Open Access

Table A.1

Molecular line properties and observational parameters of the PRODIGE-ANTIHEROES data.

Transition Rest-frequency
ν
(GHz)
Upper energy
Eu/kB
(K)
Einstein A coefficient
log Aul
(log s-1)
Channel width
δv
(km s-1)
IRAM 30m Beam
θmaj × θmin (PA)
(″×″(°))
Line noise
σline
(K)
Lower Upper velocity Missing
flux
(%)
Beam
θ
(″)
Line noise
σline,30m (mK)
vlow
(km s-1
vupp
NOEMA+IRAM 30m
c-C3H2 (33,0 - 22,1) 216.279 19.5 -3.6 0.1 12.0 99 1.28×0.92 (15) 0.34 3.0 7.0 98
DCN (3 - 2) 217.239 20.9 -3.3 0.1 11.9 100 1.28×0.92 (15) 0.35 1.0 10.0 57
c-C3H2 (60,6 - 51,5) 217.822 38.6 -3.3 0.1 11.9 93 1.27×0.92 (15) 0.35 3.0 7.0 85
c-C3H2 (51,4 - 42,3) 217.940 35.4 -3.4 0.1 11.9 96 1.27×0.91 (15) 0.35 3.0 7.0 88
C18O (2 - 1) 219.560 15.8 -6.2 0.1 11.8 101 1.26×0.91 (14) 0.34 1.0 11.0 93
SO(65 - 54) 219.949 35.0 -3.9 0.1 11.8 101 1.26×0.91 (14) 0.38 2.0 6.0 73
CO(2 - 1) 230.538 16.6 -6.2 0.1 11.2 99 1.22×0.85 (13) 0.38 ... ... 90
NOEMA
SO2 (42,2 - 31,3) 235.152 19.0 -4.1 0.1 11.0 106 1.16×0.81 (15) 0.39 2.0 6.0 ...

Notes. The transition properties (quantum numbers, ν, Eu/kB, and Aul) are taken from the Cologne Database for Molecular Spectroscopy (CDMS, Müller et al. 2005). The noise per channel in the line data, σline, is estimated in the central area of the mosaic as the standard deviation in line-free channels. The last two columns show the velocity ranges, vlow and vupp, used to compute the line-integrated intensity maps. The estimate of missing flux due to spatial filtering is calculated based on an integrated intensity comparison considering all areas with S/N >5 in the NOEMA and merged data.

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