Table 1.
Hyades late-M and early-L confirmed spectroscopically with Gaia proper motions and distances.
| Name | RA | Dec | SpT | SourceID | Plx | pmRA | pmDEC | H |
|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss.ss) | (dd:”:".") | (mas) | (mas yr−1) | (mas yr−1) | (mag) | |||
| Hya01 | 04:20:24.50 | +23:56:13.0 | M8.5 | 149089760932648448 | 22.6480 ± 0.4575 | 130.178 ± 0.876 | −28.598 ± 0.660 | 13.85 |
| Hya03 | 04:10:24.01 | +14:59:10.3 | L0.5 | 3311691879984803072 | 17.3183 ± 1.5853 | 107.981 ± 2.747 | −11.185 ± 2.612 | 14.78 |
| Hya04 | 04:42:18.59 | +17:54:37.3 | M9.5 | 3409343115420601728 | – | – | – | 14.97 |
| Hya06 | 04:22:05.22 | +13:58:47.3 | M9.5 | 3310992904122021120 | 18.2032 ± 0.9181 | 89.391 ± 1.612 | −17.657 ± 1.307 | 14.81 |
| Hya08 | 04:58:45.75 | +12:12:34.1 | L0.5 | 3295377360811741184 | 24.2448 ± 0.9774 | 85.748 ± 2.536 | −16.008 ± 1.265 | 14.55 |
Notes. Hya05 (M3) and Hya07 (M5) are not listed below because they were rejected as spectroscopic members of the Hyades based on their optical spectra (Lodieu et al. 2014b). The other L dwarfs are not in Gaia but listed in Table 2 with ground-based parallaxes.
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