| 3*Morpho3 | Radio-excess galaxies | FIRST revised2 | ||||||
| Factor 5 | Factor 3 | Factor 5 | Factor 3 | |||||
| N | % | N | % | N | % | N | % | |
| All T (n=397) | 6 | 1.5 | 16 | 4.0 | 3 | 0.8 | 12 | 3.0 |
| E-S0a (n=21) | 1 | 4.8 | 4 | 19.1 | 1 | 4.8 | 4 | 19.1 |
| Sa-Irr (n=376) | 5 | 1.3 | 12 | 3.2 | 2 | 0.5 | 8 | 2.1 |
All percentages for the fraction of radio-excess galaxies are upper limits as explained in Sect. 4.1.3.
In Sect. 4.1.3 we explain how we revise these numbers using the FIRST survey. 
Morphological subsamples. The percentages are computed over the number of galaxies for each subsample.
|