**Table 1:** Zeeman splitting results.
Source		$\alpha_{\rm J2000}$	$\delta_{\rm J2000}$	$V_{\rm LSR}$	Peak Flux	Int. Flux	$\Delta V_{\rm z}$	\|B\|
		hh mm ss	$^\circ~'~''$	km s^-1	(Jy/beam)	(Jy/beam)	m s^-1	(mG)
09.62+0.20^a		18 06 14.66	-20 31 31.60	1.0	6757	3091	- $0.137\pm0.002$	- $2.80\pm0.04$
				-0.1^b			$0.42\pm0.02$	$8.6\pm0.4$
				1.2^b			$-0.145\pm0.002$	$-2.96\pm0.04$
12.89+0.49^a	IRAS 18089-1732	18 11 51.46	-17 31 28.84	39.3	71	105	$0.41\pm0.03$	$8.4\pm0.7$
				34.8^b			$0.18\pm0.05$	$4\pm1$
				39.2^b			$0.59\pm0.05$	$12\pm1$
23.01-0.41^a		18 34 40.37	-09 00 38.30	74.8	585	1016	- $1.49\pm0.03$	- $30.3\pm0.7$
				74.9^b			- $1.49\pm0.02$	- $30.3\pm0.4$
				81.0^b			$0.7\pm0.1$	$14\pm2$
25.71+0.04		18 38 03.10	-06 24 32.00	95.6	590	591	<0.06	<1.2
25.83-0.18		18 39 04.70	-06 24 17.00	90.7	69	84	$0.99\pm0.20$	$20\pm4$
28.15+0.00		18 42 41.00	-04 15 21.00	101.3	30	24	<1.8	<37
31.28+0.06	IRAS 18456-0129	18 48 12.38	-01 26 22.60	110.4	74	174	$2.06\pm0.26$	$42\pm5$
32.03+0.06	IRAS 18470-0050	18 49 37.04	-00 46 50.10	98.7	69	81	<0.51	<11
33.64-0.21		18 53 28.70	+00 31 58.00	58.6	63	54	- $0.89\pm0.17$	- $18\pm3$
35.20-0.74	IRAS 18556+0136	18 58 12.98	+01 40 37.50	30.5	169	167	$0.81\pm0.04$	$16.5\pm0.7$
35.20-1.74	W48	19 01 45.60	+01 13 28.00	41.5	476	643	$0.32\pm0.02$	$6.4\pm0.3$
37.40+1.52	IRAS 18517+0437	18 54 13.80	+04 41 32.00	41.0	320	193	$0.75\pm0.02$	$15.4\pm0.4$
43.80-0.13	W49N	19 11 55.10	+09 36 00.00	40.0	35	81	<1.9	<39
49.49-0.39	W51-e1/e2	19 23 44.50	+14 30 31.00	59.0	1029	885	$0.72\pm0.04$	$14.7\pm0.8$
69.52-0.97	ON1	20 10 09.07	+31 31 34.40	11.6	96	45	<0.2	<4.1
78.10+3.64	IRAS 20126+4104	20 14 26.04	+41 13 33.39	-6.1	60	77	<0.8	<17
81.87+0.78^a	W75N	20 38 36.80	+42 37 59.00	5.0	273	317	$0.40\pm0.02$	$8.2\pm0.3$
				5.0^b			$0.28\pm0.02$	$5.7\pm0.4$
				7.3^b			$0.46\pm0.02$	$9.4\pm0.4$
109.86+2.10	Cepheus A	22 56 18.09	+62 01 49.45	-4.2	364	484	$0.39\pm0.01$	$8.1\pm0.2$
111.53+0.76^a	NGC 7538	23 13 45.36	+61 28 10.55	-56.1	233	514	$0.79\pm0.03$	$16.2\pm0.6$
				-58^b			$0.78\pm0.04$	$16.0\pm0.8$
				-56^b			$0.59\pm0.02$	$12.1\pm0.4$
133.94+1.04	W3(OH)	02 27 04.72	+61 52 24.73	-44.0	3705	8198	$0.141\pm0.003$	$2.87\pm0.05$
173.49+2.42	S231	05 39 13.06	+35 45 51.29	-13.0	52	53	$0.95\pm0.11$	$19\pm2$
174.19-0.09	AFGL 5142	05 30 42.00	+33 47 14.00	2.1	55	34	<0.8	<18
188.95+0.89	IRAS 06058+2138	06 08 53.35	+21 38 28.67	10.9	633	485	- $0.49\pm0.02$	- $9.9\pm0.4$
192.60-0.05	S255	06 12 54.02	+17 59 23.00	5.0	94	78	$0.47\pm0.05$	$9.6\pm0.9$

^a Significant magnetic field changes across the maser spectrum.
^b Velocity of the maser feature for which Zeeman splitting was determined separately.

Source LaTeX | All tables | In the text