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Table 1.

Line parameters of the detected transitions of HSO.

Transition νobs(a) νobs − νcalc(b) Δv Notes
(MHz) (MHz) (km s−1) (mK) (mK km s−1)
B1-b

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 1 − 0 39 517.602 ± 0.010 +0.008 0.95 ± 0.15 2.25 ± 0.47 2.28 ± 0.35
N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.198 ± 0.003 −0.024 1.22 ± 0.06 5.95 ± 0.37 7.73 ± 0.31
N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 1 − 1 39 553.383 ± 0.016 −0.054 1.38 ± 0.24 1.56 ± 0.46 2.30 ± 0.39
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 1 − 0 39 826.737 ± 0.022 +0.070 0.97 ± 0.32 1.19 ± 0.38 1.24 ± 0.33
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 0 − 1 39 857.384 ± 0.013 −0.028 1.14 ± 0.19 1.46 ± 0.36 1.77 ± 0.29
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 1 − 1 39 862.473 ± 0.015 −0.037 1.60 ± 0.24 1.71 ± 0.40 2.90 ± 0.38
N = 20, 2 − 10, 1J = 5/2 − 3/2 F = 2 − 1 79 162.483 ± 0.004 (A)
N = 20, 2 − 10, 1J = 5/2 − 3/2 F = 3 − 2 79 164.952 ± 0.016 +0.025 0.76 ± 0.22 9.90 ± 2.44 8.06 ± 1.58
N = 20, 2 − 10, 1J = 5/2 − 3/2 F = 2 − 2 79 183.698 (c) ≤3.07 (B)
N = 20, 2 − 10, 1J = 3/2 − 1/2 F = 1 − 1 79 368.415 (c) ≤3.20 (B)
N = 20, 2 − 10, 1J = 3/2 − 1/2 F = 1 − 0 79 373.513 (c) ≤3.22 (B)
N = 20, 2 − 10, 1J = 3/2 − 1/2 F = 2 − 1 79 378.760 ± 0.013 +0.064 0.33 ± 0.11 7.31 ± 2.22 2.54 ± 0.76
N = 20, 2 − 10, 1J = 3/2 − 3/2 F = 1 − 1 79 677.488 (c) ≤3.06 (B)
N = 20, 2 − 10, 1J = 3/2 − 3/2 F = 2 − 2 79 708.983 (c) ≤ 2.66 (B)

TMC-1 CP

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 1 − 0 39 517.601 ± 0.015 +0.007 1.30 ± 0.23 0.57 ± 0.13 0.78 ± 0.13
N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.209 ± 0.010 −0.013 1.19 ± 0.10 1.26 ± 0.13 1.60 ± 0.11
N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 1 − 1 39 553.438 ± 0.010 +0.001 0.38 ± 0.15 0.34 ± 0.12 0.14 ± 0.04
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 1 − 0 39 826.664 ± 0.010 −0.003 0.45 ± 0.21 0.38 ± 0.10 0.18 ± 0.06
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 0 − 1 39 857.413 ± 0.020 +0.001 0.88 ± 0.33 0.27 ± 0.12 0.25 ± 0.09
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 1 − 1 39 862.501 ± 0.017 −0.009 1.06 ± 0.34 0.51 ± 0.12 0.57 ± 0.16
N = 20, 2 − 10, 1J = 5/2 − 3/2 F = 3 − 2 79 164.927 (c) ≤2.00 (B)
N = 20, 2 − 10, 1J = 3/2 − 1/2 F = 2 − 1 79 378.696 (c) ≤1.90 (B)

L183

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 1 − 0 39 517.554 ± 0.015 −0.040 0.61 ± 0.21 1.50 ± 0.50 0.97 ± 0.34
N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.214 ± 0.012 −0.008 0.62 ± 0.45 2.42 ± 0.74 1.60 ± 0.68
N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 1 − 1 39 553.437 (c) ≤0.63 (B)
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 1 − 0 39 826.667 (c) ≤0.80 (B)
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 0 − 1 39 857.412 (c) ≤0.66 (B)
N = 10, 1 − 00, 0J = 1/2 − 1/2 F = 1 − 1 39 862.522 ± 0.014 +0.012 0.99 ± 0.17 2.26 ± 0.64 2.38 ± 0.46

L483

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.174 ± 0.006 −0.048 0.86 ± 0.10 2.47 ± 0.40 2.27 ± 0.24
N = 20, 2 − 10, 1J = 5/2 − 3/2 F = 3 − 2 79 164.927 (c) ≤3.58 (B)

L1495B

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.184 ± 0.010 −0.038 0.95 ± 0.14 2.97 ± 0.64 2.99 ± 0.45

L1527

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.130 ± 0.012 −0.092 1.26 ± 0.22 2.91 ± 0.50 3.90 ± 0.52

Lupus-1A

N = 10, 1 − 00, 0J = 3/2 − 1/2 F = 2 − 1 39 532.195 ± 0.007 −0.027 0.66 ± 0.13 4.43 ± 0.69 3.12 ± 0.48

Notes. All observational parameters and their associated uncertainties are obtained from a Gaussian fit to each line profile.

(a)

Observed frequencies adopting a vLSR of 6.70 and 5.83 km s−1 for B1-b and TMC-1 CP, respectively (see text). For the other dense cores, we used the following values: 2.4 km s−1 for L183 (Marcelino et al. 2009; Lattanzi et al. 2020), 5.3 km s−1 for L483 (Agúndez et al. 2019), 7.67 km s−1 for L1495B (Hirota et al. 2004), 5.9 km s−1 for L1527 (Yoshida et al. 2019), and 5.0 km s−1 for Lupus-1A (Sakai et al. 2010b).

(b)

Observed minus calculated frequency, where calculated frequencies are those obtained in this work (see text and Table A.1).

(c)

For the non-detected lines, frequencies in the table are the calculated ones.

(A) Blended with negative frequency-switching artifact.

(B) Non-detection 3σ limits are shown. The σ value is computed as , where the rms is measured in the spectra, c is the speed of light, δν is the spectral resolution (0.03815 MHz and 0.04883 MHz for the Yebes 40 m and the IRAM 30 m observations, respectively), and Δv is the full width at half maximun for which we used the average of the observed values.

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