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Table 1

CS line parameters in IRC +10216.

Transition ν rest ν obs v exp Notes
(MHz) (MHz) K km s-1 km s-1

CS
v=0 J=2-1 97980.952 97980.8(1) 117(3) 13.8(2)
v=0 J=3-2 146969.025 146968.6(2) 267(6) 13.8(3)
v=0 J=4-3 195954.213 195953.7(4) 286(8) 13.3(3)
v=0 J=5-4 244935.554 244935.1(3) 308(8) 12.5(4)
v=0 J=6-5 293912.089 293911.7(3) 423(10) 12.6(4)
v=0 J=7-6 342882.854 342881.8(3) 259(8) 12.3(4)
v=1 J=2-1 97270.997 97271.5(5) 0.11(2) 6.1(6) $ ! 
v=1 J=3-2 145904.089 145903.8(3) 1.05(5) 5.4(4)
v=1 J=5-4 243160.648 243161.1(5) 1.38(7) 6.6(3) $
v=1 J=6-5 291782.190 291782.2(5) 3.0(1) 11.8(8)
v=1 J=7-6 340397.957 340398.3(5) 1.74(8) 10.4(6)
v=2 J=6-5 289651.545 289651.9(5) 0.60(5) 5.8(6)
v=2 J=7-6 337912.189 337912.9(6) 0.34(3) 4.8(6)
v=3 J=5-4 239608.923 239610.1(5) 0.07(1) 3.3(2)
v=3 J=6-5 287520.096 287521.1(8) 0.28(2) 7.1(5)
v=3 J=7-6 335425.481 335425.8(8) 0.14(2) 3.4(5)

13CS
v=0 J=2-1 92494.273 92494.2(2) 4.1(2) 14.2(8) $
v=0 J=3-2 138739.267 138739.1(2) 10.7(5) 14.1(4) $
v=0 J=5-4 231220.689 231220.6(2) 16.8(8) 14.2(3)
v=0 J=6-5 277455.403 277456.2(6) 22.6(10) 14.5(6)
v=0 J=7-6 323684.976 323686.3(10) 12.5(8) 14.4(8)
v=1 J=5-4 229592.986 229593.0(6) 0.05(1) 2.5(2)

C34S
v=0 J=2-1 96412.956 96412.9(2) 10.1(4) 14.3(3)
v=0 J=3-2 144617.107 144617.0(1) 21.5(5) 13.8(2)
v=0 J=5-4 241016.098 241016.1(1) 39.4(8) 14.4(2)
v=0 J=6-5 289209.077 289208.9(5) 40(1) 13.7(4)
v=0 J=7-6 337396.471 337396.1(5) 24.2(8) 14.0(4)
v=1 J=3-2 143577.671 143576.9(10) 0.04(1) 6.9(10)  ! 
v=1 J=6-5 287130.180 287131.1(5) 0.18(2) 4.9(7)

C33S
v=0 J=2-1 97172.063 97171.6(5) 1.71(8) 15.1(7) $
v=0 J=3-2 145755.730 145755.6(4) 4.9(2) 14.4(7) $
v=0 J=5-4 242913.608 242913.7(2) 8.3(1) 14.4(4)
v=0 J=6-5 291485.927 291485.9(6) 10.0(3) 14.2(6) $
v=0 J=7-6 340052.572 340052.8(8) 6.1(2) 13.6(8) $

Notes. Numbers in parentheses are 1σ errors in units of the last digits. Observed frequencies νobs were derived adopting a systemic velocity vLSR for IRC +10216 of − 26.5 km s-1 (Cernicharo et al. 2000). ∥ Line width parameter vexp has been fixed.$ Blended with another line. An individual fit for each line is possible.? Two transitions are very close in frequency. A single line is fitted. ! Marginal detection.♠ Clear or probable maser line.∞ Complex line profile. Line fit is not particularly good.

Notes. Numbers in parentheses are 1σ errors in units of the last digits. Observed frequencies νobs were derived adopting a systemic velocity vLSR for IRC +10216 of − 26.5 km s-1 (Cernicharo et al. 2000).

 ∥ Line width parameter vexp has been fixed.

$ Blended with another line. An individual fit for each line is possible.

? Two transitions are very close in frequency. A single line is fitted.

 ! Marginal detection.

♠ Clear or probable maser line.

∞ Complex line profile. Line fit is not particularly good.

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