Ab initio modeling of molecular IR spectra of astrophysical interest: application to CH4

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Table 4:

Comparison of partition functions for the complete datasets (Col. 2) and two truncated datasets. In addition partition functions from (Chakraborty et al. 2004) (Col. 5) are listed.
T [K]	Q	Q₅₈₀₀	Q₅₄₀₀	Q_Chak
100	118	118	118	117
200	330	330	330	329
300	609	609	609	609
400	965	965	965	968
500	1433	1433	1433	1448
600	2069	2069	2068	2109
700	2943	2940	2936	3032
800	4143	4128	4112	4321
900	5770	5719	5670	6103
1000	7931	7798	7678	8616
1100	10 728	10 436	10 185
1200	14 249	13 686	13 224
1300	18 563	17 581	16 807
1400	23 718	22 137	20 932
1500	29 738	27 349	25 580

Source LaTeX | All tables | In the text

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