Table 3.
Percentages of different BGGs in group classes.
| ID | FQ | FRSF | FBSF |
|---|---|---|---|
| (1) | (2) | (3) | (4) |
| HL43 | 0.91 |
0.08 |
0.01 |
| HL1543 | 0.87 |
0.08 |
0.05 |
| LL2.515 | 0.62 |
0.17 |
0.21 |
| LL2.5 | 0.45 |
0.16 |
0.39 |
| LL2.5* | 0.42 |
0.17 |
0.41 |
| Single | 0.37 |
0.18 |
0.44 |
Notes. Columns are as follows: (1) Notation (ID, see text) LL2.5* denotes the average of the sample to which we added 10% of randomly selected single galaxies to the LL2.5 sample; (2) Percentage of groups with a quenched BGG having logSFR ≤ −0.5 (Q); (3) Percentage of groups with a red star-forming BGG (RSF); (4) Percentage of groups with a blue star-forming BGG (BSF). In Cols. 2–4 we show the changes in percentages if we had used SFR limits logSFR = −0.6 and logSFR = −0.4.
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