Table 2
The number of galaxies for each Hubble bin for the remaining three quadrants of the top right and left panels of Fig. 1.
| Morphology | Total | (u − r) > 2.3 | (u − r) > 2.3 | (u − r) < 2.3 | (u − r) < 2.3 | (u − r) < 2.3 | (u − r) < 2.3 |
| and nr< 2.5 | and  > 1.2 |
and nr< 2.5 | and > 1.2 |
and nr> 2.5 | and < 1.2 |
||
|
|
|||||||
| E | 19 | 3 | 1 | 0 | 0 | 0 | 0 |
| S0 | 13 | 2 | 7 | 0 | 0 | 1 | 1 |
| Sa | 2 | 0 | 1 | 0 | 0 | 0 | 0 |
| Sab-Sb | 27 | 5 | 11 | 8 | 10 | 5 | 3 |
| Sbc-Sc | 49 | 3 | 4 | 41 | 36 | 4 | 9 |
| Scd-Sd | 21 | 0 | 0 | 21 | 19 | 0 | 2 |
| Sm-Irr | 11 | 0 | 0 | 11 | 7 | 0 | 4 |
Notes. Column 1: Hubble type, Col. 2: total number of galaxies in each Hubble type after applying the following cuts: Mr< −18.7 and z< 0.01, Cols. 3−8: number of galaxies selected in each cut for the original sample.
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