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. Author manuscript; available in PMC: 2021 Jul 29.
Published in final edited form as: Astron Astrophys. 2021 May 5;649:L4. doi: 10.1051/0004-6361/202140978

Table 1. Observed line parameters of the target O-bearing COMs of this study in TMC-1.

Molecule Transition Eup (K) v calc (MHz) T*A peak (mK) va (km s) VLSR (km s−1) T*Adv (mK km s−1) S/N b (σ) B eff/F eff c
trans-C2H3CHO 41,4-31,3 6.2 34768.987 3.06 ± 0.31 0.62 ± 0.08 5.77 ± 0.03 2.03 ± 0.21 14.5 0.603
40,4-30,3 4.3 35578.136 3.77 ± 0.33 0.81 ± 0.08 5.79 ± 0.03 3.27 ± 0.27 19.4 0.597
41,3 −31,2 6.4 36435.990 3.17 ± 0.29 0.85 ± 0.09 5.73 ± 0.04 2.87 ± 0.25 19.2 0.590
51,5-41,4 8.3 43455.469 1.81 ± 0.49 0.72 ± 0.27 5.78 ± 0.08 1.38 ± 0.37 6.5 0.530
50,5-40,4 6.4 44449.749 3.67 ± 0.54 0.54 ± 0.08 5.80 ± 0.04 2.11 ± 0.31 10.5 0.521
51,4-41,3 8.6 45538.994 4.72 ± 0.66 0.69 ± 0.09 5.80 ± 0.04 3.45 ± 0.43 12.6 0.511
syn-C2H3OH 40,4-31,3 9.3 32449.221 1.17 ± 0.32 1.07 ± 0.21 5.61 ± 0.11 1.34 ± 0.27 6.8 0.622
21,2-11,1 5.1 37459.184 d 0.581
20,2-10,1 2.8 39016.387 1.90 ± 0.39 0.89 ± 0.16 5.81 ± 0.07 1.79 ± 0.29 9.0 0.568
21,1-11,0 5.3 40650.606 1.71 ± 0.41 0.65 ± 0.19 5.88 ± 0.08 1.18 ± 0.28 6.7 0.554
HCOOCH3 31,3-21,2 E 4.0 34156.889 1.92 ± 0.29 0.62 ± 0.12 5.93 ± 0.06 1.27 ± 0.23 9.6 0.608
31,3-21,2 A 3.9 34158.061 1.86 ± 0.29 0.80 ± 0.16 5.84 ± 0.07 1.59 ± 0.28 10.6 0.608
30,3-20,2 E 3.5 36102.227e 0.593
30,3-20,2 A 3.5 36104.775 2.61 ± 0.29 0.74 ± 0.09 5.80 ± 0.04 2.05 ± 0.22 14.6 0.592
31,2-21,1 E 4.4 38976.085 1.81 ± 0.35 0.66 ± 0.14 5.93 ± 0.07 1.28 ± 0.25 8.3 0.568
31,2-21,1 A 4.4 38980.803 2.45 ± 0.35 0.57 ± 0.09 5.92 ± 0.04 1.49 ± 0.21 10.4 0.568
41,4-31,3 E 6.1 45395.802 2.82 ± 0.57 0.63 ± 0.18 6.00 ± 0.07 1.89 ± 0.40 8.3 0.512
41,4-31,3 A 6.1 45397.360 2.39 ± 0.57 0.42 ± 0.19 5.91 ± 0.10 1.07 ± 0.32 5.8 0.512
40,4-30,3 E 5.8 47534.116 3.19 ± 0.75 0.59 ± 0.12 5.92 ± 0.07 2.01 ± 0.44 7.1 0.493
40,4-30,3 A 5.8 47536.905 2.76 ± 0.75 0.98 ± 0.23 5.99 ± 0.10 2.88 ± 0.60 7.9 0.493
CH3OCH3 21,1 −20,2 AE + EA 4.2 31105.223 1.35 ± 0.39 0.92 ± 0.25 5.72 ± 0.13 1.31 ± 0.36 5.8 0.632
21,1-20,2 EE 4.2 31106.150 1.52 ± 0.39 0.54 ± 0.34 5.94 ± 0.08 0.87 ± 0.29 5.0 0.632
31,2-30,3 AE + EA 7.0 32977.276 1.37 ± 0.25 0.63 ± 0.13 5.84 ± 0.07 0.91 ± 0.19 7.8 0.618
31,2-30,3 EE 7.0 32978.232 1.37 ± 0.25 0.95 ± 0.23 5.84 ± 0.09 1.38 ± 0.27 9.6 0.618
31.2-30,3 AA 7.0 32979.187 1.06 ± 0.25 0.85 ± 0.32 5.99 ± 0.12 0.96 ± 0.29 7.1 0.618
41.3-40,4 EE 10.8 35593.408 1.22 ± 0.27 0.56 ± 0.13 5.82 ± 0.07 0.73 ± 0.16 6.4 0.597
11,1-00,0 EE 2.3 47674.967 3.31 ± 0.62 0.59 ± 0.12 6.02 ± 0.06 2.08 ± 0.38 8.9 0.492

The line parameters T*A peak, Δv, VLSR, and ∫ T*Adv and the associated errors are derived from a Gaussian fit to each line profile.

a

Δv is the full width at half maximum (FWHM).

b

Signal-to-noise ratio is computed as S/N = ∫T*Adv / [rms × -Δv×δv(c/vcalc), where c is the speed of light, δv is the spectral resolution (0.03815 MHz), the rms is given in the uncertainty of T*A peak, and the rest of parameters are given in the table.

c

Beff is given by the Ruze formula B eff = 0.738 exp [™(v/72.2)2], where v is the frequency in GHz, and F eff = 0.97.

d

Line overlaps with a hyperfine component of CH2CCH (see Agúndez et al. 2021).

e

Line detected but not fitted because it overlaps with a negative frequency-switching artifact.