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Table 2.
Rejected NGC 474 dwarf satellite candidates.
| Name | RA | Dec | Exp. time | Vel. | [M/H] | Age | M/L | S/N | MV |
|---|---|---|---|---|---|---|---|---|---|
| deg | deg | s | km/s | dex | Myr | M⊙ /L⊙ | mag | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| MATLAS-19 | 19.558893 | 2.903885 | 5256 | 5576.0 ± 39.2 | −2.25 ± 0.26 | 5.8 ± 2.0 | 1.12 ± 0.25 | 5.3 | −13.0 |
| MATLAS-23 (c) | 19.711599 | 3.561740 | – | 4934 ± 8 | – | – | – | – | −15.4 |
| MATLAS-33 | 20.384933 | 3.671406 | 2628 | 6844.8 ± 19.6 | −1.60 ± 0.24 | 9.7 ± 2.6 | 1.72 ± 0.36 | 6.1 | −14.5 |
| MATLAS-34 (d) | 20.396175 | 3.563550 | 2628 | 9053.4 ± 36.1 | – | – | – | 10.3 | −15.8 |
Notes. Same as Table 1.
(c)
MATLAS-23 was not observed with MUSE. Its velocity comes from ALFALFA HI observations (Yu et al. 2022).
(10) The distances are estimated from the Hubble flow using a Hubble constant of 70 km/s/Mpc.
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