Table A.1
Emission lines detected in ALMA Cycle 1 and 4 measurements towards HH212 mm.
Transition | ν a | Eup a | S μ2 a | rms | F int b |
(GHz) | (K) | (D2) | (K) | (K km s-1) | |
|
|||||
13CH3OH Cycle 1 | |||||
|
|||||
130,13–121,12A | 338.75995 | 206 | 13 | 0.29 | 9.6(1.1) |
134,9–143,11E | 347.78840 | 303 | 4 | 0.36 | 4.0(1.4) |
110,11–101,9E | 348.10019 | 162 | 5 | 0.84 | 7.5(3.0) |
11,1–00,0A | 350.10312 | 17 | 2 | 1.16 | 7.4(3.0) |
81,7–72,5E | 350.42158 | 103 | 2 | 0.93 | 8.7(2.6) |
|
|||||
CH2DOH Cycle 1 | |||||
|
|||||
90,9–81,8 e0 | 337.34866 | 96 | 6 | 0.15 | 15.3(0.5) |
91,8–82,6 o1c | 338.46254 | 120 | 2 | 0.26 | 10.7(2.1)c |
131,12–120,12 e0 | 338.86898 | 202 | 2 | 0.13 | 9.7(0.4) |
61,6–50,5 e0 | 338.95711 | 48 | 5 | 0.29 | 16.7(0.9) |
184,15–183,15 e1 | 347.76728 | 438 | 10 | 0.09 | 6.6(0.3) |
184,14–183,16 e1 | 347.95281 | 438 | 10 | 0.18 | 6.4(0.6) |
41,3–40,4 e1 | 348.16076 | 38 | 4 | 0.15 | 18.1(0.5) |
74,4–73,4 e1 | 349.95168 | 132 | 3 | 0.16 | 25.3(0.5) |
74,3–73,5 e1 | 349.95272 | 132 | 3 | ||
64,3–63,3 e1 | 350.02735 | 117 | 2 | 0.23 | 19.5(0.7) |
64,2–63,4 e1 | 350.02777 | 117 | 2 | ||
54,2–53,2 e1 | 350.09024 | 104 | 2 | 0.63 | 20.0(2.2) |
54,1–53,3 e1 | 350.09038 | 104 | 2 | ||
62,5–51,5 e1c | 350.45387 | 72 | 4 | 0.63 | 17.0(3.9)c |
51,4–50,5 e1 | 350.63207 | 49 | 5 | 0.60 | 21.0(2.0) |
|
|||||
13CH3OH Cycle 4 | |||||
|
|||||
121,11–120,12 A | 335.56021 | 193 | 23 | 0.81 | 61.7(2.7) |
|
|||||
CH2DOH Cycle 4 | |||||
|
|||||
162,15–161,15 o1d | 334.68395 | 327 | 8 | 0.67 | 51.1(2.9)d |
Notes.
Frequencies and spectroscopic parameters are extracted from the Jet Propulsion Laboratory molecular database (JPL, Pickett et al. 1998) and from the Cologne Database for Molecular Spectroscopy (CDMS, Müller et al. 2001). Upper level energies refer to the ground state of each symmetry.
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