Table 1.
Physical properties of the galaxy sample.
| Galaxy | D | Re |
 |
 |
Renc |
 |
 |
|---|---|---|---|---|---|---|---|
| [Mpc] | [log10 M⊙] | [log10 M⊙] | [log10 M⊙] | [log10 M⊙] | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| FCC 153 | 20.8 | 19.80″ | 9.55 | 9.63 | 165.78″ | 10.06 | 11.43 |
| 2.00 kpc | 16.72 kpc | ||||||
| FCC 170 | 21.9 | 15.90″ | 10.33 | 8.83 | 148.39″ | 10.67 | 10.74 |
| 1.69 kpc | 15.76 kpc | ||||||
| FCC 177 | 20.0 | 35.90″ | 9.43 | 9.71 | 133.347″ | 9.73 | 10.84 |
| 3.48 kpc | 12.93 kpc | ||||||
Notes. (1) galaxy name; (2) distance to the galaxy measured by Blakeslee et al. (2009) using surface-brightness fluctuations; (3) r-band effective radius taken from Iodice et al. (2019b) and converted into physical units at our adopted distances; (4) and (5) stellar and DM masses enclosed within Re, respectively; (6) radius which encloses 98% of the stellar mass; (7) and (8) stellar and DM masses enclosed within Renc, respectively.
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