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Table A.2

C3O.

Source Trans. ν (a) Eup (a) log (Aup /s−1) (a) Telescope HPBW Det. rms Tmb FWHM Iint VLSR Refs.
NJ (MHz) (K) (′′) (mK) (mK) (km s−1) (mK km s−1) (km s−1)

C3O
TMC-1 2–1 19 243.5 1 –6.72 Green Bank-140 ft 90 Y 5 1, 2
5–4 48 108.5 7 –5.47 Nobeyama 39 Y 23 2
8–7 76 972.6 17 –4.85 Kitt Peak 82 Y 21 2
9–8 86 593.7 21 –4.69 Kitt Peak 82 Y 15 2
9–8 86 593.7 21 –4.69 FCRAO (b) 60 Y 7 2
L1544 8–7 76 972.6 20.8 –4.84 IRAM-ASAI 33 Y 3.0 41.8 ± 2.9 0.43 ± 0.03 19.05 ± 2.65 7.14 ± 0.01 5
9–8 86 593.7 20.8 –4.69 IRAM-ASAI 29 Y 2.6 35.2 ± 2.4 0.43 ± 0.03 16.04 ± 2.21 7.10 ± 0.01 3, 5
10–9 96 214.7 25.4 –4.55 IRAM-ASAI 26 Y 3.1 20.3 ± 3.1 0.34 ± 0.06 7.32 ± 2.41 7.16 ± 0.02 5
11–10 105 835.4 30.5 –4.42 IRAM-ASAI 24 N 4.3 5
12–11 115 455.9 36.0 –4.31 IRAM-ASAI 22 N 17.9 5
L1498 4–3 38 486.9 5 –5.77 IRA-Noto 54 Y 3.8 12.7 ± 3.5 1.08 ± 0.10 17.03 ± 4.00 7.17 ± 0.50 5
9–8 86 593.7 21 –4.69 IRAM 28 Y 2.6 14.3 ± 2.5 0.45 ± 0.07 6.87 ± 1.18 7.88 ± 0.03 5
11–10 105 835.4 30.5 –4.42 IRAM 24 N 4.4 5
Elias 18 4–3 38 486.9 5 –5.77 IRA-Noto 54 Y 7 4
9–8 86 593.7 21 –4.69 IRAM 28 Y 2.9 15.9 ± 2.5 0.54 ± 0.01 9.12 ± 1.18 6.02 ± 0.03 5
11–10 105 835.4 30.5 –4.42 IRAM 24 N 4.6 5
IRAS 16293-2422 9–8 86 593.7 21 –4.69 IRAM-TIMASSS 28 N 5 5
L1157-mm 9–8 86 593.7 21 –4.69 IRAM-ASAI 28 N 3 5
L1157-B1 9–8 86 593.7 21 –4.69 IRAM-ASAI 28 N 3 5
SVS13A 9–8 86 593.7 21 –4.69 IRAM-ASAI 28 N 3 5
OMC-2 FIR4 9–8 86 593.7 21 –4.69 IRAM-ASAI 28 N 3 5
IRAS 4A 9–8 86 593.7 21 –4.69 IRAM-ASAI 28 N 3 5

Notes. (a) C3O frequencies and spectroscopic parameters were extracted from the Cologne Database for Molecular Spectroscopy (CDMS; Müller et al. 2001, 2005). (b) FCRAO is the acronym for Five Colleges Radio Astronomy Observatory, Quabbin, Massachusetts. (†) Details of the detection are given in the reference reported in the last column. For the observations towards L1544, the rms on a 50 kHz frequency bin was computed over a range of 15 km s−1. The error in the main-beam temperature Tmb and Iint does not include the 10% calibration accuracy for the IRAM 30 m telescope. Bands with a Tmb value equal to 3σ rms are considered tentative detections, while we attribute the detected status to those bands with a Tmb ≥ 4σ rms.

References.(1) Matthews et al. (1984); (2) Brown et al. (1985); (3) Vastel et al. (2014); (4) Palumbo et al. (2008); (5) this work.

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