1.05 ± 0.02	−7.20 ± 0.20	30.49 ± 3.35	32.42 ± 0.24
r′₀	24.627	$94 . 77_{- 1.66}^{+ 1.67}$ $94.77^{+1.67}_{-1.66}$	24.79 ± 0.05	1.12 ± 0.02	−7.56 ± 0.20	29.46 ± 5.04	32.35 ± 0.37
i′₀	25.332	$74 . 92_{- 0.78}^{+ 0.82}$ $74.92^{+0.82}_{-0.78}$	24.53 ± 0.02	1.22 ± 0.02	−7.82 ± 0.20	29.49 ± 3.18	32.35 ± 0.23

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 three columns show the absolute turnover magnitude for the filter considered, and the calculated distance and distance modulus for NGC 4709.

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