Table 1: Positions of the IRAS point sources satisifying the Sridharan et al. (2002) criteria, precessed to J2000 co-ordinates, alongside the kinematic distance of the IRAS source and date(s) of observation. All sources were observed during the spring and summer of 2000. All distances are taken from Sridharan et al. 2002 with the exception of IRAS 18449-0158, for which we derive the kinematic distance using $V_{\rm LSR}$ from the CS(2-1) observations of Bronfman et al. (1996). Candidates with only the far kinematic distance listed have had their distance uncertainty resolved.
IRAS Source Position (J2000) Distance (kpc) Date(s) of

$\alpha$ $\delta$ far near observation

05358+3543 05 39 10.4 +35 45 19 1.8 03/18

05490+2658 05 52 12.9 +26 59 33 2.1 03/18

05553+1631 05 58 13.9 +16 32 00 2.5 03/18

18089-1732 18 11 51.3 -17 31 29 13.0 3.6 05/11

18090-1832 18 12 01.9 -18 31 56 10.0 6.6 05/11

18102-1800 18 13 12.2 -17 59 35 14.0 2.6 05/11

18151-1208 18 17 57.1 -12 07 22 3.0 05/11

18159-1550 18 18 47.6 -15 48 54 11.7 4.7 05/11

18182-1433 18 21 07.9 -14 31 53 11.8 4.5 05/11

18223-1243 18 25 11.1 -12 42 15 12.4 3.7 05/11

18247-1147 18 27 31.1 -11 45 56 9.3 6.7 05/11

18264-1152 18 29 14.3 -11 50 26 12.5 3.5 05/11

18272-1217 18 30 02.7 -12 15 27 2.9 05/11

18290-0924 18 31 44.8 -09 22 09 10.5 5.3 05/11

18306-0835 18 33 21.8 -08 33 39 10.7 4.9 05/11

18308-0841 18 33 31.9 -08 39 17 10.7 4.9 05/11

18310-0825 18 33 47.2 -08 23 35 10.4 5.2 05/11

18337-0743 18 36 29.0 -07 40 33 11.5 4 05/11, 05/30

18345-0641 18 37 16.8 -06 38 32 9.5 05/11

18348-0616 18 37 29.0 -06 14 15 9.0 6.3 05/11

18372-0541 18 39 56.0 -05 38 49 13.4 1.8 05/11

18385-0512 18 41 12.0 -05 09 07 13.1 2 05/23

18426-0204 18 45 12.8 -02 01 12 13.5 1.1 05/23

18431-0312 18 45 46.9 -03 09 24 8.2 6.7 05/23

18437-0216 18 46 22.7 -02 13 24 7.3 05/23

18440-0148 18 46 36.3 -01 45 23 8.3 05/23

18445-0222 18 47 10.8 -02 19 06 9.4 5.3 06/13

18447-0229 18 47 23.7 -02 25 55 8.2 6.6 05/30

18449-0158 18 47 35.6 -01 55 26 8.7 5.9 06/13

18454-0136 18 48 03.7 -01 33 23 11.9 2.7 05/30

18454-0158 18 48 01.3 -01 54 49 5.6 06/13

18460-0307 18 48 39.2 -03 03 53 9.5 5.2 05/30

18470-0044 18 49 36.7 -00 41 05 8.2 06/13

18472-0022 18 49 50.7 -00 19 09 11.1 3.2 05/30

18488+0000 18 51 24.8 +00 04 18 8.9 5.4 06/13

18521+0134 18 54 40.8 +01 38 01 9.0 5 05/30

18530+0215 18 55 34.2 +02 19 08 8.7 5.1 06/13

18540+0220 18 56 35.6 +02 24 54 10.6 3.3 05/30

18553+0414 18 57 53.0 +04 18 06 12.9 0.6 06/19

18566+0408 18 59 09.9 +04 12 14 6.7 05/30

19012+0536 19 03 45.1 +05 40 40 8.6 4.6 05/23

19035+0641 19 06 01.1 +06 46 35 2.2 05/23

19074+0752 19 09 53.3 +07 57 22 8.9 3.7 05/23

19175+1357 19 19 49.1 +14 02 46 10.6 05/23

19217+1651 19 23 58.8 +16 57 36 10.5 05/23

19220+1432 19 24 19.7 +14 38 03 5.5 06/13

19266+1745 19 28 54.0 +17 51 56 10.0 0.3 05/30

19282+1814 19 30 28.1 +18 20 53 8.2 1.9 05/30

19403+2258 19 42 27.2 +23 05 12 6.3 2.4 06/13

19410+2336 19 43 11.6 +23 44 06 6.4 2.1 05/30

19411+2306 19 43 18.1 +23 13 59 5.8 2.9 06/13

19413+2332 19 43 29.0 +23 40 04 6.8 1.8 05/30

19471+2641 19 49 09.9 +26 48 51 2.4 06/13

20051+3435 20 07 03.8 +34 44 35 3.7 1.6 05/11

20081+2720 20 10 11.5 +27 29 06 0.7 05/11, 05/23

20126+4104 20 14 26.0 +41 13 31 1.7 05/11

20205+3948 20 22 22.0 +39 58 05 4.5 05/11, 05/30

20216+4107 20 23 23.8 +41 17 40 1.7 05/11

20293+3952 20 31 10.7 +40 03 10 2.0 1.3 05/11

20319+3958 20 33 49.4 +40 08 45 1.6 05/11

20332+4124 20 35 00.5 +41 34 48 3.9 05/23

20343+4129 20 36 07.1 +41 40 01 1.4 05/23

22134+5834 22 15 09.1 +58 49 09 2.6 05/06

22551+6221 22 57 05.2 +62 37 44 0.7 05/06, 05/23

22570+5912 22 59 06.5 +59 28 28 5.1 05/06, 05/23

23033+5951 23 05 25.2 +60 08 11 3.5 05/06

23139+5939 23 16 09.3 +59 55 23 4.8 05/06

23151+5912 23 17 21.1 +59 28 49 5.7 05/06

23545+6508 23 57 05.2 +65 25 11 0.8 05/06, 05/23

**Table 1:** Positions of the IRAS point sources satisifying the Sridharan et al. (2002) criteria, precessed to J2000 co-ordinates, alongside the kinematic distance of the IRAS source and date(s) of observation. All sources were observed during the spring and summer of 2000. All distances are taken from Sridharan et al. 2002 with the exception of IRAS 18449-0158, for which we derive the kinematic distance using $V_{\rm LSR}$ from the CS(2-1) observations of Bronfman et al. (1996). Candidates with only the far kinematic distance listed have had their distance uncertainty resolved.
IRAS Source	Position (J2000)	Distance (kpc)	Date(s) of
	$\alpha$	$\delta$	far	near	observation
05358+3543	05 39 10.4	+35 45 19	1.8		03/18
05490+2658	05 52 12.9	+26 59 33	2.1		03/18
05553+1631	05 58 13.9	+16 32 00	2.5		03/18
18089-1732	18 11 51.3	-17 31 29	13.0	3.6	05/11
18090-1832	18 12 01.9	-18 31 56	10.0	6.6	05/11
18102-1800	18 13 12.2	-17 59 35	14.0	2.6	05/11
18151-1208	18 17 57.1	-12 07 22	3.0		05/11
18159-1550	18 18 47.6	-15 48 54	11.7	4.7	05/11
18182-1433	18 21 07.9	-14 31 53	11.8	4.5	05/11
18223-1243	18 25 11.1	-12 42 15	12.4	3.7	05/11
18247-1147	18 27 31.1	-11 45 56	9.3	6.7	05/11
18264-1152	18 29 14.3	-11 50 26	12.5	3.5	05/11
18272-1217	18 30 02.7	-12 15 27	2.9		05/11
18290-0924	18 31 44.8	-09 22 09	10.5	5.3	05/11
18306-0835	18 33 21.8	-08 33 39	10.7	4.9	05/11
18308-0841	18 33 31.9	-08 39 17	10.7	4.9	05/11
18310-0825	18 33 47.2	-08 23 35	10.4	5.2	05/11
18337-0743	18 36 29.0	-07 40 33	11.5	4	05/11, 05/30
18345-0641	18 37 16.8	-06 38 32	9.5		05/11
18348-0616	18 37 29.0	-06 14 15	9.0	6.3	05/11
18372-0541	18 39 56.0	-05 38 49	13.4	1.8	05/11
18385-0512	18 41 12.0	-05 09 07	13.1	2	05/23
18426-0204	18 45 12.8	-02 01 12	13.5	1.1	05/23
18431-0312	18 45 46.9	-03 09 24	8.2	6.7	05/23
18437-0216	18 46 22.7	-02 13 24	7.3		05/23
18440-0148	18 46 36.3	-01 45 23	8.3		05/23
18445-0222	18 47 10.8	-02 19 06	9.4	5.3	06/13
18447-0229	18 47 23.7	-02 25 55	8.2	6.6	05/30
18449-0158	18 47 35.6	-01 55 26	8.7	5.9	06/13
18454-0136	18 48 03.7	-01 33 23	11.9	2.7	05/30
18454-0158	18 48 01.3	-01 54 49	5.6		06/13
18460-0307	18 48 39.2	-03 03 53	9.5	5.2	05/30
18470-0044	18 49 36.7	-00 41 05	8.2		06/13
18472-0022	18 49 50.7	-00 19 09	11.1	3.2	05/30
18488+0000	18 51 24.8	+00 04 18	8.9	5.4	06/13
18521+0134	18 54 40.8	+01 38 01	9.0	5	05/30
18530+0215	18 55 34.2	+02 19 08	8.7	5.1	06/13
18540+0220	18 56 35.6	+02 24 54	10.6	3.3	05/30
18553+0414	18 57 53.0	+04 18 06	12.9	0.6	06/19
18566+0408	18 59 09.9	+04 12 14	6.7		05/30
19012+0536	19 03 45.1	+05 40 40	8.6	4.6	05/23
19035+0641	19 06 01.1	+06 46 35	2.2		05/23
19074+0752	19 09 53.3	+07 57 22	8.9	3.7	05/23
19175+1357	19 19 49.1	+14 02 46	10.6		05/23
19217+1651	19 23 58.8	+16 57 36	10.5		05/23
19220+1432	19 24 19.7	+14 38 03	5.5		06/13
19266+1745	19 28 54.0	+17 51 56	10.0	0.3	05/30
19282+1814	19 30 28.1	+18 20 53	8.2	1.9	05/30
19403+2258	19 42 27.2	+23 05 12	6.3	2.4	06/13
19410+2336	19 43 11.6	+23 44 06	6.4	2.1	05/30
19411+2306	19 43 18.1	+23 13 59	5.8	2.9	06/13
19413+2332	19 43 29.0	+23 40 04	6.8	1.8	05/30
19471+2641	19 49 09.9	+26 48 51	2.4		06/13
20051+3435	20 07 03.8	+34 44 35	3.7	1.6	05/11
20081+2720	20 10 11.5	+27 29 06	0.7		05/11, 05/23
20126+4104	20 14 26.0	+41 13 31	1.7		05/11
20205+3948	20 22 22.0	+39 58 05	4.5		05/11, 05/30
20216+4107	20 23 23.8	+41 17 40	1.7		05/11
20293+3952	20 31 10.7	+40 03 10	2.0	1.3	05/11
20319+3958	20 33 49.4	+40 08 45	1.6		05/11
20332+4124	20 35 00.5	+41 34 48	3.9		05/23
20343+4129	20 36 07.1	+41 40 01	1.4		05/23
22134+5834	22 15 09.1	+58 49 09	2.6		05/06
22551+6221	22 57 05.2	+62 37 44	0.7		05/06, 05/23
22570+5912	22 59 06.5	+59 28 28	5.1		05/06, 05/23
23033+5951	23 05 25.2	+60 08 11	3.5		05/06
23139+5939	23 16 09.3	+59 55 23	4.8		05/06
23151+5912	23 17 21.1	+59 28 49	5.7		05/06
23545+6508	23 57 05.2	+65 25 11	0.8		05/06, 05/23

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