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Table 3

Morphological parameters of the original LARS galaxies at z ~ 0.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
LARS GrP20 GSB − rP20S M20 ell Ccirc Cell CminA S Npixel A S
Rest-UV
L01 0.70 0.68 –0.87 0.61 1.34 1.94 1.73 251.40 0.42 0.16
L02 0.73 0.72 –0.79 0.53 3.14 2.50 3.49 52.26 0.50 0.26
L03 0.63 0.64 –1.17 0.30 2.20 2.71 2.76 83.18 0.21 0.11
L05 0.72 0.68 –1.26 0.34 3.11 3.07 3.27 408.69 0.33 0.15
L07 0.62 0.62 –1.02 0.40 1.99 2.28 1.24 696.00 0.26 0.09
L08 0.62 0.65 –0.89 0.33 1.95 2.36 1.43 21.98 0.37 0.29
L09 0.71 0.75 –2.33 0.80 1.76 3.52 3.35 23.86 0.21 0.24
L10 0.67 0.68 –1.52 0.52 3.53 3.53 2.76 32.83 0.33 0.24
L11 0.58 0.79 –1.22 0.87 3.40 2.51 3.40 44.05 0.30 0.31
L12 0.67 0.68 –1.50 0.34 2.56 3.15 2.82 583.81 0.28 0.04
L13 0.72 0.67 –0.77 0.21 1.23 1.42 2.61 89.17 0.33 0.23
L14 0.74 0.68 –0.71 0.27 1.51 1.78 2.72 622.68 0.21 0.02
Rest-optical
L01 0.59 0.61 –1.09 0.64 1.72 2.48 2.53 21.91 0.29 0.09
L02 0.59 0.64 –1.36 0.69 2.96 3.58 2.89 4.25 0.14 0.31
L03 0.61 0.62 –2.16 0.45 3.32 4.02 3.42 50.72 0.09 0.05
L05 0.64 0.67 –1.57 0.73 3.27 3.22 4.77 64.96 0.33 0.15
L07 0.60 0.61 –1.68 0.60 3.28 3.56 2.97 14.60 0.24 0.10
L08 0.54 0.55 –1.05 0.23 2.10 2.28 1.78 36.82 0.31 0.16
L09 0.62 0.74 –1.13 0.83 2.03 1.96 4.35 11.38 0.45 0.34
L10 0.57 0.58 –1.87 0.54 3.08 3.56 3.31 9.95 0.13 0.15
L11 0.50 0.60 –1.25 0.85 3.46 2.52 3.46 18.70 0.20 0.23
L12 0.64 0.63 –1.90 0.46 3.70 3.34 3.35 54.74 0.33 0.13
L13 0.58 0.62 –1.52 0.55 2.43 2.99 3.67 3.98 0.18 0.30
L14 0.76 0.72 –1.32 0.10 2.92 2.92 3.01 35.24 0.32 0.13

Notes. Morphological parameters estimated for the original LARS galaxies, following the equations in Appendix A. (1) LARS id; (2) Gini coefficient estimated within the fixed-size segmentation map; (3) Gini coefficient estimated within the segmentation map built from the pixels with surface brightness larger than the value corresponding to that at the Petrosian radius; (4) M20; (5) SExtractor ellipticity 1-B/A; (6) concentration from circular apertures; (7) concentration from elliptical apertures; (8) concentration corresponding to the minimum of asymmetry; (9) signal-to-noise per pixel; (10) asymmetry; (11) clumpiness. As discussed in Appendix A, we could expect an uncertainty of ~10% in G, of < 5% in M20, and of ~20% in C. We could expect an even larger uncertainty in S. The difference in GrP20 and GSB − rP20S is generally marginal.

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