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Frequency [wavenumbers]	Wavelength [microns]	Integrated cross-section [km/mol]	Symmetry	Scaling factor
3083	3.244	30.85	?A	0.958
3066	3.261	51.53	?A	0.958
3065	3.263	115.3	?A	0.958
3064	3.264	24.74	?A	0.958
3063	3.265	3.444	?A	0.958
3049	3.28	11.3	?A	0.958
3046	3.283	7.789	?A	0.958
3045	3.284	7.787	?A	0.958
3044	3.285	13.16	?A	0.958
3043	3.286	7.88	?A	0.958
3042	3.287	1.022	?A	0.958
2991	3.343	19.49	?A	0.958
2952	3.387	23.01	?A	0.958
2903	3.445	42.07	?A	0.958
1605	6.231	22.46	?A	0.958
1602	6.242	9.488	?A	0.958
1600	6.251	0.7258	?A	0.958
1597	6.262	2.974	?A	0.958
1593	6.279	0.1586	?A	0.958
1531	6.53	0.2544	?A	0.958
1526	6.552	0.0925	?A	0.958
1501	6.663	0.5419	?A	0.958
1491	6.705	4.48	?A	0.958
1481	6.751	9.485	?A	0.958
1473	6.787	0.453	?A	0.958
1473	6.787	8.237	?A	0.958
1447	6.91	0.4479	?A	0.958
1439	6.95	1.482	?A	0.958
1429	6.998	0.0167	?A	0.958
1423	7.025	0.0006	?A	0.958
1406	7.111	0.6195	?A	0.958
1404	7.123	3.329	?A	0.958
1390	7.192	0.2331	?A	0.958
1389	7.198	0.7606	?A	0.958
1387	7.211	1.197	?A	0.958
1375	7.273	2.412	?A	0.958
1344	7.442	1.333	?A	0.958
1337	7.478	3.526	?A	0.958
1318	7.585	22.99	?A	0.958
1303	7.674	16.97	?A	0.958
1246	8.028	0.1575	?A	0.958
1241	8.057	0.4071	?A	0.958
1226	8.155	0.3845	?A	0.958
1221	8.192	0.6253	?A	0.958
1219	8.206	0.0759	?A	0.958
1208	8.281	0.6484	?A	0.958
1190	8.403	0.3541	?A	0.958
1172	8.533	0.3652	?A	0.958
1171	8.541	0.2659	?A	0.958
1160	8.618	0.0484	?A	0.958
1149	8.705	2.964	?A	0.958
1145	8.731	7.171	?A	0.958
1073	9.321	0.756	?A	0.958
1056	9.473	3.784	?A	0.958
1037	9.646	1.725	?A	0.958
998.6	10.01	1.458	?A	0.958
988.8	10.11	0.1139	?A	0.958
976.5	10.24	0.0067	?A	0.958
971.3	10.3	0.001	?A	0.958
965.6	10.36	0.0896	?A	0.958
959.1	10.43	0.0207	?A	0.958
954.8	10.47	0.3129	?A	0.958
953.4	10.49	0.0739	?A	0.958
898.3	11.13	0.5088	?A	0.958
890.5	11.23	44.97	?A	0.958
856.2	11.68	103.4	?A	0.958
842.2	11.87	0	?A	0.958
819.2	12.21	6.967	?A	0.958
804.4	12.43	0.0056	?A	0.958
804.4	12.43	0.0144	?A	0.958
795.6	12.57	0.0429	?A	0.958
793	12.61	2.116	?A	0.958
778.9	12.84	2.151	?A	0.958
777.4	12.86	7.227	?A	0.958
759.5	13.17	0.0601	?A	0.958
755	13.24	0.0161	?A	0.958
735.4	13.6	2.309	?A	0.958
678.4	14.74	0.018	?A	0.958
673.1	14.86	0.1198	?A	0.958
669	14.95	0.2351	?A	0.958
657.2	15.22	0.0033	?A	0.958
650.3	15.38	0.1874	?A	0.958
636.8	15.7	0.0008	?A	0.958
602.8	16.59	1.077	?A	0.958
570.4	17.53	7.764	?A	0.958
566	17.67	0.1664	?A	0.958
545.2	18.34	12.64	?A	0.958
541.4	18.47	0.1038	?A	0.958
527.4	18.96	1.179	?A	0.958
519	19.27	0.0686	?A	0.958
492.8	20.29	0.0618	?A	0.958
473.5	21.12	0.0754	?A	0.958
464.1	21.55	1.148	?A	0.958
448.8	22.28	0.0052	?A	0.958
443.9	22.53	0.4545	?A	0.958
405.6	24.66	1.869	?A	0.958
379.2	26.37	3.093	?A	0.958
364.2	27.46	0.0067	?A	0.958
347.3	28.8	1.036	?A	0.958
341.7	29.27	0.1112	?A	0.958
299.2	33.42	0.0019	?A	0.958
294.3	33.97	0.005	?A	0.958
291.2	34.34	0.0017	?A	0.958
259.1	38.6	0.8846	?A	0.958
236.5	42.28	0.0269	?A	0.958
197.1	50.74	0.0462	?A	0.958
169	59.18	0.0688	?A	0.958
143.9	69.5	0.9528	?A	0.958
113.9	87.79	3.421	?A	0.958
87.23	114.6	0.0027	?A	0.958
69.64	143.6	0.3013	?A	0.958

Vibrations

• C.W. Bauschlicher, Jr., A. Ricca, C. Boersma, L.J. Allamandola, "THE NASA AMES PAH IR SPECTROSCOPIC DATABASE: COMPUTATIONAL VERSION 3.00 WITH UPDATED CONTENT AND THE INTRODUCTION OF MULTIPLE SCALING FACTORS", The Astrophysical Journal Supplement Series, 234, 32, 2018 10.3847/1538-4365/aaa019 — BibTeX - RIS
• C. Boersma, C.W. Bauschlicher, Jr., A. Ricca, A.L. Mattioda, J. Cami, E. Peeters, F. Sánchez de Armas, G. Puerta Saborido, D.M. Hudgins, and L.J. Allamandola, "THE NASA AMES PAH IR SPECTROSCOPIC DATABASE VERSION 2.00: UPDATED CONTENT, WEBSITE AND ON/OFFLINE TOOLS", The Astrophysical Journal Supplement Series, 211, 8, 2014 10.1088/0067-0049/211/1/8 — BibTeX - RIS
• Mattioda, A. L., Hudgins, D. M., Boersma, C., Ricca, A., Peeters, E., Cami, J., Sánchez de Armas, F., Puerta Saborido, G., Bauschlicher, C. W., J., and Allamandola, L. J. "THE NASA AMES PAH IR SPECTROSCOPIC DATABASE: THE LABORATORY SPECTRA", The Astrophysical Journal Supplement Series, 251, 22, 2020 10.3847/1538-4365/abc2c8 — BibTeX - RIS