Table 3.
Globular cluster candidate numbers and their specific frequencies associated with the new UDGs and LSB galaxies in the Hydra I cluster.
| Object | Raw GCs | Back. sub. GCs | NGC | SN |
|---|---|---|---|---|
| UDG 13 | 0 | −1.4 | – | – |
| UDG 14 | 1 | 0.04 | 0 ± 1 | 0 ± 23 |
| UDG 15 | 1 | 0.46 | 2 ± 3 | 41 ± 75 |
| UDG 16 | 0 | −0.33 | – | – |
| UDG 17 | 1 | 0.73 | 3 ± 3 | 11 ± 14 |
| UDG 18 | 3 | 2.8 | 11 ± 7 | 168 ± 153 |
| UDG 19 | 0 | −0.24 | – | – |
| UDG 20 | 0 | −0.69 | – | – |
| UDG 21 | 0 | −0.6 | – | – |
| UDG 22 | 0 | −0.24 | – | – |
| UDG 23 | 0 | −0.45 | – | – |
| UDG 32 | 3 | 1.8 | 7 ± 4 | 12 ± 10 |
| LSB 1 | 0 | −0.42 | – | – |
| LSB 2 | 0 | −0.36 | – | – |
| LSB 3 | 1 | −0.44 | – | – |
| LSB 4 | 2 | 1.9 | 8 ± 3 | 28 ± 16 |
| LSB 5 | 0 | −0.09 | – | – |
| LSB 6 | 1 | 0.46 | 2 ± 1 | 2 ± 1 |
| LSB 7 | 0 | −0.63 | – | – |
| LSB 8 | 0 | −0.36 | – | – |
Notes. For each galaxy in our sample, we show the raw GC candidate counts within a 1.5Re aperture (second column), the local background-subtracted counts (third column), the completeness-corrected total GC counts (NGC, fourth column), and the respective specific frequency (last column).
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