Table 1
Total sample of ⟨ z ⟩ = 1.4 galaxies.
| Object | z | Re | n | Camera-Filter | σ | σe | logM⋆ |
| (kpc) | (km s-1) | (km s-1) | (M⊙) | ||||
|
|
|||||||
| S2F1-5111 | 1.267 | 2.09 ± 0.07 | 3.3 | HST/NIC2-F160W | 269 | 281 ± 23 | 11.05 |
| S2F1-6331 | 1.297 | 2.59 ± 0.11 | 4.1 | HST/NIC2-F160W | 434 | 447 ± 27 | 11.48 |
| S2F1-5271 | 1.331 | 1.57 ± 0.24 | 3.1 | HST/NIC2-F160W | 226 | 240 ± 26 | 11.14 |
| S2F1-3891 | 1.406 | 2.10 ± 0.18 | 4.5 | HST/NIC2-F160W | 224 | 234 ± 45 | 11.14 |
| 22392 | 1.415 | 2.16 ± 0.433 | 2.23 | HST/ACS-F850LP | 111 ± 35 | 116 ± 37 | 10.643 |
| 24702 | 1.415 | 1.81 ± 0.363 | 4.23 | HST/ACS-F850LP | 141 ± 26 | 150 ± 28 | 10.943 |
| A173004 | 1.423 | 2.9 ± 0.515 | 5.3 | HST/WFC3-F160W | 265 ± 7 | 272 ± 7 | 11.26 |
| A211294 | 1.583 | 1.5 ± 0.275 | 5.0 | HST/WFC3-F160W | 260 ± 9 | 278 ± 10 | 11.18 |
| C214344 | 1.522 | 1.9 ± 0.335 | 3.1 | HST/WFC3-F160W | 218 ± 16 | 230 ± 17 | 11.20 |
| C208664 | 1.522 | 2.4 ± 0.425 | 3.0 | HST/WFC3-F160W | 272 ± 23 | 282 ± 23 | 11.30 |
| 329156 | 1.261 | 1.33 ± 0.13 | 6.3 | HST/WFC3-F160W | 271 ± 17 | 10.88 | |
| 23416 | 1.266 | 1.21 ± 0.12 | 3.8 | HST/WFC3-F160W | 196 ± 27 | 10.87 | |
| 290596 | 1.278 | 1.62 ± 0.16 | 4.3 | HST/WFC3-F160W | 211 ± 16 | 10.90 | |
| 23376 | 1.327 | 1.54 ± 0.15 | 3.5 | HST/WFC3-F160W | 284 ± 20 | 11.04 | |
| 147586 | 1.331 | 0.83 ± 0.08 | 2.2 | HST/WFC3-F160W | 165 ± 16 | 10.71 | |
| 50206 | 1.415 | 2.07 ± 0.20 | 4.6 | HST/WFC3-F160W | 180 ± 54 | 10.83 | |
| 138806 | 1.432 | 0.87 ± 0.08 | 2.6 | HST/WFC3-F160W | 179 ± 70 | 10.64 | |
| S2F1-1427 | 1.386 | 3.04 ± 0.12 | 3.5 | HST/NIC2-F160W | 340 |
347 |
11.54 |
Notes. Column 1: ID, Column 2: redshift, Column 3: effective radius, Column 4: Sersic index, Column 5: filter adopted to derive the surface brightness parameters, Column 6: measured velocity dispersion, Column 7: velocity dispersion corrected to Re aperture following Cappellari et al. (2006), Column 8: Stellar mass. References for the velocity dispersion values are listed near the ID value. When a data of the galaxy comes from a paper different from the one where the σ is published, the new reference is specified near its value. 1Gargiulo et al. (2014); 2Cappellari et al. (2009); 3Cimatti et al. (2008); 4Bezanson et al. (2013); 5van de Sande et al. (2013); 6Belli et al. (2014); 7Longhetti et al. (2014).
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