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Table 1

30 m/PdBI lines.

Line Freq. 30 m flux1 PdBI flux2 PdBI/30 m
(MHz) (Jy × km s-1) Flux (Jy/beam × km s-1)

O13CS 18 17 218 199 1.07 (0.40) 0.63 (0.04) ~60%
H2CO 30,3 20,2 218 222 41.11 (1.13) 4.51 (0.19) ~10%
HC3N 24 23 218 325 2.40 (0.38) 1.84 (0.34) ~100%
CH3OH 42,0 31,0 218 440 12.54 (0.49) 2.80 (0.03) ~20%
H2CO 32,2 22,1 218 476 10.80 (0.42) 3.26 (0.56) ~30%
H2CO 32,1 22,0 218 760 10.54 (0.42) 2.98 (0.11) ~30%
OCS 18 17 218 903 3.11 (0.44) 3.29 (0.05) ~100%
C18O 2 1 219 560 32.85 (0.20) 2.47 (0.10) <10%
HNCO 103,83,7* 219 657 <1.13 1.04 (0.11) ~100%
103,73,6*
HNCO 102,9 92,8* 219 734 1.91 (0.53) 2.13 (0.12) ~100%
102,8 92,7* 219 737
HNCO 100,10 90,9 219 798 3.14 (0.42) 2.12 (0.12) ~70%
H213CO 31,2 21,1 219 909 1.96 (0.37) 1.18 (0.11) ~60%
SO 56 45 219 949 43.20 (2.75) 8.65 (0.21) ~20%
E-CH3OH 80 71 220 078 3.59 (0.95) 3.95 (0.14) ~100%
13CO 2 1 220 399 144.49 (1.67) 5.54 (0.13) <1%
CH3CN 125 115 220 641 2.18 (0.64) 2.50 (0.13) ~100%
CH3CN 124 114 220 679 2.00 (0.25) 2.20 (0.08) ~100%
CH3CN 123 113 220 709 1.68 (0.65) 2.16 (0.70) ~100%
CH3CN 122 112 220 730 2.07 (0.58) 2.05 (0.46) ~100%
CH3CN 120 110* 220 747 5.14 (0.71) 4.05 (0.52) ~100%
121 111* 220 743 ~100%

Notes. Comparison between the flux measured with the 30 m and PdB telescopes for all the lines detected with the 30 m single-dish telescope.

(1)

Velocity-integrated flux density in the 30 m spectrum.

(2)

Velocity-integrated flux density towards the emission peak.

(*)

Blended lines.

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