Table 2: Positions observed in CO(1-0) with the IRAM 30 m telescope. Column 3 gives the rms noise level for each spectrum in milliKelvins (main beam brightness temperature) and Col. 4 the uncertainty in the CO integrated intensity in K km s^-1.

RA	Dec	rms
B1950	B1950	mK	K km s-1
9:53:05.0	69:21:30	20.3	0.15
9:53:05.0	69:22:00	20.6	0.15
9:53:05.0	69:22:30	19.5	0.14
9:53:05.0	69:23:00	20.1	0.14
9:53:05.0	69:23:30	20.5	0.15
9:53:05.0	69:24:00	20.9	0.15
9:53:20.0	69:30:00	13.5	0.10
9:53:22.0	69:30:00	21.9	0.16
9:53:18.0	69:30:00	20.4	0.15
9:53:22.0	69:29:30	14.5	0.10
9:53:20.0	69:29:30	22.9	0.17
9:53:20.0	69:30:30	19.7	0.14
9:53:18.0	69:30:30	14.3	0.10
9:53:18.0	69:31:00	13.8	0.10
9:53:16.0	69:31:00	13.3	0.10
9:53:27.0	69:31:18	11.3	0.08
9:53:29.0	69:31:18	14.8	0.11
9:53:27.0	69:31:48	16.2	0.12
9:53:25.0	69:31:18	15.9	0.11
9:53:27.0	69:30:48	15.3	0.11
9:53:55.9	69:18:20	22.7	0.16
9:53:55.9	69:18:40	22.7	0.16
9:53:55.9	69:19:00	21.6	0.16
9:53:55.9	69:19:20	21.8	0.16
9:53:55.9	69:19:40	21.6	0.16
9:53:55.9	69:20:00	22.8	0.16
9:53:54.8	69:19:50	14.1	0.10
9:53:54.8	69:19:30	13.6	0.10
9:53:54.8	69:19:10	13.0	0.09
9:53:48.0	69:18:09	07.4	0.05
9:53:49.1	69:17:55	09.0	0.06
9:53:49.1	69:17:35	09.0	0.06