Table A.3: Fully corrected Fe 5335 Lick index and SSP model ages, metallicities [Z/H], and Mg/Fe ratios [ $\alpha$ /Fe] of the FORS Deep Field galaxies. Average errors in $\log$ (age), [Z/H], and [ $\alpha$ /Fe] are 0.18 dex, 0.2 dex, and 0.15 dex, respectively. In Col. 8 it is indicated, which Balmer line was used to derive the model age. The last four columns are based on the HST/ACS images: ACS total I magnitude (GALFIT), mean surface brightness in B within $R_{\rm e}$ corrected for cosmological dimming, and half-light radius (GALFIT). Physical units for $\Omega _{\rm matter}=0.3$ , $\Omega _{\lambda }=0.7$ , H₀ = 70 km s^-1 Mpc^-1.
FDF Fe 5335 dFe 5335 qFe 5335 age [Z/H] [ $\alpha$ /Fe] Balmer $I_{\rm tot}$ $\langle\mu_B\rangle_{\rm e}$ $R_{\rm e}$ $\log R_{\rm e}$

Å Å Gyr line [mag] [mag/sq.as.] [arcsec] [kpc]

1161 2.5 0.3 1 5.3 -0.07 -0.09 H $\gamma_{\rm F}$ 19.9 20.3 0.40 0.33

4285 1.6 0.3 2 6.3 -0.15 0.44 H $\delta_{\rm F}$ 19.9 20.3 0.40 0.33

5011 * * 9 * * * * 20.8 20.6 0.50 0.54

5908 2.6 0.2 0 6.5 0.32 0.26 H $\beta$ 16.3 21.5 2.50 0.95

6307 1.8 0.5 0 8.8 -0.10 0.37 H $\beta$ 19.8 20.8 0.59 0.53

6336 * * 9 * * * * 21.2 21.8 0.50 0.46

6338 2.5 0.3 0 5.0 0.16 0.12 H $\beta$ * * * *

6439 2.3 0.5 0 1.9 0.20 0.15 H $\beta$ 19.1 19.2 0.35 0.27

7116 2.5 0.4 2 2.6 0.25 0.15 H $\beta$ 20.6 19.7 0.25 0.16

7459 * * 9 * * * * * * * *

7796 2.7 0.4 0 1.3 0.65 0.12 H $\gamma_{\rm F}$ 20.1 21.8 0.75 0.61

8372 2.3 0.4 0 7.2 0.16 0.28 H $\beta$ 18.6 19.8 0.40 0.17

8626 3.4 0.2 1 * * * * 17.9 21.0 1.45 0.90

**Table A.3:** Fully corrected Fe 5335 Lick index and SSP model ages, metallicities [Z/H], and Mg/Fe ratios [ $\alpha$ /Fe] of the FORS Deep Field galaxies. Average errors in $\log$ (age), [Z/H], and [ $\alpha$ /Fe] are 0.18 dex, 0.2 dex, and 0.15 dex, respectively. In Col. 8 it is indicated, which Balmer line was used to derive the model age. The last four columns are based on the HST/ACS images: ACS total I magnitude (GALFIT), mean surface brightness in B within $R_{\rm e}$ corrected for cosmological dimming, and half-light radius (GALFIT). Physical units for $\Omega _{\rm matter}=0.3$ , $\Omega _{\lambda }=0.7$ , H₀ = 70 km s^-1 Mpc^-1.
FDF	Fe 5335	dFe 5335	qFe 5335	age	[Z/H]	[ $\alpha$ /Fe]	Balmer	$I_{\rm tot}$	$\langle\mu_B\rangle_{\rm e}$	$R_{\rm e}$	$\log R_{\rm e}$
	Å	Å		Gyr			line	[mag]	[mag/sq.as.]	[arcsec]	[kpc]
1161	2.5	0.3	1	5.3	-0.07	-0.09	H $\gamma_{\rm F}$	19.9	20.3	0.40	0.33
4285	1.6	0.3	2	6.3	-0.15	0.44	H $\delta_{\rm F}$	19.9	20.3	0.40	0.33
5011	*	*	9	*	*	*	*	20.8	20.6	0.50	0.54
5908	2.6	0.2	0	6.5	0.32	0.26	H $\beta$	16.3	21.5	2.50	0.95
6307	1.8	0.5	0	8.8	-0.10	0.37	H $\beta$	19.8	20.8	0.59	0.53
6336	*	*	9	*	*	*	*	21.2	21.8	0.50	0.46
6338	2.5	0.3	0	5.0	0.16	0.12	H $\beta$	*	*	*	*
6439	2.3	0.5	0	1.9	0.20	0.15	H $\beta$	19.1	19.2	0.35	0.27
7116	2.5	0.4	2	2.6	0.25	0.15	H $\beta$	20.6	19.7	0.25	0.16
7459	*	*	9	*	*	*	*	*	*	*	*
7796	2.7	0.4	0	1.3	0.65	0.12	H $\gamma_{\rm F}$	20.1	21.8	0.75	0.61
8372	2.3	0.4	0	7.2	0.16	0.28	H $\beta$	18.6	19.8	0.40	0.17
8626	3.4	0.2	1	*	*	*	*	17.9	21.0	1.45	0.90

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data analysis
	3 The kinematic scaling relations
	4 The Mg ${_\textit {{b}}{-}\sigma }$ relation
	5 Line diagnostic diagrams
	6 The stellar populations
	7 Summary and discussion
	Appendix A: Parameters of the FORS Deep Field galaxies
	References