Table 1.
Properties of the LEWIS sample galaxies.
| Galaxies | RA [J2000] | Dec [J2000] | Mr [mag] | μe [mag arcsec−2] | μ0 [mag arcsec−2] | Re [kpc] | NGC | |
|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
| UDG 3 | 10:36:58.63 | −27:08:10.21 | −14.70 | 26.1 ± 0.2 | 25.2 ± 0.2 | 1.88 ± 0.12 | 15 ± 6 | |
| UDG 7 | 10:36:37.16 | −27:22:54.93 | −13.72 | 26.9 ± 0.4 | 24.4 ± 0.4 | 1.66 ± 0.12 | 3 ± 1 | |
| UDG 9 | 10:37:22.85 | −27:36:02.80 | −15.16 | 26.8 ± 0.2 | 24.2 ± 0.2 | 3.46 ± 0.12 | 7 ± 1 | |
| UDG 11 | 10:34:59.55 | −27:25:37.95 | −14.75 | 25.7 ± 0.1 | 24.4 ± 0.1 | 1.66 ± 0.12 | 7 ± 3 |
Notes. Col. (1): the target name in the LEWIS sample. Col. (2–3): the right ascension and declination of the galaxies. Col. (4–7): the absolute magnitude at the distance of the Hydra I Cluster in the r−band, the effective and central surface brightness, and the effective radius, in the g−band from Iodice et al. (2020), La Marca et al. (2022b), respectively. Col. (8): total number of GCs candidates hosted by the galaxies estimated in VEGAS imaging data Iodice et al. (2020), La Marca et al. (2022b).
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