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Frequency [wavenumbers]	Wavelength [microns]	Integrated cross-section [km/mol]	Symmetry	Scaling factor
3110	3.215	1.407	A1	0.958
3098	3.228	0.2855	A1	0.958
3097	3.229	0.266	B2	0.958
3095	3.232	0.1247	A1	0.958
3094	3.232	0.7352	B2	0.958
3084	3.242	0.1184	A1	0.958
3083	3.243	0.3691	B2	0.958
3082	3.244	1.034	B2	0.958
3081	3.246	2.179	A1	0.958
3081	3.246	0.0005	B2	0.958
3080	3.246	0.0621	A1	0.958
3071	3.256	0.5697	A1	0.958
3071	3.257	0.5319	B2	0.958
1581	6.323	369.8	A1	0.958
1567	6.381	95.57	A1	0.958
1562	6.401	227.8	B2	0.958
1550	6.451	26.93	A1	0.958
1531	6.532	11.13	B2	0.958
1518	6.587	41.49	A1	0.958
1514	6.605	320.9	B2	0.958
1496	6.686	13.33	B2	0.958
1494	6.693	19.27	A1	0.958
1466	6.822	3.866	B2	0.958
1461	6.845	5.491	A1	0.958
1458	6.859	7.548	B2	0.958
1449	6.902	98.11	A1	0.958
1434	6.973	47.38	B2	0.958
1429	6.998	10.08	A1	0.958
1409	7.097	11.02	B2	0.958
1404	7.124	75.12	A1	0.958
1396	7.162	0.7509	B2	0.958
1383	7.23	3.869	A1	0.958
1375	7.271	59.47	B2	0.958
1357	7.369	509.6	B2	0.958
1349	7.412	114.5	A1	0.958
1344	7.438	0.0582	A1	0.958
1335	7.493	12.59	B2	0.958
1316	7.596	43.51	B2	0.958
1311	7.628	0.982	A1	0.958
1266	7.896	0.8814	B2	0.958
1254	7.972	33.36	A1	0.958
1227	8.147	29.91	A1	0.958
1225	8.166	51.74	B2	0.958
1218	8.21	11.64	B2	0.958
1217	8.219	116.4	A1	0.958
1203	8.312	0.2255	B2	0.958
1194	8.377	85.82	A1	0.958
1187	8.424	3.054	B2	0.958
1154	8.666	0.1889	A1	0.958
1153	8.676	4.257	B2	0.958
1136	8.805	112.1	B2	0.958
1135	8.808	3.318	A1	0.958
1069	9.351	1.048	A1	0.958
1065	9.393	2.218	B2	0.958
1047	9.552	0.0028	A1	0.958
1029	9.722	0.1448	B1	0.958
1013	9.872	0.2229	B1	0.958
1004	9.96	0	A2	0.958
995.3	10.05	0.082	B1	0.958
988.9	10.11	0	A2	0.958
984.2	10.16	13.57	B2	0.958
975.5	10.25	0	A2	0.958
939.2	10.65	75.52	B1	0.958
929.8	10.76	0.4837	A1	0.958
922	10.85	0	A2	0.958
905	11.05	0.5184	B2	0.958
879.8	11.37	83.73	B1	0.958
853.7	11.71	0	A2	0.958
843	11.86	7.048	A1	0.958
829	12.06	0.2206	B1	0.958
805.8	12.41	18.68	B1	0.958
797.2	12.54	0	A2	0.958
792.4	12.62	13.47	B2	0.958
775.6	12.89	5.399	A1	0.958
770.1	12.99	2.377	B1	0.958
755.4	13.24	19.16	B1	0.958
744.8	13.43	0	A2	0.958
731.1	13.68	0.6404	B2	0.958
726.9	13.76	25.67	A1	0.958
703.9	14.21	6.694	B1	0.958
673.3	14.85	1.594	A1	0.958
649.5	15.4	0.3968	B2	0.958
646.4	15.47	0	A2	0.958
627.1	15.95	0.0006	B1	0.958
617.1	16.21	1.019	B2	0.958
614.5	16.27	10.72	A1	0.958
592.5	16.88	1.958	B1	0.958
559.3	17.88	0	A2	0.958
547.4	18.27	0.4452	A1	0.958
536.4	18.64	30.98	B1	0.958
520.3	19.22	0.1293	B2	0.958
512.7	19.51	8.257	A1	0.958
508.7	19.66	0	A2	0.958
498.8	20.05	0.3042	B1	0.958
458.5	21.81	1.996	B2	0.958
454.9	21.98	0	A2	0.958
442.8	22.58	0.0016	A1	0.958
434.6	23.01	0.5719	B1	0.958
428.5	23.34	0.1831	B2	0.958
387.4	25.81	5.133	A1	0.958
361.7	27.65	0	A2	0.958
347.3	28.79	1.623	B2	0.958
327.5	30.54	5.387	A1	0.958
317.9	31.46	1.051	B1	0.958
299.4	33.4	0.7933	B1	0.958
280.2	35.69	0.0019	B2	0.958
278.4	35.91	0	A2	0.958
244.6	40.88	0	A2	0.958
234.6	42.62	0.3621	B1	0.958
165.9	60.29	2.517	B1	0.958
145.3	68.82	0	A2	0.958
108.2	92.45	12.18	B1	0.958
82.51	121.2	0	A2	0.958
63.99	156.3	1.513	B1	0.958

• 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