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Table 2

Targeted transitions and beam sizes, beam coupling efficiencies, and spectral resolution of our IRAM 30 m, APEX SEPIA, and ALMA Band 6 observations.

Transition Frequency Eu Telescope Beff Δv FWHM
(MHz) (K) (km s−1) (″)
H2CO
30,3 − 20,2 218222.192 10.5 IRAM 0.62 0.26 11
32,1 − 22,0 218760.066 57.6 IRAM 0.62 0.26 11
32,2 − 22,1 218475.632 57.6 IRAM 0.62 0.26 11
HCO
30,3 − 20,2 212811.184 10.2 ALMA 0.75 0.09 5 – 8
31,2 − 21,1 219908.525 22.4 IRAM 0.62 0.26 11
31,3 − 21,2 206131.626 21.7 APEX 0.72 0.06 30
HDCO
30,3 − 20,2 192893.256 9.3 APEX 0.72 0.06 32
31,3 − 21,2 185307.113 16.9 APEX 0.72 0.06 34
32,1 − 22,0 193907.460 41.1 APEX 0.72 0.06 32
32,2 − 22,1 193391.605 41.1 APEX 0.72 0.06 32
D2CO
30,3 − 20,2 174413.115 8.4 APEX 0.72 0.07 36

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