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Table 1:

Parallaxes and proper motions for TOPP red dwarfs.
ID, LHS GJ RA     Dec     N*,Nf $\mu_{\alpha}$ $\mu_{\delta}$ $\Delta T$ COR $\pi$ Literature $\pi$
    (h:m:s   ) ($^\circ$:$^{\prime}$: $^{\prime\prime}$)      (mas/yr) (mas/yr) (yrs) (mas) (mas) (mas)
1, 1047 1005 0:15:28.2 -16: 7:43.5 7, 37 596.8 $\pm$ 4.7 -629.0 $\pm$ 5.1 3.29 2.05 179.8 $\pm$ 11.6 191.9 $\pm$ 17.21
2, 1050 12 0:15:52.3 +13:32:41.0 8, 83 606.7 $\pm$ 1.4 336.2 $\pm$ 1.5 5.20 1.86 87.4 $\pm$ 3.4 84 $\pm$ 112
3, 1104 ... 0:35:47.9 +52:41:41.7 33,136 775.9 $\pm$ 1.0 -174.3 $\pm$ 1.5 5.20 1.05 40.5 $\pm$ 2.2         ...          
4, 1475 119 A 2:56:29.6 +55:26: 1.2 33,108 723.9 $\pm$ 2.6 -444.3 $\pm$ 2.8 5.20 0.44 59.9 $\pm$ 5.0 30.94 $\pm$ 9.861
5, 228 ... 7:16:21.9 +23:42:32.4 24,171 936.1 $\pm$ 0.4 -571.1 $\pm$ 0.4 6.30 1.30 23.6 $\pm$ 1.1 17.8 $\pm$ 3.03
6, 1923 3444 7:32:10.7 +57:55:33.7 16,145 2.7 $\pm$ 0.6 -914.2 $\pm$ 0.7 6.02 2.27 44.0 $\pm$ 1.7         ...          
7, 243 ... 8: 3: 7.1 +34:55:59.6 11,113 -512.7 $\pm$ 0.7 -1494.0 $\pm$ 0.8 3.29 1.61 41.0 $\pm$ 1.2         ...          
8, 1976 ... 8: 3: 7.1 +52:50:38.0 12, 33 362.3 $\pm$ 2.3 -668.2 $\pm$ 2.1 4.11 1.11 40.3 $\pm$ 5.1 32.07 $\pm$ 4.261
9, 2065 3517 8:53:46.0 - 3:29:36.0 11, 23 -507.1 $\pm$ 1.5 -189.9 $\pm$ 2.8 4.93 1.66 109.9 $\pm$ 4.6 113.3 $\pm$ 2.04
10, 306 3668 11:31:26.7 -14:58:17.0 8, 14 401.3 $\pm$ 5.6 -1378.2 $\pm$ 5.2 6.02 1.78 85.0 $\pm$ 19.2 89.24 $\pm$ 1.697
11, 2472 452.1 11:54: 8.1 + 9:48:11.9 7, 36 90.0 $\pm$ 1.5 -791.0 $\pm$ 1.5 6.02 1.91 88.3 $\pm$ 3.7 92 $\pm$ 125
12, 326 ... 12:24:23.2 - 4:43:47.2 13, 54 -1142.3 $\pm$ 1.7 -635.8 $\pm$ 1.6 4.11 2.10 10.6 $\pm$ 4.3         ...          
13, 334 ... 12:34:14.5 +20:36:33.4 8, 34 333.7 $\pm$ 1.3 -1294.8 $\pm$ 1.9 5.20 2.42 22.1 $\pm$ 3.9         ...          
14, 2632 ... 12:46:50.8 +31:47:57.0 12,127 -796.6 $\pm$ 0.8 40.9 $\pm$ 0.6 6.30 2.05 53.3 $\pm$ 2.3         ...          
15, ... 1167 A 13: 9:32.1 +28:56:45.0 7, 14 -337.6 $\pm$ 1.8 -207.9 $\pm$ 2.9 3.83 1.88 92.5 $\pm$ 5.0 84 $\pm$ 126
16, 2686 ... 13: 9:59.7 +47:44:40.5 5, 42 -634.2 $\pm$ 1.2 -606.7 $\pm$ 1.3 6.30 1.80 96.8 $\pm$ 4.7         ...          
17, 2719 ... 13:20:32.2 - 3:55:23.0 5, 64 -850.4 $\pm$ 0.9 287.5 $\pm$ 1.3 6.57 2.00 37.1 $\pm$ 3.4         ...          
18, 360 ... 13:46:53.6 + 5:43: 5.2 11, 33 -767.9 $\pm$ 1.0 -848.0 $\pm$ 1.3 4.38 2.05 17.8 $\pm$ 3.0 10.33 $\pm$ 2.854
19, 369 545 14:20: 7.5 - 9:35:49.4 8, 28 -606.7 $\pm$ 1.3 -829.2 $\pm$ 2.1 5.20 1.85 69.0 $\pm$ 4.0 71.52 $\pm$ 1.387
20, 2924 3849 14:28:36.2 +33:10:47.9 10, 29 -338.0 $\pm$ 2.9 -714.8 $\pm$ 2.5 4.38 1.15 84.5 $\pm$ 5.5 90.0 $\pm$ 1.38
21, 3343 4040 17:57:50.9 +46:34:53.3 9,155 -10.7 $\pm$ 0.6 592.0 $\pm$ 1.0 6.02 1.99 68.4 $\pm$ 2.3 73.75 $\pm$ 1.841
22, 3445 9652 A 19:14:37.5 +19:18:31.2 23,153 -630.7 $\pm$ 0.8 441.2 $\pm$ 1.3 6.30 0.41 55.7 $\pm$ 2.3 52.45 $\pm$ 2.751
23, 3482 767 A 19:46:15.1 +32: 1: 0.8 74, 93 463.9 $\pm$ 1.1 -393.8 $\pm$ 1.7 6.02 0.28 68.6 $\pm$ 3.4 74.90 $\pm$ 2.931
24, 3494 1245 A 19:53:48.9 +44:24:56.5 15,113 410.9 $\pm$ 3.2 -469.9 $\pm$ 1.5 4.11 0.52 227.9 $\pm$ 3.9 219.2 $\pm$ 1.49
25, 528 1271 22:42:43.4 +17:40:12.1 9,104 1105.0 $\pm$ 0.9 528.4 $\pm$ 1.1 5.20 1.70 57.6 $\pm$ 2.4 47.13 $\pm$ 2.961
26, 3872 4302 22:54:38.4 - 5:27:59.7 6, 32 609.9 $\pm$ 1.5 354.3 $\pm$ 2.0 5.20 2.19 40.6 $\pm$ 4.6         ...          
27, 535 4312 23: 7:42.2 +68:41:51.5 40, 70 1139.0 $\pm$ 1.3 60.3 $\pm$ 1.4 5.48 0.78 76.7 $\pm$ 2.8 63.5 $\pm$ 4.210

References. (1) Perryman et al. (1997); (2) van Maanen (1944); (3) Harrington et al. (1985); (4) Costa et al. (2005); (5) Stearns (1959); (6) Heintz (1994); (7) Jao et al. (2005); (8) Monet et al. (1992); (9) Harrington et al. (1993); (10) Dahn et al. (1982).

Notes. N* = number of reference stars; Nf = number of frames; $\Delta T$ = epoch range; COR = correction to absolute parallax.


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