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Table 2.

LSB candidates in the Hydra I cluster.

Object RA Dec Mr g − r μ0 Re n q
J2000 J2000 [mag] [mag] [mag arcsec−2] [kpc]
Hydra I-LSB 1 10:35:17.540 −27:10:51.96 −13.31 ± 0.14 1.1 ± 0.4 24.2 ± 0.3 0.86 ± 0.12 1.05 ± 0.02 0.713 ± 0.009
Hydra I-LSB 2 10:34:53.099 −27:12:00.06 −15.12 ± 0.04 0.69 ± 0.09 23.57 ± 0.13 1.08 ± 0.12 0.69 ± 0.004 0.903 ± 0.003
Hydra I-LSB 3 10:34:37.181 −27:12:41.14 −14.55 ± 0.09 0.34 ± 0.15 23.73 ± 0.14 0.997 ± 0.12 0.660 ± 0.004 0.979 ± 0.003
Hydra I-LSB 4 10:35:37.232 −27:14:50.14 −14.25 ± 0.05 0.58 ± 0.12 23.5 ± 0.2 0.62 ± 0.12 0.580 ± 0.005 0.925 ± 0.003
Hydra I-LSB 5 10:37:54.147 −27:16:15.31 −13.64 ± 0.11 0.4 ± 0.2 25.65 ± 0.14 1.29 ± 0.12 0.58 ± 0.02 0.858 ± 0.013
Hydra I-LSB 6 10:38:05.430 −27:15:46.89 −14.08 ± 0.06 0.60 ± 0.11 24.0 ± 0.2 1.02 ± 0.12 0.882 ± 0.012 0.763 ± 0.006
Hydra I-LSB 7 10:37:43.555 −27:20:44.73 −13.19 ± 0.05 0.55 ± 0.11 25.00 ± 0.15 1.21 ± 0.12 0.63 ± 0.02 0.55 ± 0.01
Hydra I-LSB 8 10:35:42.806 −27:20:09.61 −12.35 ± 0.13 0.4 ± 0.2 25.60 ± 0.13 0.92 ± 0.13 0.78 ± 0.03 0.94 ± 0.02
Hydra I-LSB 9 10:36:16.856 −27:36:50.83 −13.01 ± 0.09 0.7 ± 0.2 25.12 ± 0.12 1.00 ± 0.12 0.73 ± 0.02 0.63 ± 0.01
Hydra I-LSB 10 10:35:03.551 −27:25:50.07 −14.46 ± 0.10 0.9 ± 0.3 23.6 ± 0.2 0.98 ± 0.12 0.609 ± 0.006 0.675 ± 0.003
Hydra I-LSB 11 10:34:56.212 −27:32:57.79 −15.32 ± 0.07 0.29 ± 0.09 22.86 ± 0.15 1.14 ± 0.12 0.765 ± 0.003 0.834 ± 0.001
Hydra I-LSB 12 10:38:03.959 −27:45:28.18 −14.40 ± 0.05 0.9 ± 0.2 24.3 ± 0.2 1.28 ± 0.12 0.627 ± 0.011 0.484 ± 0.004
Hydra I-LSB 13 10:37:19.034 −27:42:29.29 −13.95 ± 0.07 0.62 ± 0.14 24.53 ± 0.14 1.08 ± 0.12 0.56 ± 0.01 0.653 ± 0.006
Hydra I-LSB 14 10:36:41.231 −27:48:20.04 −13.85 ± 0.08 1.0 ± 0.4 24.0 ± 0.3 1.03 ± 0.12 0.81 ± 0.01 0.546 ± 0.005
Hydra I-LSB 15 10:34:42.961 −27:40:14.42 −14.96 ± 0.10 0.6 ± 0.2 23.1 ± 0.2 0.89 ± 0.12 0.795 ± 0.004 0.920 ± 0.003

Notes. Column 1 reports the name of the LSB candidate, and in Cols. 2 and 3 we list the coordinates. In Cols. 4 and 5, the total r-band magnitude and the average g − r colour are reported. Columns 6 and 9 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 Sersic 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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