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. Author manuscript; available in PMC: 2020 Nov 9.
Published in final edited form as: Astron Astrophys. 2020 Sep 23;641:L9. doi: 10.1051/0004-6361/202039231

Table 2. Observed line parameters for C5N in TMC-1.

Ju νaobs
(MHz)
νo b c
(kHz)
Δvc
(kms-1)
∫T*Advd
(mK kms-1)
T*A
(mK)
12 33332.572 1.7 0.75±0.08 5.0±0.2 6.2
13 36110.244 5.5 0.73±0.07 5.5±0.2 7.1
14 38887.893 -2.6 0.54±0.09 3.7±0.3 6.4
15 41665.548 7.1 0.50±0.16 2.4±0.41 4.6
16 44443.178 4.5 0.63±0.15 3.3±0.5 4.9
17 47220.754 -38.8 0.76±0.19 2.0±0.5 2.5
(a)

Observed frequencies for a vLSR of 5.83 km s−1. The uncertainty is 10 kHz for all lines except for J=17-16, for which it is 20 kHz.

(b)

Observed minus calculated frequencies.

(c)

Line width at half intensity derived by fitting a Gaussian line profile to the observed transitions.

(d)

Integrated line intensity.