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Table 5

Our sample of high-z ETGs.

Object RA Dec z Re n b/a σ σoff σe log(M,cha/M) K
(kpc) (km s-1) (km s-1) (km s-1)

S2F1-511 03:06:34.04 +00:02:30.9 1.267 2.09 ± 0.07 3.3 0.60 269 [–4 ÷ 12] 281 11.05 18.1 ± 0.1
S2F1-633 03:06:35.10 +00:04:43.6 1.297 2.59 ± 0.11 4.1 0.53 434 [–24 ÷ –7] 447 11.48 18.2 ± 0.1
S2F1-527 03:06:43.34 +00:02:44.8 1.331 1.57 ± 0.24 3.1 0.88 226 [–16 ÷ 1] 240 11.14 18.3 ± 0.1
S2F1-389 03:06:28.03 +00:00:31.6 1.406 2.10 ± 0.18 4.5 0.85 224 [–30 ÷ –18] 234 11.14 18.2 ± 0.1
S2F1-443 03:06:31.76 +00:01:13.4 1.910 3.36 ± 0.15 1.9 0.79 352 [–21 ÷ 8] 357 11.59 18.4 ± 0.1

Notes. Column 1: id number; Col. 2: RA; Col. 3: Dec; Col. 4: redshift; Col. 5: circularized effective radius in kpc; Col. 6: Sersic index; Col. 7: axis ratio; Col. 8: velocity dispersion as measured within the 1′′ aperture slit; Col. 9: the range in which varies the offset factor σoff to be applied to σ according to the simulation of Appendix B; Col. 10: velocity dispersion as measured within the effective radius; Col. 11: stellar mass derived with BC03 code and Chabrier IMF; Col. 12: Vega magnitude in K-band (Saracco et al. 2009).

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