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Table A.2.

Measure differences (Δ(fJPL- fOBS)) and corresponding uncertainty (σΔ) between predicted (fJPL) and observed (fOBS) line frequencies.

Star fJPL v, NJ F′−F Δ(fJPL- fOBS) σΔ Channel width
(MHz) (MHz) (MHz) (MHz)
W Hya
130078.430 13 − 13+ -0.163 0.680 0.977
130113.648 12 − 12+ -0.141 0.667 0.977
265734.656 18+ − 18 1.359 1.379 0.977
265765.312 17+ − 17 1.600 1.367 0.977
333394.344 17 − 17+ 7.751 1.705 0.977
333411.688 18 − 18+ 6.448 1.873 0.977
130639.219 10+ − 10 -0.619 0.816 0.977
130654.695 11+ − 11 0.754 0.738 0.977
R Dor
107036.922 12+ − 12 -0.190 0.721 0.717
107073.172 11+ − 11 -0.273 0.812 0.717
252127.094 14+ − 14 2.605 1.650 0.977
252145.359 15+ − 15 2.345 1.645 0.977
317396.750 16+ − 16 5.941 1.854 1.953
317415.312 17+ − 17 6.636 1.598 1.953
351593.094 17 − 17+ 9.528 1.783 0.488
351611.656 18 − 18+ 9.161 1.769 0.488
IK Tau
252127.094 14+ − 14 2.988 1.633 1.953
252145.359 15+ − 15 2.109 1.660 1.953

Notes. These values are also displayed in Fig. 3. In Cols. 3 and 4 we indicate the transitions specifying the quantum numbers described in the text and the positive or negative parity of the energy levels involved. In the last column we give the channel width of the different spectra.

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