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Table 3:

Line-strength indices in our sample of red-galaxies with S/N(Å) > 10 and no- or weak-emission lines. The number between brackets after the indices values indicates the presence (1) or not (0) of sky-subtraction residuals or telluric absorptions inside the definition passband of the index. Only those indices with labels (0) are used in our analysis. Type: Indicate the presence (2) or not (1) of weak ( $\rm [OII]<7$ Å) emission lines. Last column lists the measured velocity dispersion and its error. This is only a portion of the table, shown for guidance regarding its format and content. The full table is electronically available at CDS and at http://www.ucm.es/info/Astrof/psb/ediscs.html
  D4000 H $\delta_{\rm A}$ H $\delta_{\rm F}$ CN2 Ca4227 G4300 H $\gamma_{\rm A}$
1018471-1210513 1.83 $\pm $ 0.01 (1) 1.28 $\pm $ 0.41 (0) 2.11 $\pm $ 0.27 (0) 0.027 $\pm $ 0.015 (0) 1.27 $\pm $ 0.23 (0) 2.71 $\pm $ 0.43 (0) $-1.53\pm0.47$ (0)
1018464-1211205 2.22 $\pm $ 0.02 (1) $-0.18\pm0.69$ (0) 0.84 $\pm $ 0.47 (0) 0.038 $\pm $ 0.024 (0) 0.87 $\pm $ 0.38 (0) 4.86 $\pm $ 0.65 (0) $-4.75\pm0.81$ (0)
1018467-1211527 2.13 $\pm $ 0.01 (0) $-0.97\pm0.29$ (0) 0.63 $\pm $ 0.19 (0) 0.108 $\pm $ 0.010 (0) 0.48 $\pm $ 0.16 (0) 5.10 $\pm $ 0.26 (0) $-5.55\pm0.33$ (0)
1018401-1214013 1.98 $\pm $ 0.02 (0) $-0.57\pm$0.65 (0) 0.40 $\pm $ 0.45 (0) 0.072 $\pm $ 0.022 (0) 0.53 $\pm $ 0.37 (0) 7.13 $\pm $ 0.57 (0) $-4.71\pm0.76$ (0)
  H $\gamma _{\rm F}$ Fe4383 Ca4455 Fe4531 type $\sigma\pm \rm err$  
1018471-1210513 0.52 $\pm $ 0.28 (0) 3.71 $\pm $ 0.68 (0) 0.67 $\pm $ 0.38 (0) 3.28 $\pm $ 0.58 (0) 2 245.9 $\pm $ 15.8  
1018464-1211205 $-2.01\pm0.52$ (0) 4.10 $\pm $ 1.09 (0) 0.91 $\pm $ 0.60 (0) 3.47 $\pm $ 0.93 (0) 1 279.9 $\pm $ 27.6  
1018467-1211527 $-1.73\pm0.21$ (0) 3.27 $\pm $ 0.44 (0) 0.98 $\pm $ 0.24 (0) 3.03 $\pm $ 0.38 (0) 1 211.1 $\pm $ 14.8  
1018401-1214013 $-0.29\pm0.45$ (0) 1.77 $\pm $ 1.06 (0) 0.71 $\pm $ 0.57 (0) 1.37 $\pm $ 0.91 (0) 1 129.2 $\pm $ 21.0  

Source LaTeX | All tables | In the text

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