Table 3.
New candidate ultracool dwarfs.
| α | δ | Teff | G | ϖ | μαcosδ | μδ | Search | i | z |
|---|---|---|---|---|---|---|---|---|---|
| (ICRS, deg) | (ICRS, deg) | (K) | (mag) | (mas) | (mas yr−1) | (mas yr−1) | (mag) | (mag) | |
| 21.70712 | 33.44938 | 2600 | 20.94 | 11.18 | 7.36 | −51.33 | P | 20.19 | 18.69 |
| 22.16372 | 33.30222 | 2600 | 18.44 | 18.93 | 77.34 | −99.44 | P | 17.81 | 16.33 |
| 23.15882 | 39.59608 | 2800 | 20.58 | 3.41 | −54.42 | −21.40 | K | ||
| 27.63937 | 33.73132 | 2900 | 19.84 | 3.79 | 2.44 | −39.94 | P | 19.34 | 18.11 |
| 28.13097 | 33.83401 | 2600 | 19.69 | 11.93 | 58.33 | −46.75 | P | 19.11 | 17.67 |
| … |
Notes. Equatorial coordinates, G magnitudes, parallaxes, and proper motions are from Gaia DR2, effective temperatures are estimated with VOSA and i,z magnitudes are from J-PLUS. The column “Search” indicates whether the source was discovered in the photometric (P) or in the kinematic (K) search. The full table is available at the SVO-JPLUS archive of ultracool dwarfs (see Appendix A).
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