Table 3: Sample table of source parameters.
224mmField Namea RA Dec rms Id.b $V_{\rm {LSR}}$ $T^*_{\rm {R}}$ FWHM $\int T_{\rm {R}} {\rm d}V$ Profile type RGC Near Far Notes
  (J2000) (J2000) (K)   km s-1 (T) (km s-1) (km s-1 K)   (kpc) (kpc) (kpc)  
G300.1615-00.0877 12:27:08.2 -62:49:44 0.07 1 -39.4 2.9 2.4 7.4   7.1 4.1 (0.72)  
G300.3412-00.2190 12:28:36.0 -62:58:33 0.10 1 $^\star$ -38.5 6.7 2.0 14.2 Blue shoulder 7.1 4.2 (0.84) 1
        2 34.6 1.3 4.2 5.8   10.6 12.0 (0.99)  
G300.5320-01.7926 12:29:04.3 -64:33:37 0.07 1 -0.9 0.3 1.0 0.3   8.6 8.8 (0.91)  
G300.7027+03.0398 12:33:44.9 -59:45:19 0.08 $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$  
G300.7221+01.2007 12:32:50.9 -61:35:29 0.11 1 -43.0 9.6 2.2 22.4 Blue shoulder 7.0 4.1 (0.19)  
G300.9785+01.1459 12:34:58.1 -61:39:48 0.10 1 -43.7 6.4 3.3 22.4 Red asymmetry top 6.9 4.2 (0.19)  
G301.0130+01.1153 12:35:14.6 -61:41:46 0.10 1 -43.1 6.1 3.3 21.3 Red shoulder 7.0 4.2 (0.36)  
G301.1067-01.4919 12:34:35.5 -64:18:15 0.09 $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$  
G301.1175+00.9627 12:36:02.6 -61:51:17 0.20 1 -41.6 6.7 4.7 33.4 Red shoulder 7.0 4.2 (0.66)  
G301.1726+01.0034 12:36:31.9 -61:49:03 0.10 1 -40.6 5.4 3.8 21.8 Red shoulder 7.0 4.3 (0.78)  
G301.5309-00.8231 12:38:48.2 -63:39:38 0.07 1 -5.1 3.4 0.7 2.5   8.4 0.2 (0.93) 8.7 (0.91)  
G301.8147+00.7808 12:41:53.8 -62:04:13 0.07 1 -37.4 9.3 2.1 20.7 Blue shoulder 7.1 4.4 (1.11)  
G302.0213+00.2542 12:43:31.2 -62:36:13 0.08 1 $^\star$ -46.1 4.0 2.9 12.3   6.9 4.3 (0.19) 1
        2 -37.7 3.1 1.2 3.9 Blue shoulder 7.1 4.5 (1.11)  
G302.4546-00.7401 12:47:08.6 -63:36:29 0.07 1 30.4 0.5 3.1 1.6 Blended 10.4 12.1 (0.97)  
        2 $^\star$ 35.3 1.3 3.2 4.4 Blended 10.7 12.6 (1.00) 1
G302.4867-00.0308 12:47:31.7 -62:53:57 0.10 1 $^\star$ -37.1 4.4 3.1 14.5 Blended (main component) 7.1 4.5 (1.19) 4
        2 -34.2 2.6 2.1 5.8 Blended (red shoulder) 7.2 3.6 (1.17) 5.6 (1.34)  
        3 -29.1 0.9 4.0 3.8   7.4 2.7 (1.50) 6.5 (1.56)  
G302.5005-00.7701 12:47:33.1 -63:38:19 0.10 1 30.0 2.6 3.2 8.8 Red shoulder 10.4 12.1 (0.96)  
G302.6604-00.7908 12:48:59.5 -63:39:41 0.10 1 23.1 0.7 3.4 2.5 Blended 9.9 11.4 (0.92)  
        2 $^\star$ 26.4 1.3 2.1 2.9 Blended 10.1 11.8 (0.94) 1
G303.5353-00.5982 12:56:50.4 -63:27:49 0.10 1 $^\star$ 18.9 3.3 2.3 8.0   9.7 11.3 (0.90) 1
        2 31.6 0.9 4.1 3.9   10.5 12.5 (0.98)  
G303.5990-00.6524 12:57:25.2 -63:30:59 0.08 1 -2.3 1.6 0.4 0.7   8.5 9.4 (0.87)  
        2 $^\star$ 19.1 1.8 2.5 4.8   9.7 11.3 (0.90) 1
G303.9973+00.2800 13:00:41.5 -62:34:22 0.10 1 -45.1 1.1 2.3 2.7 Blended 6.9 4.6 (0.87)  
        2 -42.3 2.2 2.4 5.6 Blended 6.9 4.7 (1.06)  
        3 -28.9 0.4 4.4 1.9   7.4 2.5 (1.47) 7.0 (1.47)  
        4 30.7 2.4 2.5 6.4   10.5 12.5 (0.97)  
G304.5719+00.7163 13:05:28.1 -62:06:39 0.10 $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$ $\cdots$  
G304.7700-00.5193 13:07:49.9 -63:19:58 0.11 1 24.6 1.7 1.9 3.4   10.0 12.1 (0.94)  
a Observations made with the JCMT and Onsala telescope are indicated by $\dag $ and $\ddag $ respectively.
b Where multiple components have been detected we identify the most likely component associated with the RMS source by an $\star$.
Notes: (1) strongest component; (2) methanol maser; (3) water maser; (4) and (5) CS detection by Bronfman et al. (1996) and Fontani et al. (2005).

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