Table 1.
Fraction of star-forming galaxy sample selected with the column header that is present in the star-forming galaxy sample selected with the row header.
| sSFR | NUVrJ | NUVrK | u − r | UVJ | BPT | D4000 | |
|---|---|---|---|---|---|---|---|
| sSFR | – | 0.78 | 0.78 | 0.89 | 0.86 | 0.78 | 0.83 |
| NUVrJ | 0.99 | – | 0.99 | 0.99 | 0.98 | 0.94 | 0.98 |
| NUVrK | 0.99 | 0.99 | – | 0.99 | 0.98 | 0.94 | 0.98 |
| u − r | 0.91 | 0.80 | 0.80 | – | 0.88 | 0.82 | 0.88 |
| UVJ | 0.97 | 0.87 | 0.87 | 0.97 | – | 0.87 | 0.92 |
| BPT | 0.42 | 0.40 | 0.40 | 0.43 | 0.42 | – | 0.44 |
| D4000 | 0.89 | 0.83 | 0.83 | 0.92 | 0.87 | 0.87 | – |
Notes. If more than 90% of the column sample is present in the row sample, the cell is shaded dark blue, while if less than 50% of the column sample is present in the row sample, the cell is shaded light red.
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