Table 6.
OTELO DNN missmatches.
| ID | OTELO | DNN | Prob. | zphot | n | C | Elong. | Size |
|---|---|---|---|---|---|---|---|---|
| (px2) | ||||||||
| 267 | LT | ET r | 0.32 | 0.77 | 1.59 | 3.55 | 1.88 | 259 |
| 496 | LT | ET v | 0.12 | 0.70 | 2.54 | 3.54 | 1.22 | 231 |
| 1895 | ET | LT r | 1.00 | 0.04 | 0.72 | 3.47 | 1.22 | 61 |
| 2818 | LT | ET v | 0.12 | 0.72 | 3.29 | 3.32 | 1.39 | 255 |
| 3680 | ET | LT v | 1.00 | 1.45 | 0.36 | 2.14 | 1.49 | 27 |
| 4010 | LT | ET v | 0.08 | 0.33 | 3.91 | 4.29 | 1.09 | 1002 |
| 4923 | ET | LT v | 1.00 | 0.08 | 0.41 | 1.12 | 1.04 | 55 |
| 10207 | ET | LT v | 1.00 | 0.12 | 1.62 | 2.31 | 1.99 | 21 |
Notes. Column 1: galaxy identifier in the OTELO catalog. Column 2: OTELO classification. Column 3: DNN classification and a letter code to indicate reject (r) or validate (v); this classification after visual inspection by three of the authors. Column 4: DNN classification likelihood, closer to zero for ET instances and closer to one for LT. Columns 5–7: the photometric redshift, the Sérsic index, and the concentration value, respectively. Column 8: shows the elongation, that is, the ratio between the major and minor axes of the galaxy image as calculated by SExtractor (Bertin & Arnouts 1996). Column 9: shows the area in pixels of the HST Advanced Camera for surveys (scale 0.03 arcsec px−1).
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