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Table A.4

Vacuum wavenumbers (cm-1) of clean CH CX transitions in our stellar spectra used for the calculation of the constants.

22
J R11ff R11ee Q11ef Q11fe P11ee P11ff

7.5 ... ... ... ... ... ...
8.5 ... ... ... ... 31192.72(21) ...
9.5 ... ... 31381.79(24) ... ... ...
10.5 ... ... 31369.38(56) ... 31121.54(30) ...
11.5 ... ... ... ... 31083.62(21) ...
12.5 ... ... ... ... 31043.85(1) ...
13.5 ... ... 31317.60(20) ... 31002.36(2) ...
14.5 ... ... 31294.66(–11) ... ... ...
15.5 ... 31628.30(–11) ... ... ... ...
16.5 ... 31614.50(–26) ... ... ... ...

J R22ff R22ee Q22ef Q22fe P22ff P22ee
7.5 ... ... ... ... ... 31193.40(–3)
8.5 ... ... ... 31382.58(10) ... ...
9.5 ... ... ... 31369.38(–19) ... 31121.54(–17)
10.5 ... ... ... ... ... 31083.62(–7)
11.5 ... ... ... ... ... 31043.85(–11)
12.5 ... ... ... 31317.60(–13) ... 31002.36(6)
13.5 ... ... ... 31294.66(–33) ... ...
14.5 31628.30(27) ... ... ... ... ...
15.5 31614.50(24) ... ... ... ... ...
16.5 ... ... ... ... ... ...

Notes. The numbers in parentheses are the observed minus calculated value.

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