Table 3: Observed line fluxes ( $W=\int T_{\rm MB}~ {\rm d}V$ in K km s-1), line widths ($\Delta V$ in km s-1) and opacities for the CN 3 $ 5\over 2$-2 $ 3\over 2$ transitions. The frequencies are given in GHz. Upper limits are at $3\sigma $ in line flux. Numbers in brackets are uncertainties in units of the the last decimal place. The line width was taken to be fixed with an estimated error of $\lesssim $30%.
Source 340.035     340.031     340.019     340.008    
  W $\Delta V$ $\tau$ W $\Delta V$ $\tau$ W $\Delta V$ $\tau$ W $\Delta V$ $\tau$
AFGL 2591 7.71(14) 2.7 0.27(3) 8.39(14) 2.7 0.29(3) 1.40(13) 2.7 0.05(1) 1.49(20) 2.7 0.05(1)
W3 IRS 5 8.34(22) 3.1 0.25(5) 9.04(22) 3.1 0.27(5) 1.52(20) 3.1 0.05(1) 1.36(20) 3.1 0.04(1)
IRAS 16293 1.14(7) 1.2 0.52(5) 0.92(6) 1.0 0.53(5) 0.12(5) 1.0 0.10(1) <0.06 ... ...
N1333-I2 0.61(4) 1.0 0.06(1) 0.59(4) 1.0 0.06(1) 0.16(4) 0.8 0.02(1) <0.10 ... ...
N1333-I4A 0.38(4) 1.2 0.09(1) 0.31(4) 0.9 0.08(1) <0.09 ... ... <0.09 ... ...
L1448-C 0.46(2) 1.1 0.12(1) 0.45(2) 1.1 0.12(1) 0.06(2) 1.1 0.02(<1) 0.06(2) 1.1 0.01(<1)
L483 1.21(10) 1.3 0.09(1) 1.28(10) 1.3 0.09(1) 0.19(10) 1.2 0.01 0.20(10) 1.0 0.02(<1)
L723 0.36(3) 1.4 0.03(<1) 0.40(3) 1.3 0.03(<1) <0.06 ... ... <0.06 ... ...
SMM4 1.36(4) 3.0 0.05(2) 0.98(4) 2.5 0.05(2) 0.22(5) 2.2 0.01(<1) 0.16(4) 2.0 0.01(<1)
V1057 Cyg 0.29(3) 1.1 0.11(2) 0.31(3) 1.2 0.11(2) <0.07 ... ... <0.07 ... ...
L1489 0.28(5) 1.1 0.01(<1) 0.21(5) 1.1 0.01(<1) <0.07 ... ... <0.07 ... ...


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