Table 3
Comparison between morphological parameters derived from HSC-SSP images used to train the low redshift network in this work and derived from GAMA-KiDS data in Pearson et al. (2019b).
| Parameter | Mean δ | Std δ | Outliers |
|---|---|---|---|
| Asymmetry (A) | −0.060 | 0.087 | 22 |
| Concentration (C) | −0.052 | 0.299 | 26 |
| Deviation (D) | 0.011 | 0.097 | 28 |
| Ellipticity asymmetry (Eli A) | −0.003 | 0.095 | 22 |
| Ellipticity centroid (Eli Cen) | −0.003 | 0.096 | 22 |
| Elongation asymmetry (Elo A) | 0.073 | 2.882 | 4 |
| Elongation centroid (Elo Cen) | 0.051 | 2.694 | 2 |
| Gini | 0.010 | 0.052 | 21 |
| Gini-M20 bulge (GMB) | 0.027 | 0.235 | 14 |
| Gini-M20 merger (GMM) | 0.013 | 0.068 | 24 |
| Intensity (I) | −0.023 | 0.160 | 38 |
| M20 | 0.029 | 0.200 | 28 |
| Multimode (M) | 0.000 | 0.158 | 55 |
| Sérsic amplitude(a) (SA) | 0.330 | 1.077 | 21 |
| Sérsic ellipticity (SE) | −0.044 | 0.150 | 33 |
| Sérsic index (n) | −0.433 | 6.744 | 9 |
| Smoothness (S) | −0.039 | 0.367 | 24 |
Notes. These differences are expressed the value from HSC-SSP morphological parameters subtracted from the GAMA-KiDS morphologies (δ): negative means imply that HSC-SSP morphologies are larger than GAMA-KiDS. (a)Comparison is made with surface brightness (mag arcsec−2), not the counts reported in Table 1 and Pearson et al. (2019a).
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