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Table 1.

Parameters of the new UDG candidates in the Hydra I cluster.

Object RA Dec Detection Mr, 0 (g − r)0 M/Lr M* μe μ0 Re n χ2
[deg] [deg] [mag] [mag] [107M] [mag arcsec−2] [mag arcsec−2] [kpc]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
UDG 13 159.060384 −27.507390 V −12.73 0.64 ± 0.30 2.00 ± 1.00 2.0 ± 1.0 27.35 ± 0.11 24.23 ± 0.20 1.60 ± 0.20 1.70 ± 0.06 6.3
UDG 14 159.000949 −27.544729 A −11.91 0.70 ± 0.30 2.00 ± 2.00 1.1 ± 0.8 28.50 ± 0.04 24.50 ± 0.50 1.83 ± 0.12 2.0 ± 0.2 1.1
UDG 15 159.010624 −27.605435 V −11.95 0.50 ± 0.30 1.20 ± 0.80 0.6 ± 0.4 27.70 ± 0.20 25.01 ± 0.30 1.51 ± 0.15 1.40 ± 0.10 11.0
UDG 16 159.10242 −27.235641 V −12.84 0.43 ± 0.20 1.00 ± 0.50 1.1 ± 0.5 27.63 ± 0.11 25.90 ± 0.20 1.75 ± 0.12 0.97 ± 0.09 1.0
UDG 17 159.173845 −27.277078 V −13.99 0.86 ± 0.11 4.00 ± 1.00 12 ± 3.0 26.70 ± 0.08 24.90 ± 0.10 1.50 ± 0.20 1.00 ± 0.10 1.6
UDG 18 159.070065 −27.338011 V −12.28 0.52 ± 0.20 1.30 ± 0.60 0.9 ± 0.4 27.60 ± 0.20 25.56 ± 0.19 1.64 ± 0.12 1.08 ± 0.03 1.7
UDG 19 159.010682 −27.290000 V −11.49 0.80 ± 0.20 3.00 ± 1.00 1.0 ± 0.5 28.50 ± 0.20 26.50 ± 0.30 1.98 ± 0.12 1.10 ± 0.13 1.1
UDG 20 159.518455 −27.497272 A −12.95 0.49 ± 0.05 1.20 ± 0.14 1.4 ± 0.2 27.33 ± 0.15 26.03 ± 0.33 1.97 ± 0.12 0.79 ± 0.12 1.4
UDG 21 159.225691 −27.615297 A −12.78 0.45 ± 0.10 1.00 ± 0.20 1.1 ± 0.3 27.30 ± 0.50 24.00 ± 0.40 1.50 ± 0.12 1.70 ± 0.15 1.5
UDG 22 158.670717 −27.700909 A −13.92 0.50 ± 0.05 1.23 ± 0.14 3.6 ± 0.4 26.50 ± 0.14 25.26 ± 0.18 3.60 ± 0.12 0.72 ± 0.08 1.0
UDG 23 158.865410 −27.771273 A −14.11 0.42 ± 0.02 0.96 ± 0.04 3.4 ± 0.2 27.20 ± 0.20 24.29 ± 0.30 2.47 ± 0.20 1.5 ± 0.14 6.0

Notes. Column 1 reports the name of the UDG candidate. In Cols. 2 and 3 we list the coordinates of the UDGs in J2000. In Col. 4 we report the kind of detection, i.e. visual inspection (flag “V”) or by the automatic tool (flag “A”). In Cols. 5 and 6 we report the total r-band magnitude and the average g − r color. Columns 7 and 8 give the stellar mass-to-light ratio derived in the r band and stellar mass, respectively. Columns 9–12 list the structural parameters derived from the 2D fit in the g band: the effective and central surface brightness, the effective radius in kpc and the n exponent of the Sérsic law, respectively. In Col. 13 we report the value of , which indicates the goodness of the fit of the surface brightness profiles. Magnitudes and colors are corrected for Galactic extinction using values from Schlafly & Finkbeiner (2011).

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