Table A.1.
Line parameters for the lines of HCSCN and HCSCCH.
J Ka Kc | νobs(a) | δν(b) | ∫TA*dv(c) | Δv(d) | TA*(e) |
---|---|---|---|---|---|
MHz | kHz | (mK km s−1) | (km s−1) | (mK) | |
HCSCN | |||||
514 − 413 | 31386.932(10) | −6 | 3.46(25) | 1.10(09) | 2.96(27) |
616 − 515 | 36310.152(10) | 0 | 4.14(17) | 0.86(04) | 4.51(22) |
606 − 505 | 36958.682(10) | −2 | 7.70(20) | 0.75(02) | 9.63(27) |
615 − 514 | 37661.251(10) | 7 | 5.28(25) | 0.92(05) | 5.37(30) |
717 − 616 | 42357.921(10) | −8 | 4.41(26) | 0.77(05) | 5.37(31) |
707 − 606 | 43103.558(10) | 5 | 7.77(25) | 0.69(03) | 10.61(31) |
716 − 615 | 43933.874(10) | 0 | 4.79(24) | 0.69(04) | 6.50(28) |
818 − 717 | 48403.924(10) | 10 | 2.94(33) | 0.58(07) | 4.73(56) |
808 − 707 | 49241.600(10) | 8 | 6.61(38) | 0.68(04) | 9.06(64) |
817 − 716 | 50204.498(10) | −14 | 3.99(19) | 0.40(13) | 9.3(2.7) |
211 − 202 | |||||
F = 1 − 1 | 40166.115(20) | 23 | 0.42(13) | 0.63(22) | 0.63(27) |
F = 3 − 3 | 40166.591(20) | 21 | 1.34(14) | 0.71(11) | 1.78(27) |
F = 2 − 2 | 40167.426(20) | −5 | 0.82(12) | 0.67(11) | 1.14(27) |
312 − 303 | |||||
F = 2 − 2 | 40508.116(20) | −16 | 1.29(14) | 0.83(09) | 1.56(27) |
F = 4 − 4 | 40508.352(20) | 10 | 1.89(12) | 0.58(05) | 3.05(27) |
F = 3 − 3 | 40508.954(20) | 10 | 1.82(13) | 0.67(05) | 2.55(27) |
413 − 404 | |||||
F = 3 − 3 | 40967.200(20) | 16 | 0.85(14) | 0.48(09) | 1.68(28) |
F = 5 − 5 | 40967.313(20) | 0 | 1.67(17) | 0.57(07) | 2.75(28) |
F = 4 − 4 | 40967.798(20) | −13 | 1.30(17) | 0.86(13) | 1.41(28) |
514 − 505 | |||||
F = 4 − 4 | 41546.232(20) | 2 | 0.96(14) | 0.50(15) | 1.79(31) |
F = 6 − 6 | 41546.328(20) | 6 | 1.29(17) | 0.55(08) | 2.20(31) |
F = 5 − 5 | 41546.769(20) | −1 | 1.32(17) | 0.52(08) | 2.40(31) |
615 − 606 | |||||
F = 5 − 5 | 42248.836(20) | 17 | 0.54(17) | 0.50(20) | 1.01(29) |
F = 7 − 7 | 42248.879(20) | −11 | 1.48(24) | 0.68(20) | 2.04(29) |
F = 6 − 6 | 42249.309(20) | −5 | 1.83(16) | 0.83(17) | 2.08(29) |
716 − 707 | |||||
F = 8 − 8 + F = 6 − 6 | 43079.209(20) | 25 | 1.22(12) | 0.58(07) | 1.94(27) |
F = 7 − 7 | 43079.628(20) | 6 | 1.08(14) | 0.55(09) | 1.83(27) |
817 − 808 | |||||
F = 9 − 9 + 7 − 7 | 44042.119(20) | 9 | 1.17(35) | 1.05(30) | 1.05(35) |
918 − 909 | |||||
F = 10 − 10 + 8 − 8 | 45143.106(20) | 10 | 1.04(20) | 0.62(13) | 1.58(34) |
HCSCCH (f) | |||||
616 − 515 | 35370.056(10) | 0 | 0.68(12) | 0.87(15) | 0.73(17) |
606 − 505 | 35990.280(10) | −16 | 1.37(16) | 0.82(11) | 1.56(16) |
615 − 514 | 36660.308(20) | 32 | 0.52(10) | 0.57(14) | 0.86(18) |
625 − 524 | 36021.980(20) | −18 | 0.40(14) | 0.65(25) | 0.57(20) |
707 − 606 | 41975.060(20) | 28 | 0.93(33) | 0.54(20) | 1.61(35) |
717 − 616 | 41261.501(20) | 21 | 0.56(17) | 0.56(19) | 0.94(24) |
818 − 717 | 47151.323(20) | 39 | 2.02(67) | 0.91(25) | 2.10(44) |
Notes. Values between parentheses correspond to the uncertainties of the parameters in units of the least significant digits.
Observed frequency assuming a vLSR of 5.83 km s−1. The hyperfine splitting for a-type transitions is unresolved.
Observed minus calculated frequencies using the rotational constant of the merged fit provided in Table 1.
Line width at half intensity derived by fitting a Gaussian function to the observed line profile (in km s−1).
For this species, predicted frequencies are obtained from the rotational and distortion constants derived from a fit to the laboratory data of Brown & Godfrey (1982) and Cabtree et al. (2016).
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