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 |
| H |
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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