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Table 4

Sample of high-z ETGs collected from literature.

Object RA Dec z Re n b/a Camera-Filter σ σe log M
h:m:s d:m:s (kpc) (km s-1) (km s-1) (M)

A17300(1) 14:18:39.78 52:41:59.51 1.423 2.9 ± 0.51(2) 5.3 ... HST/WFC3-F160W 265 ± 7 272 ± 7 11.26
A21129(1) 14:19:10.56 52:46:26.79 1.583 1.5 ± 0.27(2) 5.0 ... HST/WFC3-F160W 260 ± 9 278 ± 10 11.18
C21434(1) 10:00:36.10 2:32:13.77 1.522 1.9 ± 0.33(2) 3.1 ... HST/WFC3-F160W 218 ± 16 230 ± 17 11.20
C20866(1) 9:59:18.64 2:31:39.03 1.522 2.4 ± 0.42(2) 3.0 ... HST/WFC3-F160W 272 ± 23 282 ± 23 11.30
21750(3) 215.03490 52.9829 1.242 2.59 ± 0.26 5.2 0.57 HST/WFC3-F160W ... 259 ± 16 11.03
7310(3) 150.05791 2.2904 1.255 4.34 ± 0.43 3.8 0.87 HST/WFC3-F160W ... 167 ± 15 11.13
S2F1-142(4) 03:06:36.51 00:03:01.0 1.386 3.04 ± 0.12 3.5 0.74 HST/NIC2-F160W 340 347 11.54

Notes. Column 1: ID; Col. 2: RA; Col. 3: Dec; Col. 4; redshift; Col. 5: circularized effective radius; Col. 6: Sersic index; Col. 7: axis ratio; Col. 8: filter adopted to derive the surface brightness parameters; Col. 9: measured velocity dispersion; Col. 10: velocity dispersion within Re; Col. 11: stellar masses. References for the velocity dispersion values are listed near the ID value. When a data of the galaxy comes from a paper other than that in which the σ is published, the new reference is specified near its value.

Reference. (1) Bezanson et al. (2013); (2) van de Sande et al. (2013); (3) Belli et al. (2014); (4) Longhetti et al. (2014).

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