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Table 6.

Ultra-diffuse galaxy parameters.

Galaxy mH g − r V − H (M*/L)H M* N GC raw $ N_{\mathrm{GC}}^{\mathrm{raw}} $ NGC SN Mh Mh Mh
(AB mag) (AB mag) (Vega mag) (107M) (1010M) (1010M) (1010M)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
UDG3 17.96 ± 0.04 0.75 ± 0.3 2.61 ± 0.39 0.81 ± 0.59 11 ± 8.0 3 ± 2 15 ± 9 27 ± 18 5.1 ± 3.3 2.97 ± 1.47 2.36 ± 1.10
UDG7 19.26 ± 0.03 0.6 ± 0.3 2.14 ± 0.35 0.56 ± 0.41 2.28 ± 1.67 2 ± 1 11 ± 6 46 ± 25 3.8 ± 1.9 1.42 ± 0.8 0.88 ± 0.41
UDG9 19.01 ± 0.08 0.6 ± 0.2 0.97 ± 0.27 0.56 ± 0.28 2.87 ± 1.42 0 ± 2 0 ± 11 0 ± 12 .... 1.58 ± 0.77 1.02 ± 0.32
UDG11 18.19 ± 0.03 0.43 ± 0.11 2.00 ± 0.18 0.37 ± 0.1 4.03 ± 1.09 7 ± 2 37 ± 11 56 ± 19 12.8 ± 4.1 1.86 ± 0.80 1.26 ± 0.22

Notes. Col. 1 galaxy ID; Col. 2 total H-band magnitude; Col. 3 (g − r) color from Iodice et al. (2020); Col. 4 derived (V − H) color used to validate our photometry (see Sect. 5.3); Col. 5 M*/L ratio derived from Into & Portinari (2013); Col. 6 stellar mass derived assuming the absolute solar magnitude MH from Into & Portinari (2013); Cols. 7–9 reports the raw number of GC ( N GC raw $ N_{\mathrm{GC}}^{\mathrm{raw}} $), the corrected for completeness number of GCs (NGC) and the specific frequency (SN); Cols 10–12 reports the dark halo mass estimated using Harris et al. (2017), Moster et al. (2013), Zaritsky & Behroozi (2023) relations, respectively.

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