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Table 2

Molecular lines and frequencies.

Molecule J + 1 → J Eu/kB Frequency n crit a Bandwidth Resolution Beam B eff F eff 1σ rms
(K) (GHz) (cm-3) (MHz) (km s-1) (′′) (K)

IRAM 30 m telescope
H13CO+ 1–0 4.16   86.754   1.7 × 105 160 0.16 29 0.78 0.98 0.06
SiO 2–1 6.25   86.847   7.3 × 105 160 0.16 29 0.78 0.98 0.07
HCO+ 1–0 4.28   89.189   1.8 × 105 40 0.08 28 0.78 0.98 0.10
CH3CN 5–4, K = 0, 1, 2, 3, 4 13.24b 91.987b 4.7 × 105 120 0.16 27 0.78 0.98 0.09
N2H+ 1–0 4.47   93.174   1.6 × 105 40 0.08 27 0.78 0.98 0.11
C18O 2–1 15.81   219.560   9.2 × 103 512 1.5 12 0.62 0.94 0.12
CO 2–1 16.60   230.538   1.1 × 104 512 1.5 11 0.58 0.92 1.3
APEX telescope
N2H+ 3–2 26.83   279.512   3.0 × 106 1000 0.15 22 0.73 0.97 0.23
H2CO 404–303c 34.90   290.623   9.2 × 106 1000 0.15 22 0.73 0.97 0.20
HCO+ 4–3 42.80   356.734   9.1 × 106 1000 0.12 18 0.73 0.97 0.47
CO 3–2 33.19   345.796   3.5 × 104 1000 0.12 18 0.73 0.97 1.1

Notes. Columns are (from left to right) the molecule, its transition, its upper energy level, its frequency, its critical column density, the bandwidth used in the observation, the velocity resolution of the observation, the telescope beam, the main beam and forward beam efficiency of the observation, and the mean 1σ noise value. .

(a)

Calculated from the collision rates at T = 20 K from the LAMBDA molecular database (Schöier et al. 2005).

(b)

Frequency and Eu/kB for the K = 0 level. Observed were K = 0, 1, 2, 3, 4

(c)

The observed K level is given in subscript.

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