Table 3:

Derived parameters from model comparisons.

ID, LHS	MK	M/H	Mass	Age
	Type		()	(Gyr)	(km s-1)
1,1047*	M41	0	0.16-0.18	0.08-0.17	22 1
2, 1050	M3.51	0	0.21-0.23	0.125-10	37 1
3, 1104		0	0.42-0.46	0.12-10	59 3
4, 1475	M11	0	0.55-0.58	0.12-0.30	48 4
5, 228		-1	0.10-0.14	0.05-0.20	206 10
6, 1923	M62	0	0.10-0.11	0.4-10	98 4
7, 243		-.5	0.08-0.11	0.11-0.25	179 5
8, 1976*		0	0.53-0.61	0.055-10	83 10
9, 2065	M9e3	0	0.06-0.07	0.25-0.45	23 1
10, 306	M5.54	0	0.10-0.13	0.04-10	80 18
11, 2472	M3.51	0	0.18-0.21	0.12-10	43 2
12, 326		-.5	0.34-0.44	0.035-10	582 238
13, 334		-1	0.09-0.10	0.3-10	286 51
14, 2632	M7.55	0	0.08-0.10	0.6-10	60 3
15, ...	M41	0	0.11-0.14	0.12-10	19 1
16, 2686		0	0.08-0.10	0.09-0.18	36 2
17, 2719		0	0.14-0.16	0.2-10	114 11
18, 360		-1	0.20-0.35	0.2-10	304 51
19, 369	M41	0	0.18-0.22	0.060-0.105	70 4
20, 2924	M9e3	0	0.07-0.08	0.6-10	43 3
21, 3343	M36	0	0.37-0.42	0.070-0.105	41 1
22, 3445*	M31	0	0.36-0.45	0.03-0.05	63 3
23, 3482	M1.53	0	0.60-0.62	0.2-10	38 2
24, 3494*	M5.5e3	0	0.09-0.11	0.12-0.20	12 0
25, 528	M31	0	0.39-0.45	0.065-0.1	97 4
26, 3872	M46	0	0.23-0.28	0.06-0.125	82 9
27, 535	M3.56	-.5	0.16-0.20	0.05-0.12	26 1

References. ⁽¹⁾ Bidelman (1985); ⁽²⁾ Fleming et al. (1993); ⁽³⁾ Leggett (1992); ⁽⁴⁾ Mathioudakis & Doyle (1991); ⁽⁵⁾ Kirkpatrick et al. (1995); ⁽⁶⁾ Gliese & Jahreiß (1991).

Notes. The mass and age ranges are based only on the errors in the parallax and photometry and do not include the systematic error of uncertain metallicity. The latter can have a large impact on mass and age as described in Sect. 4.2. ^(*) These are known or suspect unresolved binary systems while the parameters are based on an assumption of being single stars. Unaccounted multiplicity will tend to increase the predicted age and decrease the predicted mass.