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Table 1.

Summary of data used.

Data Resolution Magnitude limit Redshift range Mass limit Training sample Complete sample
(arcsec) log(M/M) per class (Mass limited)
SDSS 1.4 17.77 0.005 <  z ≤ 0.1 10.1 3003 206 037

KiDS 0.77 19.8 (a) 0.00 <  z ≤ 0.15 9.6 1917 1270

CANDELS-z000 0.15 24.5 0.00 <  z ≤ 0.60 8.3 694 (b) 2072
CANDELS-z060 0.15 24.5 0.60 <  z ≤ 0.85 8.7 694 (b) 2004
CANDELS-z085 0.15 24.5 0.85 <  z ≤ 1.21 9.1 694 (b) 2031
CANDELS-z121 0.15 24.5 1.21 <  z ≤ 1.66 9.4 694 (b) 2010
CANDELS-z166 0.15 24.5 1.66 <  z ≤ 4.00 9.9 694 (b) 1910

Notes. The SDSS and KiDS limiting magnitudes are in r-band while the CANDELS limiting magnitude in H-band.

(a)

As the training set is derived from GAMA classifications, the limiting magnitude is that of the GAMA survey not that of the KiDS survey.

(b)

The CANDELS network was trained with 694 galaxies per class for galaxies with 0.00 <  z ≤ 4.00. The galaxies were split into the redshift bins shown after classification.

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