Table A.2.
Proper motions of candidates estimated in our cross-match (Cols. 2 and 3) and from Gaia DR2 (Cols. 4 and 5).
| Object | μ α (mas yr−1) | μ δ (mas yr−1) |
 (mas yr−1) |
 (mas yr−1) |
d Phot. (pc) | d Gaia (pc) | d others (pc) | SpType (Estimated) | SpType (Reported) |
|---|---|---|---|---|---|---|---|---|---|
| 2M0353+1030 | 133 | −18 | 127 | −22 | 52 ± 1.3 |
|
. . . | L0.7 | L0.9V a |
| 2M0355+1439 | 148 | −16 | 154 | −20 | 29 ± 0.4 |
|
… | M9.8 | M8.8V a |
| 2M0408+0742 | 145 | 84 | 142 | 73 | 28 ± 0.2 |
|
… | M9.2 | M8.1V a |
| 2M0409+1247 | 106 | −10 | … | … | 39 ± 2.1 | … | … | L4.5 | … |
| 2M0410+1459 | 107 | −22 | 108 | −11 | 64 ± 3.8 |
|
b
|
M9.6 | L0.5 b |
| 2M0416+2052 | 112 | −31 | 119 | −39 | 40 ± 0.5 |
|
… | M7.1 | … |
| 2M0418+2131 | 120 | −55 | … | … | 37 ± 2.9 | … | 48.8 ± 4.0 a | L7.1 | L5 c |
| 2M0420+2356 | 126 | −36 | 130 | −29 | 39 ± 0.3 |
|
b
|
L0.1 | M8.5 b |
| 2M0420+1345 | 109 | −9 | 116 | −21 | 40 ± 0.5 |
|
… | M8.9 | M8.5 |
| 2M0421+2023 | 96 | −36 | 104 | −33 | 47 ± 0.1 |
|
… | M6.9 | … |
| 2M0422+1358 | 84 | −10 | 89 | −18 | 66 ± 1.9 |
|
c
|
M9.1 | M9.5 b |
| 2M0424+0637 | 159 | 65 | … | … | 31 ± 2.0 | … | … | L9.1 | L4.0 ± 0.5 d |
| 2M0429+2437 | 45 | −71 | … | … | 42 ± 1.9 | … | … | L7.2 | L6.0−L8.0 d |
| 2M0429+2529 | 93 | −53 | 98 | −52 | 49 ± 0.7 |
|
… | M7.1 | M8V |
| 2M0433+1611 | 73 | −24 | … | … | 38 ± 1.4 | … | … | L8.0 | … |
| 2M0435+2008 | 91 | −43 | 101 | −43 | 27 ± 0.8 |
|
… | L0 | … |
| 2M0435+1927 | 174 | −46 | 179 | −39 | 58 ± 0.5 |
|
… | M9.9 | … |
| 2M0435+1215 | 75 | 1 | 92 | −13 | 42 ± 0.3 |
|
… | M7.0 | … |
| 2M0436+1151 | 94 | −11 | 100 | −8 | 28 ± 0.3 |
|
… | L0.2 | M9 e |
| 2M0436+1901 | 93 | −30 | … | … | 33 ± 2.1 | … | 35 ± 4 b | L7.0 | L5 f |
| 2M0438+0700 | 82 | 23 | … | … | 44 ± 1.0 | … | … | L5.1 | L1 ± 1 d |
| 2M0440+2325 | 85 | −29 | 90 | −46 | 38 ± 0.6 |
|
… | M6.8 | … |
| 2M0441+2130 | 96 | −31 | … | … | 38 ± 1.4 | … | 45 ± 9 b | L7.4 | L6 f |
| 2M0441+1453 | 87 | −15 | 98 | −23 | 37 ± 1.6 |
|
… | L0.4 | … |
| 2M0444+1901 | 79 | −30 | 74 | −32 | 61 ± 0.9 |
|
… | M9.9 | … |
| 2M0445+1443 | 80 | −15 | 82 | −22 | 49 ± 0.8 |
|
… | M7.6 | … |
| 2M0445+1503 | 84 | −8 | 84 | −23 | 49 ± 0.6 |
|
… | M6.9 | … |
| 2M0445+1246 | 88 | −12 | 100 | −16 | 40 ± 0.5 |
|
… | L1.5 | … |
| 2M0446+1857 | 82 | −36 | 86 | −38 | 44 ± 0.9 |
|
… | M7.0 | … |
| 2M0447+1719 | 85 | −21 | 95 | −31 | 38 ± 0.4 |
|
… | M6.8 | … |
| 2M0448+2051 | 67 | −27 | 76 | −37 | 35 ± 0.3 |
|
… | M6.9 | M6V g |
| 2M0453+2033 | 58 | −90 | 68 | −89 | 31 ± 0.4 |
|
… | L3.5 | … |
| 2M0455+2140 | 71 | −39 | 77 | −45 | 37 ± 0.4 |
|
… | M8.9 | M8.5V g |
| 2M0458+1212 | 82 | −12 | 86 | −16 | 50 ± 2.8 |
|
f
|
L0.8 | L0.5 b |
| 2M0459+1304 | 71 | −22 | 80 | −21 | 42 ± 0.3 |
|
… | M9.7 | … |
| 2M0500+1207 | 104 | −7 | 98 | −17 | 46 ± 0.6 |
|
… | M7.2 | … |
Notes. Column 6 show the estimated distance using the maximum likelihood method developed for this work. Errors in Col. 6 are the dispersion of distance estimates carried out in the five bands considered in the maximum likelihood method, see text. Columns 7 and 8 shows distances measured by the Gaia mission and by other authors, respectively. Estimated spectral types with our method are listed in Col. 9, while types reported by other authors are listed in the last column.
References.
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