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Table 3.

Derived parameters of LTGs in the Fornax A subgroup.

Object mg g − r g − i Rer Dcore Mi M* M/L
mag mag mag arcsec deg mag 1010 M
(1) (2) (3) (4) (5) (6) (7) (8) (9)
FCC013 (NGC 1310) 12.48 ± 0.04 0.57 ± 0.1 0.77 ± 0.02 27.6 ± 0.2 0.25 −19.74 0.47 0.76
FCC022 (NGC 1317) 11.15 ± 0.01 0.77 ± 0.02 0.99 ± 0.02 35.36 ± 0.03 0.02 −20.98 1.71 0.88
FCC028 13.33 ± 0.02 0.57 ± 0.04 0.98 ± 0.05 22.1 ± 0.5 0.28 −19.07 0.29 0.87
FCC029 (NGC 1326) 10.62 ± 0.02 0.62 ± 0.04 1.01 ± 0.04 48.2 ± 1 0.68 −21.53 2.94 0.91
FCC033 (NGC 1316C) 13.81 ± 0.03 0.69 ± 0.1 0.97 ± 0.04 22.6 ± 0.5 0.37 −18.30 0.14 0.85
FCC035 14.79 ± 0.03 0.17 ± 0.1 0.18 ± 0.1 17.1 ± 0.4 0.44 −17.39 0.017 0.24
FCC037 (NGC 1326A) 13.55 ± 0.03 0.51 ± 0.1 0.95 ± 0.1 41.0 ± 0.8 0.87 −18.54 0.17 0.83
FCC039 (NGC 1326B) 12.87 ± 0.1 0.32 ± 0.1 0.73 ± 0.1 53.03 ± 2 0.86 −19.00 0.18 0.58
FCC062 (NGC 1341) 12.37 ± 0.02 0.54 ± 0.04 1.01 ± 0.04 20.6 ± 0.4 0.92 −19.72 0.55 0.91

Notes. Column 1 – Fornax A subgroup members from Ferguson (1989); Col. 2 – Total magnitude in g-band derived from the isophote fit. Values were corrected for the Galactic extinction, using the absorption coefficient by Schlegel et al. (1998); Cols. 3 and 4 – Average g − r and g − i colours; Col. 5 – Effective radius in r-band, in arcsec; Col. 6 – Projected distance from the galaxy centre in degree, that is, from NGC 1316 (FCC021); Col. 7 – Absolute magnitude in i-band, derived using the distance modulus from NED and Tully et al. (2009); Cols. 8 and 9 – Stellar mass and mass-to-light (M/L) in i-band.

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