Table 2: Adaptive optics measurement of the new low-mass companions. Gl 268.3 was observed with the Keck adaptive optics system. All other observations were obtained at CFHT with the PUEO adaptive optics system. Periods listed within parentheses are estimated from the observed separation, the distance to the system and its approximate mass. They are uncertain by a factor of approximately 3. 0.5 dex.
Name $\rho$ $\theta$ $\Delta m$ Date Filt. Period Accurate mass

'' $\deg$ (yr) prospects

G 131-26AB 0.111 169.9 0.46 07 Aug. 2001 H (4) Excellent

LP 467-16AB 0.409 147.2 0.69 16 Aug. 2000 K (20) Fair

Gl 84 0.39 101 3.59 23 Jul. 2002 H (15) Fair

Gl 120.1CD 0.083 170.1 0.02 15 Aug. 2000 H 1.54 Mediocre

LHS 1630 0.61 72 0.34 18 Sep. 2002 K (50) Poor

Gl 173.1AabC 0.474 188.0 1.91 05 Mar. 1999 K (80) Poor

G 39-29 0.54 299 0.42 13 Sep. 2002 K (35) Mediocre

Gl 186 0.31 298 2.00 19-Sep. 2002 K (40) Mediocre

LHS 224AB 0.163 344.7 0.14 18 Apr. 2000 K 3.19 Good

Gl 263AB 0.110 287.4 0.46 26 Feb. 1999 H 3.62 Excellent

Gl 268.3AB 0.054 153.6 0.57 25 Feb. 2000 H 0.834 Excellent

Gl 277AC 0.684 195.0 2.02 20 Apr. 2000 K (35) Mediocre

GJ 2069AD 0.682 158.0 3.20 18 Feb. 2000 K (40) Fair

GJ 2069BC 0.549 219.1 0.52 18 Feb. 2000 K (30) Fair

Gl 346AB 0.431 101.0 0.80 04 Apr. 1999 H (60) Poor

GJ 1138AB 0.303 56.1 1.89 20 Apr. 2000 K (10) Good

Gl 416AB 0.138 85.0 1.05 19 Feb. 2000 K 7.33 Good

Gl 494AB 0.475 81.5 4.41 19 Feb. 2000 K 14.5 Good

Gl 508AC 0.092 281.7 0.43 20 Apr. 2000 K 1.22 Good

Gl 508AB 0.579 102.0 0.29 20 Apr. 2000 K 49 Fair

G165-8AB 0.174 253.3 0.16 19 Feb. 2000 K (7) Good

Gl 533AB 0.230 352.8 2.02 04 Apr. 1999 H 7.36 Fair

Gl 563.4AB 0.383 139.0 3.40 26 Feb. 1999 H 16.07 Fair

Gl 588.1AB 0.408 109.6 0.97 04 Apr. 1999 K (60) Poor

Gl 609.2AB 0.220 287.0 2.04 04 Apr. 1999 H 12.15 Good

Gl 782AB 0.991 74.5 3.26 03 Jul. 2001 K (100) Poor

Gl 852BC 0.978 305.8 1.18 07 Aug. 2001 K (70) Poor

G 67-53AB 0.142 209.0 1.17 05 Aug. 2001 J (5) Excellent

LHS 4022AB 1.527 74.3 1.43 05 Aug. 2001 H (150) Poor

**Table 2:** Adaptive optics measurement of the new low-mass companions. Gl 268.3 was observed with the Keck adaptive optics system. All other observations were obtained at CFHT with the PUEO adaptive optics system. Periods listed within parentheses are estimated from the observed separation, the distance to the system and its approximate mass. They are uncertain by a factor of approximately 3. 0.5 dex.
Name	$\rho$	$\theta$	$\Delta m$	Date	Filt.	Period	Accurate mass
	''	$\deg$				(yr)	prospects
G 131-26AB	0.111	169.9	0.46	07 Aug. 2001	H	(4)	Excellent
LP 467-16AB	0.409	147.2	0.69	16 Aug. 2000	K	(20)	Fair
Gl 84	0.39	101	3.59	23 Jul. 2002	H	(15)	Fair
Gl 120.1CD	0.083	170.1	0.02	15 Aug. 2000	H	1.54	Mediocre
LHS 1630	0.61	72	0.34	18 Sep. 2002	K	(50)	Poor
Gl 173.1AabC	0.474	188.0	1.91	05 Mar. 1999	K	(80)	Poor
G 39-29	0.54	299	0.42	13 Sep. 2002	K	(35)	Mediocre
Gl 186	0.31	298	2.00	19-Sep. 2002	K	(40)	Mediocre
LHS 224AB	0.163	344.7	0.14	18 Apr. 2000	K	3.19	Good
Gl 263AB	0.110	287.4	0.46	26 Feb. 1999	H	3.62	Excellent
Gl 268.3AB	0.054	153.6	0.57	25 Feb. 2000	H	0.834	Excellent
Gl 277AC	0.684	195.0	2.02	20 Apr. 2000	K	(35)	Mediocre
GJ 2069AD	0.682	158.0	3.20	18 Feb. 2000	K	(40)	Fair
GJ 2069BC	0.549	219.1	0.52	18 Feb. 2000	K	(30)	Fair
Gl 346AB	0.431	101.0	0.80	04 Apr. 1999	H	(60)	Poor
GJ 1138AB	0.303	56.1	1.89	20 Apr. 2000	K	(10)	Good
Gl 416AB	0.138	85.0	1.05	19 Feb. 2000	K	7.33	Good
Gl 494AB	0.475	81.5	4.41	19 Feb. 2000	K	14.5	Good
Gl 508AC	0.092	281.7	0.43	20 Apr. 2000	K	1.22	Good
Gl 508AB	0.579	102.0	0.29	20 Apr. 2000	K	49	Fair
G165-8AB	0.174	253.3	0.16	19 Feb. 2000	K	(7)	Good
Gl 533AB	0.230	352.8	2.02	04 Apr. 1999	H	7.36	Fair
Gl 563.4AB	0.383	139.0	3.40	26 Feb. 1999	H	16.07	Fair
Gl 588.1AB	0.408	109.6	0.97	04 Apr. 1999	K	(60)	Poor
Gl 609.2AB	0.220	287.0	2.04	04 Apr. 1999	H	12.15	Good
Gl 782AB	0.991	74.5	3.26	03 Jul. 2001	K	(100)	Poor
Gl 852BC	0.978	305.8	1.18	07 Aug. 2001	K	(70)	Poor
G 67-53AB	0.142	209.0	1.17	05 Aug. 2001	J	(5)	Excellent
LHS 4022AB	1.527	74.3	1.43	05 Aug. 2001	H	(150)	Poor

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