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Table A.1

Lines detected in the ALMA-PILS spectrum of IRAS 16293−2422.

Species Q1 Q2 ν Aij Eu Fit?
GHz log10() K
H2CO 51,5 41,4 351.769 –2.9201 62.5
82,6 90,9 361.968 –5.9856 173.5
50,5 40,4 362.736 –2.8626 52.3
H2C17O 51,5 41,4 343.333 –2.9518 61.3
50,5 40,4 353.820 –2.8950 51.0
52,4 42,3 354.908 –2.9665 98.4
* 54,2 44,1 355.042 –3.3340 240.1
* 54,1 44,0 355.042 –3.3340 240.1
** 53,3 43,2 355.202 –3.0835 157.5
53,2 43,1 355.214 –3.0834 157.5
52,3 42,2 356.187 –2.9619 98.5
H2C18O 51,5 41,4 335.816 –2.9805 60.2
50,5 40,4 345.881 –2.9246 49.9
52,4 42,3 346.869 –2.9963 97.4
54,2 44,1 346.984 –3.3639 239.6
54,1 44,0 346.984 –3.3639 239.6
53,3 43,2 347.134 –3.1134 156.7
53,2 43,1 347.144 –3.1134 156.7
52,3 42,2 348.032 –2.9920 97.5
51,4 41,3 357.741 –2.8982 63.4
H213CO 51,5 41,4 343.326 –2.9517 61.3
50,5 40,4 353.812 –2.8949 51.0
52,4 42,3 354.899 –2.9664 98.4
54,2 44,1 355.029 –3.3339 240.1
54,1 44,0 355.029 –3.3339 240.1
* 121,11 121,12 355.042 –4.7277 285.4
53,3 43,2 355.191 –3.0835 157.5
** 53,2 43,1 355.203 –3.0834 157.5
52,3 42,2 356.176 –2.9618 98.5
HDCO 51,4 41,3 335.097 –2.9841 56.2
172,15 172,16 340.801 –4.5839 517.6
31,3 20,2 343.284 –5.2876 25.8
111,10 111,11 346.739 –4.6725 219.4
42,2 50,5 347.286 –6.1800 62.9
101,9 100,10 355.075 –5.2163 184.3
HDC18O 61,6 51,5 353.098 –2.9039 67.4
D2CO 61,6 51,5 330.674 –2.9892 61.1
60,6 50,5 342.522 –2.9331 58.1
152,13 152,14 345.075 –4.4700 370.5
62,5 52,4 349.631 –2.9553 80.4
65,2 55,1 351.196 –3.4129 193.7
65,1 55,0 351.196 –3.4129 193.7
64,3 54,2 351.487 –3.1522 145.2
64,2 54,1 351.492 –3.1522 145.2
63,4 53,3 351.894 –3.0204 107.6
63,3 53,2 352.244 –3.0192 107.6
62,4 52,3 357.871 –2.9248 81.2
D213CO 60,6 50,5 337.552 –2.9461 57.2
62,5 52,4 344.225 –2.9696 79.6
64,3 54,2 345.957 –3.1670 144.7
64,2 54,1 345.961 –3.1670 144.7
63,4 53,3 346.346 –3.0352 106.9
63,3 53,2 346.662 –3.0340 106.9
62,4 52,3 351.961 –2.9406 80.3
61,5 51,4 360.989 –2.8691 66.2

Notes. The stars in the left-most column indicates the lines that are blended with each other. The square in the right-most column identifies the lines used in constraining the column density (and for HDCO also the temperature).

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