Euclid on Sky
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Table 2

Similar to Table 1 but for the 30 dwarf galaxies overlapped with the Euclid ERO data of the Fornax cluster.

Galaxy FCC name (1) Alternative name(s) (2) Mr (mag) (3) Re (kpc) (4) log10(M*/M) (5)
FCC188 FDSll_DWARFl55, NGFS J033705−353525 −16.25 1.22 8.34
FCC195 FDSIO_DWARFOI4, NGFS J033723−345401, −15.43 1.28 8.04
FCC181 FDSIO_DWARFOO3, NGFS J033653−345619 −14.95 0.97 7.78
FCC160 FDSll_DWARF289, NGFS J033604−352320 −14.81 1.36 7.72
FCC133 FDSI6_DWARF253, NGFS J033420−352145 −14.61 1.13 7.70
FCC156 FDSI6_DWARF257, NGFS J033543−352018 −14.98 1.54 7.67
FCC171 FDSll_DWARF294, NGFS J033637−352309 −14.25 2.05 7.46
FCC157 FDSl6_DWARFl85a, NGFS J033543−353051 −13.75 1.19 7.33
FCC175 FDSll_DWARF246, NGFS J033643−352609 −13.80 1.61 7.19
FCC140 FDSI6_DWARF346, NGFS J033456−351127 −13.39 0.95 7.16
FCC142 FDS16 DWARF441, NGFSJ033458−350235 −13.38 0.85 7.09
FCC145 FDSI6_DWARF330, NGFS J033505−351307 −12.88 0.54 7.07
FCC168 FDSll_DWARF365, NGFS J033628−351239 −13.43 0.86 7.02
FDSll_DWARF306, NGFS J033700−352035 −13.48 1.45 7.01
FCC197 FDSll_DWARF330, NGFS J033741−351746 −12.92 0.62 6.89
FCC185 FDSI0_DWARF034, NGFS J033703−345233 −12.54 0.53 6.82
FCC144 FDSI6_DWARF280, NGFS J033500−351920 −12.68 0.57 6.77
FDSll_DWARF299, NGFS J033738−352308 −11.62 0.60 6.69
FDSLSB56 −12.70 0.93 6.68
FDSI6_DWARFI72, NGFS J033453−353411 −12.16 0.42 6.67
FCC146 FDSI6_DWARF28I, NGFS J033512−351923 −12.41 0.54 6.59
FDS16 DWARF272, NGFS J033558−352053 −12.05 0.40 6.49
FDS16_DWARF329, NGFS J033458−351324 −11.76 0.43 6.32
FDSLSB220 −11.80 1.06 6.30
FDS16_DWARF141 −11.29 0.29 6.03
FDSLSB45 −10.60 0.30 5.89
FDSLSB43 −10.60 0.39 5.83
FDS16_DWARF230b, NGFS J033512−352603 −10.67 0.59 5.78
FDS16_DWARF227, NGFS J033505−352703 −11.50 0.85 5.77
FDSLSB36 −10.60 0.39 5.76

Notes. Columns 1 and 2 present the FCC and other names of the galaxies (FDS names from Venhola et al. 2018 and/or NGFS names from Eigenthaler et al. 2018). Columns 3, 4, and 5 present the total absolute magnitude in the r−band, effective radius, and stellar mass of galaxies (Venhola et al. 2018, 2022). Throughout this paper, we use the FDS names of dwarf galaxies.

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