Table 1: Basic information on host galaxies. According to the column the references are: (1) de Vaucouleurs et al. (1991); (2) Tonry et al. (2001); (3) Tully (1988); (4) and (5) Kissler-Patig et al. (1997), Ashman & Zepf (1998).
Galaxy Type (m-M)_V M_B $N_{\rm GC}^{a}$ $S_{\rm N}^{b}$

(1) (2) (3) (4) (5)

NGC 1380 -2/LA 31.23 $\pm$ 0.18 -20.04 $560\pm30$ $1.5\pm0.5$

NGC 2434 -5/E0+ 31.67 $\pm$ 0.29 -19.48 ... ...

NGC 3115 -3/L- 29.93 $\pm$ 0.09 -19.19 $520\pm120$ $1.6\pm0.4$

NGC 3379 -5/E1 30.12 $\pm$ 0.11 -19.39 $300\pm160$ $1.2\pm0.6$

NGC 3585 -5/E6 31.51 $\pm$ 0.18 -20.93 ... ...

NGC 5846 -5/E0 31.98 $\pm$ 0.20 -21.16 $2200\pm1300$ $3.5\pm2.1$

NGC 7192 -4.3/E+ 32.89 $\pm$ 0.32 -20.55 ... ...

^a Total number of globular clusters.
^b Specific frequency, $S_{\rm N}=N_{\rm GC}\times 10^{~ 0.4\cdot(M_V + 15)}$ (Harris & van den Bergh 1981).

**Table 1:** Basic information on host galaxies. According to the column the references are: (1) de Vaucouleurs et al. (1991); (2) Tonry et al. (2001); (3) Tully (1988); (4) and (5) Kissler-Patig et al. (1997), Ashman & Zepf (1998).
Galaxy	Type	(m-M)_V	M_B	$N_{\rm GC}^{a}$	$S_{\rm N}^{b}$
	(1)	(2)	(3)	(4)	(5)
NGC 1380	-2/LA	31.23 $\pm$ 0.18	-20.04	$560\pm30$	$1.5\pm0.5$
NGC 2434	-5/E0+	31.67 $\pm$ 0.29	-19.48	...	...
NGC 3115	-3/L-	29.93 $\pm$ 0.09	-19.19	$520\pm120$	$1.6\pm0.4$
NGC 3379	-5/E1	30.12 $\pm$ 0.11	-19.39	$300\pm160$	$1.2\pm0.6$
NGC 3585	-5/E6	31.51 $\pm$ 0.18	-20.93	...	...
NGC 5846	-5/E0	31.98 $\pm$ 0.20	-21.16	$2200\pm1300$	$3.5\pm2.1$
NGC 7192	-4.3/E+	32.89 $\pm$ 0.32	-20.55	...	...

Source LaTeX | All tables | In the text

	1 Introduction
	2 Selection of data
	3 Reducing systematic uncertainties
	4 Ages and metallicities
	5 [ ${\alpha }$ /Fe] ratios
	6 Discussion
	7 Summary and conclusions
	References