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Table 1.

Parameters of the UDG candidates in the Hydra I cluster.

Object RA Dec Mr g − r M/L M* μ0 Re n q
J2000 J2000 [mag] [mag] [108M] [mag arcsec−2] [kpc]
Hydra I-UDG 1 10:37:54.12 −27:09:37.50 −15.48 ± 0.07 0.40 ± 0.09 0.90 1.12 24.20 ± 0.10 1.75 ± 0.12 0.621 ± 0.005 0.766 ± 0.003
Hydra I-UDG 2 10:37:34.89 −27:10:29.94 −14.27 ± 0.05 0.53 ± 0.2 1.35 0.55 24.97 ± 0.08 1.55 ± 0.12 0.72 ± 0.01 0.877 ± 0.007
Hydra I-UDG 3 10:36:58.63 −27:08:10.21 −14.7 ± 0.2 0.75 ± 0.3 2.71 1.65 25.2 ± 0.2 1.88 ± 0.12 0.572 ± 0.013 0.79 ± 0.01
Hydra I-UDG 4 10:37:02.64 −27:12:15.01 −16.03 ± 0.04 0.95 ± 0.10 5.11 10.6 24.86 ± 0.05 2.64 ± 0.12 0.597 ± 0.006 0.748 ± 0.003
Hydra I-UDG 5 10:36:07.68 −27:19:03.26 −14.66 ± 0.09 0.65 ± 0.14 1.98 1.16 23.7 ± 0.3 1.42 ± 0.12 0.89 ± 0.01 0.582 ± 0.004
Hydra I-UDG 6 10:36:35.80 −27:19:36.12 −14.38 ± 0.08 0.32 ± 0.2 0.70 0.32 24.08 ± 0.13 1.37 ± 0.12 0.706 ± 0.006 0.629 ± 0.002
Hydra I-UDG 7 10:36:37.16 −27:22:54.93 −13.72 ± 0.13 0.6 ± 0.3 1.98 0.49 24.37 ± 0.4 1.66 ± 0.12 1.32 ± 0.03 0.73 ± 0.01
Hydra I-UDG 8 10:38:14.59 −27:24:27.07 −14.87 ± 0.07 0.34 ± 0.13 0.74 0.53 23.22 ± 0.6 1.40 ± 0.12 0.98 ± 0.02 0.578 ± 0.005
Hydra I-UDG 9 10:37:22.85 −27:36:02.80 −15.16 ± 0.12 0.6 ± 0.2 1.92 1.78 24.2 ± 0.2 3.46 ± 0.12 1.38 ± 0.01 0.54 ± 0.01
Hydra I-UDG 10 10:35:27.32 −27:33:03.86 −13.89 ± 0.08 0.4 ± 0.2 0.90 0.26 24.33 ± 0.3 2.29 ± 0.10 1.53 ± 0.02 0.90 ± 0.01
Hydra I-UDG 11 10:35:04.16 −27:26:17.26 −14.75 ± 0.07 0.43 ± 0.11 0.99 0.63 24.36 ± 0.13 1.66 ± 0.12 0.80 ± 0.01 0.92 ± 0.01
Hydra I-UDG 12 10:34:59.55 −27:25:37.95 −14.3 ± 0.2 0.8 ± 0.4 2.8 1.19 25.1 ± 0.2 1.64 ± 0.12 0.67 ± 0.02 0.72 ± 0.01

Notes. Column 1 reports the name of the UDG candidate. In Cols. 2 and 3 we list the coordinates of the UDGs. In Cols. 4 and 5 are reported the total r-band magnitude and the average g − r colour. Columns 6 and 7 give the stellar mass-to-light ratio and stellar mass, respectively, derived in the r band. Columns 8–11 list the structural parameters derived from the 2D fit in the g band: the central surface brightness, the effective radius in kpc, the n exponent of the Sérsic law and the axial ratio, respectively. Magnitudes and colours are corrected for Galactic extinction using values from Schlegel et al. (1998).

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