Open Access
Table 1.
Observed dwarf galaxies and globular cluster with MUSE.
| Name | RA | Dec | vel | [M/H] | age | M/L | S/N | MV |
|---|---|---|---|---|---|---|---|---|
| deg | deg | km/s | dex | Gyr | M⊙ /L⊙ | mag | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| dw1335-29 | 13:35:46.7 | −29:42:28 | 706.0±17.8 | −1.49±0.13 | – | 1.91±0.11 | 6.7 | −10.3 |
| KK208 | 13:36:35.5 | −29:34:15 | 439.9±15.6 | −1.53±0.23 | – | 1.36±0.33 | 7.0 | −15.9 |
| dw1340-30 | 13:40:19.2 | −30:21:31 | 429.3±21.6 | −1.71±0.19 | – | 1.23±0.27 | 9.4 | −10.8 |
| dw1341-29 | 13:41:20.2 | −29:34:03 | 483.4±20.6 | −2.21±0.13 | – | 1.16±0.36 | 8.5 | −8.8 |
| KK218 | 13:46:39.5 | –29:58:45 | 594.9±9.0 | −1.68±0.08 | 8.3±1.4 | 1.68±0.18 | 22.3 | −12.1 |
| KK208 GC1 | 13:36:25.90 | −29:35:29.2 | 432.1±3.3 | −1.48±0.04 | 13.7±1.6 | 2.19±0.20 | 33.3 | −5.5 |
Notes. (7) the M/L ratio is the stellar mass-to-light ratio estimated by pPXF fitting of the spectrum. (8) the S/N is measured on the spectrum in a region between 660 and 680 nm.
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