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Table 1.

Transitions identified as HOCHCHCHO towards IRAS 16293 B.

Transition Frequency Uncertainty Eup Aij gup
(MHz) (MHz) (K) (s−1)
17 17 0 1 – 16 16 1 1 329184.2911 0.0223 171.1 1.30 × 10−3 35
17 17 1 1 – 16 16 0 1 329184.2911 0.0223 171.1 1.29 × 10−3 105
21 14 7 0 – 20 13 8 0 330826.2042 0.0188 148.7 8.32 × 10−4 129
21 14 8 0 – 20 13 7 0 330826.5149 0.0188 148.7 8.32 × 10−4 43
20 15 5 0 – 19 14 6 0 ( † ) 333154.5692 0.0155 147.3 9.76 × 10−4 41
20 15 6 0 – 19 14 5 0 ( † ) 333154.5726 0.0155 147.3 9.76 × 10−4 123
19 16 3 0 – 18 15 4 0 335375.7805 0.0154 146.9 1.14 × 10−3 117
19 16 4 0 – 18 15 3 0 335375.7805 0.0154 146.9 1.14 × 10−3 39
19 16 3 1 – 18 15 4 1 335563.7519 0.0154 177.9 1.12 × 10−3 39
19 16 4 1 – 18 15 3 1 335563.7519 0.0154 177.9 1.12 × 10−3 117
25 12 13 0 – 24 11 14 0 ( † ) 341865.3358 0.0411 176.0 5.78 × 10−4 153
20 16 4 1 – 19 15 5 1 344235.8096 0.0157 186.3 1.14 × 10−3 123
20 16 5 1 – 19 15 4 1 344235.8096 0.0157 186.3 1.14 × 10−3 41
24 14 10 1 – 23 13 11 1 ( † ) 356301.7349 0.0304 208.6 8.58 × 10−4 147
19 18 1 1 – 18 17 2 1 357554.8901 0.0231 195.8 1.56 × 10−3 39
19 18 2 1 – 18 17 1 1 357554.8901 0.0231 195.8 1.56 × 10−3 117
22 16 7 1 – 21 15 6 1 361541.5437 0.0191 204.3 1.18 × 10−3 45
22 16 6 1 – 21 15 7 1 361541.5438 0.0191 204.3 1.18 × 10−3 135
29 12 18 1 – 28 11 17 1 ( † ) 362238.2039 0.0768 253.7 4.87 × 10−4 177

Notes. ( † )The best-fit model only reproduces half of the line fluxes. These lines could consequently be partially blended with unknown species.

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