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Table 2

Millimeter interferometric observations presented in this paper.

Name Frequency Eup log10Aul Beam (a) Noise Int. time Integrated flux density
(GHz) (K) (s−1) (″ ×″, °) (mJy bm−1) (min) (mJy/mJy km s−1)
NOEMA continuum 203 ... ... 0.78 × 0.72, 62 1.1 180 210 ± 20
NOEMA continuum 220 ... ... 0.79 × 0.61, 54 1.2 180 170 ± 17
ALMA continuum 220 ... ... 0.031 × 0.020, −3 0.08 170 220 ± 22
ALMA continuum 230 ... ... 0.032 × 0.021, 1 0.05 111 240 ± 24
ALMA continuum 240 ... ... 0.028 × 0.018, 0 0.08 90 280 ± 28
ALMA continuum 260 ... ... 0.049 × 0.032, 11 0.05 63 190 ± 19
HO 31,3−22,0 203.4075 203.7 − 5.32 0.78 × 0.72, 59 8 180 <11
DCN 3–2 217.2385 20.85 − 3.34 0.13 × 0.10, 32 1.5 91 <8
C18O 2–1 219.5604 15.80 − 6.22 0.13 × 0.10, 31 1.8 91 330 ± 33
13CO 2–1 220.3987 15.87 − 6.22 0.13 × 0.10, 32 2.4 85 290 ± 30
12CO 2–1 230.5380 16.60 − 6.16 0.12 × 0.10, 0.5 2.5 83 1740 ± 174
N2D+ J = 3−2 231.3216 22.20 − 2.67 0.12 × 0.10, 32 0.8 91 100 ± 22
SO N = 65−54 251.8258 50.66 − 3.71 0.13 × 0.11, 0.1 1.0 71 460 ± 46
HCN v2 = 1 J = 3−2e 265.8527 1050 − 2.64 0.092 × 0.07, 0.4 0.9 71 <20
HCN 3−2 265.8862 25.52 − 3.55 0.12 × 0.10, 0.1 1.3 71 160 ± 20
HCN v2 = 1 J = 3−2f 267.1993 1050 − 2.63 0.092 × 0.07, 20 0.9 71 <20
HCO+ J = 3−2 267.5576 25.68 − 2.84 0.12 × 0.11, 3.5 1.2 71 640 ± 64

Notes. Synthesized beams and noise levels of the images are listed below. Upper limits are calculated over the size of the dust continuum emission. We report the noise to be 10% of the integrated flux density unless the measured noise is larger than 10%. The noise level for the molecular line observations is per velocity channel (0.3 km s−1). (a) Elliptical synthesized beam parametrized by the full-width half-maximum (FWHM) of the major axis × the FWHM of the minor axis, and a position angle.

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