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Table 3

Transition properties from the Cologne Database for Molecular Spectroscopy (CDMS) (Endres et al. 2016).

Species Transition Frequency Eup Aij Sources
(MHz) (K) (s−1)
HNCO (1) 100,10–90,9 219 798.27 58.0 1.47 × 10−4 G24
HNCO (2) 101,9–91,8 220 584.75 101.5 1.45 × 10−4 G17, G345
HNCO (3) 103,7–93,6 219 656.77 432.9 1.20 × 10−4 G24, G345
NH2CHO (1) 101,9–91,8 218 459.21 60.8 7.47 × 10−4 G17, G345
NH2CHO (2) 112,10–102,9 232 273.64 78.9 8.81 × 10−4 G24
H2CO (1) 30,3–20,2 218 222.19 20.9 2.82 × 10−4 G17, G24, G345
H2CO (2) 32,2–22,1 218 475.63 68.1 1.57 × 10−4 G17, G24, G345
H2CO (3) 32,1–22,0 218 760.07 68.1 1.58 × 10−4 G17, G24, G345

Notes. The last column shows the sources in which this transition appeared. HNCO (3) has a much higher upper energy level than the other transitions, so we consider it cautiously. The CDMS catalog can be accessed here: https://cdms.astro.uni-koeln.de/

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