All Tables

Table A.1: Basic parameters of the FORS Deep Field galaxies.
1. ID from Heidt et al. (2003), 2. redshift, 3. luminosity distance, 4. lookback time, 5. signal/noise, 6. velocity dispersion corrected for aperture (see Sect. 2), 7. its error, 8.-11. FORS total magnitudes (SExtractor's MAG_BEST), 12. absolute restframe B magnitude, 3., 4., and 12. for $\Omega _{\rm matter}=0.3$ , $\Omega _{\lambda }=0.7$ , H₀ = 70 km s^-1 Mpc^-1.
Table A.2: Line strengths of fully corrected (see Sect. 2) Lick indices of the FORS Deep Field galaxies together with their errors and (by-eye) quality flags. Units are Å. Quality flags: 0: satisfactory, 1: a bit noisy, 2: in region of strong sky line, 6: affected by telluric B band, 7: affected by telluric A band, 8: affected by end of spectrum, 9: not visible.
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.