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No.	Name	R.A. (1950)	Dec (1950)	K	J-K	H-K	ref.
1	G158-100	00 31 22.7	-12 24 29	12.967	0.462	0.081	2
2	SA92-342	00 52 36.0	00 26 58	10.466	0.247	0.038	1
3	F 11	01 01 46.6	03 57 34	12.822	-0.222	-0.097	1, 2
4	SA93-317	01 52 03.7	00 28 20	10.264	0.292	0.040	1
5	F 16	01 52 04.7	-07 00 47	12.342	-0.007	-0.002	1, 2
6	F 22	02 27 39.2	05 02 34	13.374	-0.135	-0.069	1, 2
7	SA94-242	02 54 47.2	00 06 39	10.940	0.165	0.037	1
8	SA94-251	02 55 12.9	00 04 04	8.313	0.766	0.129	1
9	SA94-702	02 55 38.8	00 58 54	8.266	0.884	0.158	1
10	GD 50	03 46 17.4	-01 07 38	14.919	-0.170	-0.049	2
11	SA96-83	04 50 25.4	-00 19 34	11.278	0.076	0.016	1
12	GD 71	05 49 34.8	15 52 37	13.898	-0.217	-0.091	1
13	SA97-249	05 54 33.8	00 00 53	10.135	0.382	0.047	1
14	Rubin 149	07 21 41.2	-00 27 10	14.261	-0.153	-0.079	2
15	M67-I-48	08 48 21.9	11 55 02	12.360	0.418	0.060	3
16	M67-IV-8	08 48 31.0	12 00 36	12.631	0.340	0.038	3
17	M67-IV-27	08 48 35.4	12 03 26	12.270	0.411	0.073	3
18	SA100-280	08 51 02.1	-00 25 14	10.522	0.292	0.031	1
19	G162-66	10 31 14.5	-11 26 08	13.796	-0.231	-0.142	1, 2
20	G163-50	11 05 27.6	-04 53 04	13.473	-0.120	-0.069	1, 2
23	M3-193	13 39 25.7	28 44 59	12.374	0.623	0.072	4
24	SA106-1024	14 37 33.3	00 14 36	10.753	0.151	0.019	1
25	SA107-1006	15 35 59.9	00 24 03	9.756	0.475	0.070	1
26	SA108-475	16 34 26.3	-00 28 39	7.972	0.858	0.155	1
27	M13-A14	16 38 54.2	36 26 56	13.123	0.371	0.058	4
28	SA109-71	17 41 32.5	-00 23 44	10.597	0.148	0.047	1
35	G21-15 see note below	18 24 44.5	04 01 17	11.757	0.474	0.089	2
29	G93-48	21 49 53.0	02 09 16	13.346	-0.171	-0.075	1, 2
30	SA114-750	22 39 11.3	00 56 55	12.015	-0.092	-0.036	1
31	GD 246	23 09 50.4	10 30 46	14.039	-0.241	-0.120	1, 2
32	F 108	23 13 38.2	-02 06 58	13.664	-0.205	-0.088	1, 2

Note re G21-15: FS 35 is not the originally intended target, G21-15, but a nearby anonymous star. The coordinates for G21-15 in Turnshek et al (1990) are incorrect. (Those in Landolt 1983, 1992 are correct, however.) The star we have designated FS 35 has no optical photometry or spectroscopy known to us so the chance of variability is higher than for the other standards. However the 15 JHK observations on 8 nights show no significant signs of variability. Note also that finding chart linked here is also in error.

References: 1. Landolt 1983 A.J. 88, 439 2. Turnshek et al 1990 A.J. 99, 1243 3. Eggen and Sandage Ap.J. 140,130 4. Private communication 5. Courteau, S., A Compilation of the UKIRT Faint JHK Standards, NOAO, 1995