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Table 4

Morphological parameters of galaxies.

ID n 850 b / a E v B E v R
[mag] [kpc] [mag/arcsec2] [mag] [mag] [kpc] [mag/arcsec2] mag

1 3.9 0.7 21.79 7.8 (8.2) ± 1.2 20.8(20.9) ± 0.4 1.36(1.39) . 19.21 6.3(6.5) ± 0.2 19.1(19.2) ± 0.1 1.16(1.16)
2 6.3 0.7 21.08 6.5 (3.2) ± 0.7 19.8(18.3) ± 0.3 2.35(2.21) . 18.51 9.4(4.6) ± 0.2 19.3(17.7) ± 0.05 1.90(1.86)
3 2.6 0.5 21.79 1.3 (1.7) ± 0.1 17.0(17.6) ± 0.1 1.60(1.62) . 19.51 1.6(2.0) ± 0.1 16.5(16.9) ± 0.1 1.33(1.39)
4 4.4 0.7 20.38 16.7(13.3) ± 5.6 21.2(20.7) ± 0.8 2.13(2.03) . 18.26 10.3(8.7) ± 0.9 19.2(18.9) ± 0.2 1.73(1.75)
5 3.6 0.9 22.68 1.7 (1.5) ± 0.2 18.6(18.4) ± 0.3 2.35(2.21) . 19.93 1.7(1.6) ± 0.2 17.0(16.8) ± 0.5 1.90(1.86)
606 4.3 0.6 22.22 2.4 (2.2) ± 0.2 18.8(18.6) ± 0.2 2.35(2.21) . 19.69 3.0(2.9) ± 0.3 18.0(17.9) ± 0.2 1.90(1.86)
590 2.8 0.7 22.44 2.4 (3.4) ± 0.1 19.0(19.8) ± 0.2 1.92(1.85) . 19.93 2.3(2.9) ± 0.2 17.7(18.2) ± 0.2 1.56(1.49)
568 4.2 0.4 22.82 1.1 (0.8) ± 0.1 17.7(17.2) ± 0.2 1.92(1.85) . 20.39 1.2(1.2) ± 0.2 16.7(16.7) ± 0.3 1.58(1.61)
719 6.0 0.7 22.73 0.9 (0.7) ± 0.1 17.2(16.6) ± 0.2 1.42(1.43) . 21.73 2.4(1.8) ± 0.6 19.6(19.9) ± 0.5 1.21(1.20)
1250 2.2 0.8 23.20 2.1 (3.6) ± 0.3 19.6(20.7) ± 0.2 2.32(2.17) . 20.92 2.4(3.5) ± 0.2 18.7(19.6) ± 0.1 1.88(1.83)
1260 3.9 0.7 23.75 2.1 (3.3) ± 0.4 20.3(21.3) ± 0.6 2.98(2.78) . 21.65 1.9(2.9) ± 0.2 18.9(19.8) ± 0.3 2.25(2.22)
173 3.2 0.8 23.63 0.5 (0.5) ± 0.1 16.9(16.9) ± 0.4 1.21(1.31) . 21.23 0.8(0.9) ± 0.2 16.6(16.9) ± 0.5 1.03(1.09)
1160 4.6 0.6 22.54 2.1 (1.8) ± 0.3 18.9(18.6) ± 0.4 1.58(1.52) . 20.19 2.7(2.4) ± 0.3 18.3(18.0) ± 0.3 1.31(1.30)
657 2.4 0.5 22.12 1.7 (2.1) ± 0.2 18.0(18.5) ± 0.3 2.35(2.21) . 19.93 1.7(2.1) ± 0.2 17.0(17.5) ± 0.5 1.90(1.86)
626 4.2 0.6 21.45 2.1 (2.5) ± 0.3 17.8(18.1) ± 0.3 2.35(2.21) . 19.93 2.2(2.5) ± 0.3 17.5(17.8) ± 0.5 1.90(1.86)
471 4.6 0.9 23.33 2.3 (1.9) ± 0.3 19.8(19.4) ± 0.4 2.13(2.03) .

Notes. Sérsic index n, axial ratio b/a, apparent magnitude and effective radius [kpc] as derived from the fitting to the surface brightness profile in the F850LP image and in the F160W image. The values in parentheses have been obtained assuming n = 4. The terms EvB,R represent the luminosity evolution that the stellar population of each galaxy experiences in the B and R bands, respectively, in the ~8.6 Gyr from z = 1.27 to z = 0, according to its own age at z = 1.27 and SFH using the BC03 models (see text for a detailed description). The values in parentheses have been obtained using Maraston’s models (2005).

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