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Table 6.
Distances used to derive absolute bolometric magnitudes.
| Galaxy | Distance [kpc] | Reference |
|---|---|---|
| Seg I | 23 ± 2 | Belokurov et al. (2007) |
| Sgr | 27 ± 1 | Hamanowicz et al. (2016) |
| Tri II | 30 ± 2 | Laevens et al. (2015b) |
| Ret II | 32 ± 2 | Mutlu-Pakdil et al. (2018) |
| UMa II | 35 ± 2 | Dall’Ora et al. (2012) |
| Boo I | 66 ± 2 | Dall’Ora et al. (2006) |
| UMi | 76 ± 4 | Bellazzini et al. (2002) |
| Dra | 79 ± 6 | Kinemuchi et al. (2008) |
| Scl | 86 ± 3 | Pietrzyński et al. (2008) |
| Sex | 86 ± 6 | Pietrzyński et al. (2008) |
| Car | 106 ± 6 | Karczmarek et al. (2015) |
| For | 146 ± 8 | Karczmarek et al. (2017) |
| Leo I | 269 ± 12 | Stetson et al. (2014) |
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