Table 3.
ULX abundances and frequencies across host galaxy morphological types.
| Sample | cULXss |
|||||
|---|---|---|---|---|---|---|
| Sub-sample | All | El. | Le. | ESp. | LSp. | Ir. |
| ULXs | 292 | 49 | 26 | 107 | 92 | 17 |
| Galaxies | 149 | 18 | 16 | 53 | 45 | 13 |
| Pot. gals. | 722 | 151 | 75 | 109 | 114 | 147 |
| ULX/gal. | 0.40 | 0.32 | 0.35 | 0.98 | 0.81 | 0.12 |
| Gal. frac. | 0.21 | 0.12 | 0.21 | 0.49 | 0.37 | 0.09 |
| Sample | cbULXss |
|||||
| Sub-sample | All | El. | Le. | ESp. | LSp. | Ir. |
| ULXs | 69 | 10 | 16 | 25 | 10 | 1 |
| Pot. gals. | 12 166 | 2174 | 1787 | 2052 | 1416 | 850 |
| ULX/gal.(%) | 0.57 | 0.46 | 0.90 | 1.22 | 0.71 | 0.12 |
Notes. Number of ULX candidates in cULXss and cbULXss, number of galaxies that host them, number of galaxies that could potentially host them, ULX frequencies, and fraction of galaxies with candidates, divided according to morphological groups of their host galaxies. No distinction is made between bright ULXs and their host galaxies as no more than one candidate has been found in each. For the cbULXss, the ULX frequencies/fraction of galaxies are presented in %.
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