Open Access

Table A.1

Lines of H2S, OCS, and their isotopologs towards the targeted sources. The columns show 1) the CDMS entry, 2) the quantum numbers associated to the transition, 3) the rest frequency of the line, 4) the upper energy level of the transition, 5) the Einstein A coefficient of the transition, and the line evaluation done for different protostars given in columns 6-14.

Species CDMS entry Transition Freq. (GHz) Eup (K) Aij (s−1) IRAS 16293 A IRAS 16293 B IRAS4A IRS7B B1-c BHR71-IRS1 Emb25 IRAS4B SMM3 TMC1
H2S 46519 22,0-21,1 216.710 84 4.9×10−5
H233S 35503 22,0,1 - 21,1,2 215.494 84 2.4×10−5 _ _ _
22,0,1 - 21,1,1 215.497 84 2.4×10−5
22,0,4 - 21,1,3 215.501 84 6.9×10−6
22,0,4 - 21,1,4 215.503 84 4.l×10−5
22,0,2 - 21,1,3 215.504 84 l.7×10−5
22,0,2 - 21,1,2 215.505 84 l.9×10−5
22,0,2 - 21,1,1 215.508 84 l.2×10−5
22,0,3 - 21,1,3 215.512 84 2.8×10−5
22,0,3 - 21,1,2 215.513 84 1.1×10−5
22,0,3 - 21,1,4 215.513 84 9.1×10−6
H234S 36504 22,0 - 21,1 214.377 84 4.7×10−5
HDS 35502 73,4 - 73,5 234.046 417 6.6×10−6 _
125,7 - 125,8 234.528 1148 6.3×10−6
142,12-134,9 214.325 1277 5.O×10−8
HD34S 37503 73,4-73,5 232.964 416 6.5×10−6 _ _
125,7-125,8 233.088 1145 6.2×10−6
OC33S 61503 18-17 216.147 99 2.9×10−5
O13CS 61502 19-18 230.318 110 3.5×10−5
18OCS 62506 19-18 216.753 104 2.9×10−5
OCS, υ = 0 60503 19-18 231.061 111 3.6×10−5
OCS, υ2 = l 60504 19-18 231.342 860 3.5×10−5
OCS, υ2 = 1+ 19-18 231.584 860 3.5×10−5
18OC34S 64511 21-20 233.479 123 3.7×10−5
18O13CS 63503 19-18 216.229 104 2.9×10−5

Note: ✓represents detected lines, ×represents undetected lines and – represents unobserved lines (i.e., not covered in the spectral windows observed for that source).

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