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Table 2

Observational data.

Stars in Distance Spectral SpTy V K s F 3.4 F 12 F 22
Name beam (pc)a typeb ref. (mag)c (mag)d (mag)e (mag)e (mag)e

GJ 551 1 1.30 ± 0.01 M5.5 1 11.05 4.38 ± 0.03 4.20 ± 0.09 3.83 ± 0.02 3.66 ± 0.02f
GJ 699 1 1.83 ± 0.01 M4.0 1 9.57 4.52 ± 0.02 4.39 ± 0.07 4.04 ± 0.02 3.92 ± 0.03f
GJ 406 1 2.39 ± 0.01 M6.0 2 13.53 6.08 ± 0.02 5.81 ± 0.06 5.48 ± 0.02 5.31 ± 0.03f
GJ 411 1 2.54 ± 0.01 M2.0 1 7.47 3.25 ± 0.31 3.24 ± 0.14 3.05 ± 0.01 2.93 ± 0.02f
GJ 65 A/B 2 2.68 ± 0.02 M5.5 / M6.0 1 12.06 5.34 ± 0.02 5.05 ± 0.07 4.76 ± 0.02 4.62 ± 0.03
GJ 729 1 2.97 ± 0.02 M3.5 1 10.44 5.37 ± 0.02 5.16 ± 0.06 4.91 ± 0.01 4.72 ± 0.03f
GJ 905 1 3.16 ± 0.01 M5.5 1 12.29 5.93 ± 0.02 5.69 ± 0.06 5.39 ± 0.02 5.25 ± 0.03f
GJ 887 1 3.28 ± 0.01 M0.5 3 7.34 3.47 ± 0.20 3.24 ± 0.12 3.08 ± 0.01 3.00 ± 0.02f
GJ 447 1 3.35 ± 0.02 M4.0 1 11.16 5.65 ± 0.02 5.46 ± 0.06 5.18 ± 0.01 5.03 ± 0.03f
GJ 866 A/B/C 3 3.45 ± 0.05 M5.0 1 12.30 5.54 ± 0.02 5.31 ± 0.06 5.01 ± 0.02 4.88 ± 0.03
GJ 15 A 1 3.57 ± 0.01 M1.5 1 8.08 4.02 ± 0.02 3.85 ± 0.10 3.71 ± 0.02 3.60 ± 0.02f
GJ 15 B 1 3.57 ± 0.01 M3.5 1 11.06 5.95 ± 0.02 5.75 ± 0.05 5.46 ± 0.02 5.30 ± 0.03f
GJ 1111 1 3.63 ± 0.04 M6.5 1 14.90 7.26 ± 0.02 7.03 ± 0.03 6.63 ± 0.02 6.47 ± 0.06f
GJ 1061 1 3.68 ± 0.02 M5.5 1 13.09 6.61 ± 0.02 6.37 ± 0.05 6.01 ± 0.02 5.87 ± 0.03f
GJ 54.1 1 3.72 ± 0.04 M4.5 1 12.10 6.42 ± 0.02 6.17 ± 0.04 5.89 ± 0.01 5.72 ± 0.04f
GJ 273 1 3.76 ± 0.01 M3.5 1 9.85 4.86 ± 0.02 4.72 ± 0.07 4.46 ± 0.02 4.33 ± 0.03f
SCR 1845-6357 A 1 3.85 ± 0.02 M8.5 2 17.40 8.51 ± 0.02 8.14 ± 0.02 7.38 ± 0.02 7.08 ± 0.07
SO 0253+1652 1 3.85 ± 0.01 M7.0 2 15.14 7.59 ± 0.05 7.32 ± 0.03 6.90 ± 0.02 6.72 ± 0.08
GJ 191 1 3.91 ± 0.01 M1.0 4 8.85 5.05 ± 0.02 4.95 ± 0.08 4.72 ± 0.01 4.60 ± 0.03f
DEN 1048-3956 1 4.02 ± 0.02 M8.5 2 17.39 8.45 ± 0.02 8.10 ± 0.02 7.46 ± 0.02 7.23 ± 0.09
GJ 860 A/B 2 4.03 ± 0.02 M3.0 / M4.0 1 9.57 4.78 ± 0.03 4.69 ± 0.08 4.30 ± 0.01 4.12 ± 0.03
GJ 234 A/B 2 4.09 ± 0.02 M4.5 1 11.12 5.49 ± 0.02 5.29 ± 0.07 4.99 ± 0.01 4.84 ± 0.03
GJ 628 1 4.27 ± 0.03 M3.0 1 10.10 5.08 ± 0.02 4.91 ± 0.07 4.67 ± 0.01 4.57 ± 0.03f
GJ 1 1 4.34 ± 0.02 M1.5 3 8.54 4.52 ± 0.02 4.36 ± 0.09 4.20 ± 0.01 4.07 ± 0.02f
GJ 473 A/B 2 4.39 ± 0.09 M5.5 1 12.49 6.04 ± 0.02 5.79 ± 0.05 5.49 ± 0.01 5.35 ± 0.04
GJ 83.1 1 4.45 ± 0.06 M4.5 1 12.31 6.65 ± 0.02 6.44 ± 0.04 6.10 ± 0.01 5.96 ± 0.04f
GJ 687 1 4.54 ± 0.02 M3.0 1 9.17 4.55 ± 0.02 4.40 ± 0.09 4.18 ± 0.02 4.06 ± 0.02f
LHS 292 1 4.54 ± 0.07 M7.0 2 15.73 7.93 ± 0.03 7.71 ± 0.02 7.30 ± 0.02 7.03 ± 0.09f
GJ 1245 A/C 2 4.54 ± 0.02 M5.5 1 13.41 6.85 ± 0.02 6.60 ± 0.07 6.24 ± 0.02 6.08 ± 0.05
GJ 1245 B 1 4.54 ± 0.02 M6.0 1 14.01 7.39 ± 0.02 7.18 ± 0.07 6.85 ± 0.02 6.77 ± 0.09f
GJ 674 1 4.54 ± 0.03 M2.5 3 9.37 4.86 ± 0.02 4.71 ± 0.08 4.50 ± 0.02 4.34 ± 0.03f
GJ 876 A 1 4.66 ± 0.01 M3.5 1 10.18 5.01 ± 0.02 4.84 ± 0.08 4.64 ± 0.01 4.54 ± 0.03f
GJ 1002 1 4.69 ± 0.08 M5.5 1 13.77 7.44 ± 0.02 7.18 ± 0.03 6.86 ± 0.02 6.77 ± 0.08f
LHS 288 1 4.77 ± 0.06 M5.5 2 13.92 7.73 ± 0.03 7.50 ± 0.03 7.09 ± 0.02 6.75 ± 0.07f
GJ 412 A 1 4.86 ± 0.02 M1.0 1 8.77 4.77 ± 0.02 4.64 ± 0.09 4.46 ± 0.01 4.36 ± 0.02f
GJ 412 B 1 4.86 ± 0.02 M5.5 1 14.44 7.84 ± 0.03 7.61 ± 0.02 7.22 ± 0.02 7.12 ± 0.09f
GJ 388 1 4.89 ± 0.07 M4.0 4 9.29 4.59 ± 0.02 4.42 ± 0.09 4.27 ± 0.02 4.15 ± 0.03f
GJ 832 1 4.95 ± 0.02 M1.5 3 8.66 4.50 ± 0.02 4.29 ± 0.08 4.16 ± 0.01 4.05 ± 0.02f
LP 944-020 1 4.97 ± 0.10 M9.0 2 18.69 9.55 ± 0.02 9.13 ± 0.02 8.27 ± 0.02 8.00 ± 0.11f
GJ 166 C 1 4.98 ± 0.01 M4.5 3 11.24 5.96 ± 0.03 5.81 ± 0.05 5.48 ± 0.02 5.34 ± 0.04f
GJ 873 1 5.05 ± 0.02 M3.5 1 10.22 5.30 ± 0.02 5.24 ± 0.06 4.89 ± 0.02 4.75 ± 0.03
GJ 682 1 5.05 ± 0.05 M3.5 3 10.95 5.61 ± 0.02 5.35 ± 0.07 5.20 ± 0.02 5.13 ± 0.04f
GJ 1116 A/B 2 5.23 ± 0.07 M5.5 1 13.65 6.89 ± 0.02 6.64 ± 0.04 6.28 ± 0.02 6.21 ± 0.08
G 099-049 1 5.24 ± 0.05 M3.5 1 11.31 6.04 ± 0.02 5.94 ± 0.05 5.61 ± 0.02 5.47 ± 0.04
LHS 1723 1 5.32 ± 0.04 M4.0 3 12.22 6.74 ± 0.02 6.53 ± 0.05 6.23 ± 0.02 6.13 ± 0.05
GJ 445 1 5.34 ± 0.05 M3.5 1 10.79 5.95 ± 0.03 5.75 ± 0.06 5.51 ± 0.02 5.38 ± 0.03
GJ 526 1 5.41 ± 0.02 M1.5 1 8.46 4.42 ± 0.02 4.37 ± 0.10 4.19 ± 0.01 4.10 ± 0.02
GJ 169.1 A 1 5.54 ± 0.02 M4.5 5 11.04 5.72 ± 0.02 5.54 ± 0.06 5.32 ± 0.01 5.20 ± 0.03
GJ 251 1 5.61 ± 0.05 M3.0 1 10.02 5.28 ± 0.02 5.16 ± 0.07 4.92 ± 0.02 4.78 ± 0.03
2MA 1835+3259 1 5.67 ± 0.02 M8.5 6 18.27 9.17 ± 0.02 8.80 ± 0.02 8.16 ± 0.02 7.89 ± 0.13
GJ 205 1 5.68 ± 0.03 M1.5 1 7.95 4.04 ± 0.26 3.74 ± 0.12 3.70 ± 0.02 3.63 ± 0.02
LP 816-060 1 5.71 ± 0.11 M4.0 7 11.50 6.20 ± 0.02 6.02 ± 0.05 5.77 ± 0.02 5.63 ± 0.04
GJ 229 A 1 5.75 ± 0.03 M1.0 1 8.14 4.17 ± 0.23 4.06 ± 0.13 3.97 ± 0.02 3.82 ± 0.04
GJ 213 1 5.83 ± 0.03 M4.0 1 11.57 6.39 ± 0.02 6.23 ± 0.05 5.90 ± 0.02 5.68 ± 0.04
GJ 693 1 5.84 ± 0.08 M2.0 3 10.76 6.02 ± 0.02 5.92 ± 0.06 5.60 ± 0.02 5.48 ± 0.04
GJ 752 A 1 5.85 ± 0.02 M3.0 1 9.10 4.67 ± 0.02 4.47 ± 0.08 4.38 ± 0.01 4.27 ± 0.03
GJ 752 B 1 5.85 ± 0.02 M8.0 1 17.45 8.77 ± 0.02 8.47 ± 0.02 8.08 ± 0.02 N/A
GJ 570 B/C 2 5.86 ± 0.02 M1.0 1 8.09 3.80 ± 0.23 4.06 ± 0.06 3.74 ± 0.02 3.62 ± 0.03
GJ 754 1 5.91 ± 0.05 M4.5 3 12.23 6.85 ± 0.03 6.65 ± 0.03 6.36 ± 0.02 6.20 ± 0.06
GJ 588 1 5.93 ± 0.04 M2.5 3 9.31 4.76 ± 0.02 4.70 ± 0.07 4.46 ± 0.01 4.36 ± 0.03
GJ 1005 A/B 2 5.94 ± 0.03 M4.0 1 11.49 6.39 ± 0.02 6.17 ± 0.04 5.91 ± 0.02 5.81 ± 0.04
GJ 908 1 5.95 ± 0.04 M1.0 1 8.98 5.04 ± 0.02 5.02 ± 0.07 4.76 ± 0.02 4.66 ± 0.03
GJ 285 1 5.98 ± 0.07 M4.0 1 11.19 5.70 ± 0.02 5.51 ± 0.06 5.29 ± 0.01 5.13 ± 0.03
GJ 268 A/B 2 6.12 ± 0.07 M4.5 1 11.48 5.85 ± 0.02 5.69 ± 0.06 5.38 ± 0.02 5.20 ± 0.03
GJ 784 1 6.20 ± 0.04 K7.0 3 7.95 4.28 ± 0.02 4.15 ± 0.10 4.05 ± 0.02 3.98 ± 0.02
GJ 555 1 6.22 ± 0.08 M3.5 1 11.32 5.94 ± 0.03 5.79 ± 0.06 5.54 ± 0.02 5.41 ± 0.03
GJ 896 A/B 2 6.25 ± 0.06 M3.5 / M4.5 1 10.10 4.94 ± 0.03 4.76 ± 0.08 4.64 ± 0.02 4.59 ± 0.03
GJ 581 1 6.34 ± 0.07 M2.5 1 10.57 5.84 ± 0.02 5.69 ± 0.06 5.48 ± 0.01 5.33 ± 0.03
LHS 2090 1 6.37 ± 0.11 M6.0 2 16.10 8.44 ± 0.02 8.23 ± 0.03 7.80 ± 0.02 7.96 ± 0.22
LHS 337 1 6.38 ± 0.08 M4.5 3 12.75 7.39 ± 0.02 7.24 ± 0.03 6.86 ± 0.02 6.72 ± 0.05
GJ 661 A/B 2 6.40 ± 0.05 M3.0 1 9.37 4.83 ± 0.02 4.71 ± 0.08 4.46 ± 0.02 4.34 ± 0.02
G 180-060 1 6.41 ± 0.16 M5.0 3 14.76 8.51 ± 0.02 8.29 ± 0.02 7.95 ± 0.02 7.90 ± 0.13
GJ 644 A/B/D 3 6.45 ± 0.02 M2.5 1 9.03 4.40 ± 0.04 4.22 ± 0.09 4.04 ± 0.02 3.90 ± 0.03
GJ 644 C 1 6.45 ± 0.02 M7.0 1 16.78 8.82 ± 0.02 8.59 ± 0.02 8.13 ± 0.02 7.86 ± 0.18f
GJ 643 1 6.45 ± 0.02 M3.5 1 11.80 6.72 ± 0.02 6.57 ± 0.03 6.29 ± 0.02 6.12 ± 0.05
GJ 625 1 6.53 ± 0.04 M1.5 1 10.10 5.83 ± 0.02 5.68 ± 0.06 5.46 ± 0.02 5.33 ± 0.02
GJ 1128 1 6.53 ± 0.10 M4.5 1 12.74 7.04 ± 0.02 6.80 ± 0.03 6.51 ± 0.01 6.40 ± 0.03
GJ 1156 1 6.54 ± 0.13 M5.0 1 13.80 7.57 ± 0.03 7.33 ± 0.03 6.99 ± 0.02 6.91 ± 0.08
LHS 3003 1 6.56 ± 0.09 M7.0 1 17.05 8.93 ± 0.03 8.69 ± 0.02 8.27 ± 0.02 8.12 ± 0.27f
GJ 408 1 6.70 ± 0.07 M2.5 3 10.02 5.50 ± 10.00 5.38 ± 0.06 5.19 ± 0.01 5.09 ± 0.03
GJ 829 A/B 2 6.71 ± 0.08 M3.5 1 10.30 5.45 ± 0.02 5.30 ± 0.07 5.06 ± 0.01 4.90 ± 0.03
G 041-014 A/B/C 3 6.77 ± 0.09 M3.5 3 11.46 5.69 ± 0.02 5.49 ± 0.06 5.25 ± 0.02 5.08 ± 0.03
GJ 402 1 6.80 ± 0.14 M4.0 1 11.65 6.37 ± 0.02 6.26 ± 0.05 5.98 ± 0.02 5.86 ± 0.04
GJ 880 1 6.83 ± 0.04 M1.5 1 8.65 4.52 ± 0.02 4.43 ± 0.08 4.33 ± 0.01 4.22 ± 0.02
GJ 299 1 6.84 ± 0.14 M4.0 1 12.82 7.66 ± 0.03 7.44 ± 0.03 7.12 ± 0.02 7.01 ± 0.09

Notes. 

(a)

Distances calculated from RECONS parallaxes (Henry et al. 2006).

(b)

Spectral types from the literature. When only one spectral type is given for a binary/multiple system, this represents the spectral type of the whole system and the individual spectral types are unknown. The sources of the spectral type are given in the next column and are: 1) Henry et al. (2002), 2) Henry et al. (2004), 3) Hawley et al. (1996), 4) Keenan & McNeil (1989), 5) Gray et al. (2003), 6) Reid et al. (2003), 7) Gray et al. (2006).

(c)

V magnitudes taken from the RECONS database; where more than one star is in the WISE/2MASS beam, the fluxes are added.

(d)

Ks magnitudes and errors are taken from the 2MASS database (Skrutskie et al. 2006); where more than one star is in the WISE beam, the fluxes of all stars in the beam are added.

(e)

WISE bands w1 centered at 3.4 μm, w3 centered at 12 μm, and w4 centered at 22 μm (Wright et al. 2010).

(f)

Stars with 24 μm Spitzer flux measurements from Gautier et al. (2007).

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