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Frequency [wavenumbers]	Wavelength [microns]	Integrated cross-section [km/mol]	Symmetry	Scaling factor
3109	3.217	1.403	A1	0.958
3096	3.23	0.2789	A1	0.958
3095	3.231	0.3008	B2	0.958
3094	3.232	0.1155	A1	0.958
3094	3.232	0.6728	B2	0.958
3083	3.244	0.1289	A1	0.958
3082	3.245	0.3934	B2	0.958
3081	3.246	1.019	B2	0.958
3080	3.246	2.064	A1	0.958
3080	3.247	0.0001	B2	0.958
3079	3.247	0.1511	A1	0.958
3070	3.257	0.6133	A1	0.958
3070	3.257	0.5575	B2	0.958
1581	6.323	369.7	A1	0.958
1567	6.382	95.79	A1	0.958
1562	6.402	230.1	B2	0.958
1550	6.452	27.06	A1	0.958
1531	6.533	10.1	B2	0.958
1518	6.588	41.07	A1	0.958
1514	6.607	320.3	B2	0.958
1495	6.687	13.52	B2	0.958
1494	6.694	19.17	A1	0.958
1466	6.823	4.016	B2	0.958
1461	6.844	5.697	A1	0.958
1458	6.86	6.972	B2	0.958
1449	6.904	97.94	A1	0.958
1434	6.973	47.08	B2	0.958
1429	6.998	10.08	A1	0.958
1409	7.097	11.54	B2	0.958
1404	7.124	74.78	A1	0.958
1396	7.163	0.6461	B2	0.958
1383	7.232	4.109	A1	0.958
1375	7.272	60.15	B2	0.958
1357	7.369	507.7	B2	0.958
1349	7.413	114.6	A1	0.958
1344	7.439	0.0126	A1	0.958
1334	7.494	12.66	B2	0.958
1316	7.597	43.42	B2	0.958
1311	7.629	1.049	A1	0.958
1266	7.896	0.882	B2	0.958
1254	7.972	32.81	A1	0.958
1227	8.148	29.23	A1	0.958
1224	8.167	51.74	B2	0.958
1218	8.212	11.68	B2	0.958
1217	8.219	117.1	A1	0.958
1203	8.312	0.2136	B2	0.958
1194	8.377	86.1	A1	0.958
1187	8.426	2.967	B2	0.958
1154	8.667	0.235	A1	0.958
1153	8.675	4.878	B2	0.958
1136	8.804	112.1	B2	0.958
1135	8.809	3.459	A1	0.958
1069	9.353	1.006	A1	0.958
1065	9.393	2.164	B2	0.958
1047	9.551	0.0032	A1	0.958
1028	9.723	0.1716	B1	0.958
1013	9.873	0.1738	B1	0.958
1004	9.957	0	A2	0.958
995.5	10.05	0.0687	B1	0.958
989	10.11	0	A2	0.958
984.1	10.16	13.56	B2	0.958
976	10.25	0	A2	0.958
939.6	10.64	75.38	B1	0.958
929.8	10.76	0.486	A1	0.958
922.5	10.84	0	A2	0.958
905	11.05	0.5183	B2	0.958
879.9	11.36	83.98	B1	0.958
853.9	11.71	0	A2	0.958
843	11.86	7.065	A1	0.958
829.3	12.06	0.2145	B1	0.958
806	12.41	18.66	B1	0.958
797.2	12.54	0	A2	0.958
792.3	12.62	13.46	B2	0.958
775.6	12.89	5.358	A1	0.958
770.5	12.98	2.476	B1	0.958
755.6	13.23	19.13	B1	0.958
745	13.42	0	A2	0.958
731.3	13.67	0.6429	B2	0.958
726.9	13.76	25.67	A1	0.958
703.9	14.21	6.683	B1	0.958
673.3	14.85	1.617	A1	0.958
649.6	15.39	0.3848	B2	0.958
646.5	15.47	0	A2	0.958
627.2	15.94	0.0006	B1	0.958
616.8	16.21	1.018	B2	0.958
614.4	16.27	10.68	A1	0.958
592.3	16.88	1.977	B1	0.958
559.5	17.87	0	A2	0.958
547.6	18.26	0.4306	A1	0.958
536.8	18.63	30.9	B1	0.958
520.3	19.22	0.1268	B2	0.958
512.6	19.51	8.294	A1	0.958
509	19.64	0	A2	0.958
498.4	20.06	0.3032	B1	0.958
458.4	21.82	1.986	B2	0.958
454.7	21.99	0	A2	0.958
442.8	22.58	0.0013	A1	0.958
434.7	23	0.5627	B1	0.958
428.2	23.36	0.1918	B2	0.958
387.5	25.81	5.117	A1	0.958
361.6	27.65	0	A2	0.958
347.3	28.8	1.617	B2	0.958
327.4	30.54	5.391	A1	0.958
317.7	31.48	1.037	B1	0.958
298.7	33.47	0.7872	B1	0.958
279.7	35.75	0.0021	B2	0.958
277.8	35.99	0	A2	0.958
244.2	40.96	0	A2	0.958
234.1	42.72	0.3579	B1	0.958
165.6	60.38	2.466	B1	0.958
144.6	69.14	0	A2	0.958
106.8	93.67	12.27	B1	0.958
81.56	122.6	0	A2	0.958
63.78	156.8	1.401	B1	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