Table 1
Properties of the ten most massive galaxies located within the footprint of the Euclid ERO-F images.
| Galaxy (1) | Alternative name(s) (2) | Mr (mag) (3) | Re (kpc) (4) | log10(M*/M⊙) (5) | D (Mpc) (6) |
|---|---|---|---|---|---|
| FCC167 | NGC 1380 | −22.36 | 5.80 | 10.99 | 21.2 ± 0.7 |
| FCC184 | NGC 1387 | −21.43 | 3.22 | 10.67 | 19.9 ±0.8 |
| FCC161 | NGC 1379 | −21.02 | 2.76 | 10.42 | – |
| FCC147 | NGC 1374 | −20.96 | 2.36 | 10.38 | 19.6 ± 0.6 |
| FCC170 | NGC 1381 | −20.71 | 1.69 | 10.35 | 21.9 ±0.8 |
| FCC148 | NGC 1375 | −19.79 | 2.73 | 9.76 | 19.6 ± 0.7 |
| FCC190 | NGC 1380B | −19.28 | 2.36 | 9.73 | 20.3 ± 0.7 |
| FCC143 | NGC 1373, FDS16_DWARF002 | −18.77 | 1.03 | 9.45 | 19.3 ±0.8 |
| FCC182 | FDS11_DWARF279 | −17.88 | 0.97 | 9.10 | 19.6 ± 0.8 |
| FCC136 | FDS16_DWARF159 | −17.76 | 1.75 | 9.01 | 18.8 ±0.7 |
Notes. Columns 1 and 2 present the FCC and other names of the galaxies (NGC and/or FDS names from Venhola et al. 2018). Columns 3, 4, and 5 present the total absolute magnitude in the r-band, effective radius (half-light radius), and stellar mass of galaxies (Spavone et al. 2020; Venhola et al. 2018). When available, the distances derived from the surface−brightness fluctuations (SBF) studies of Blakeslee et al. (2009) are provided in Col. 6. Throughout this paper, we use the FCC names of massive galaxies.
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