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Frequency [wavenumbers]	Wavelength [microns]	Integrated cross-section [km/mol]	Symmetry	Scaling factor
3121	3.204	0.1048	A	0.9597
3114	3.211	0.6129	A	0.9597
3109	3.216	0.1548	A	0.9597
3105	3.22	3.605	A	0.9597
3103	3.223	0.4185	A	0.9597
3101	3.225	0.097	A	0.9597
3100	3.226	1.556	A	0.9597
3098	3.228	0.4487	A	0.9597
3094	3.232	0.5603	A	0.9597
3092	3.234	0.337	A	0.9597
3090	3.237	1.706	A	0.9597
3086	3.24	0.7814	A	0.9597
3086	3.24	0.1989	A	0.9597
3084	3.242	1.835	A	0.9597
3083	3.243	0.1012	A	0.9597
3082	3.245	0.5051	A	0.9597
3077	3.25	0.1686	A	0.9597
3075	3.252	0.4453	A	0.9597
1603	6.239	74.2	A	0.9691
1587	6.301	34.03	A	0.9691
1583	6.316	160.1	A	0.9691
1581	6.327	35.14	A	0.9691
1567	6.382	352	A	0.9691
1553	6.438	88.44	A	0.9691
1547	6.466	57.48	A	0.9691
1544	6.478	340.9	A	0.9691
1535	6.515	259.4	A	0.9691
1522	6.57	103.3	A	0.9691
1510	6.621	161.2	A	0.9691
1503	6.654	156.7	A	0.9691
1482	6.747	57.74	A	0.9691
1474	6.783	55.18	A	0.9691
1466	6.823	24.03	A	0.9691
1449	6.901	37.3	A	0.9691
1441	6.938	1.357	A	0.9691
1432	6.985	10.38	A	0.9691
1418	7.051	258.8	A	0.9691
1410	7.093	4.876	A	0.9691
1399	7.149	242.8	A	0.9691
1389	7.197	10.23	A	0.9691
1380	7.247	230.8	A	0.9691
1369	7.307	31.08	A	0.9691
1359	7.359	119.1	A	0.9691
1350	7.408	497.7	A	0.9691
1346	7.432	71.88	A	0.9691
1331	7.51	115.1	A	0.9691
1320	7.574	79.39	A	0.9691
1300	7.692	171.2	A	0.9691
1289	7.758	11.66	A	0.9691
1266	7.899	562.3	A	0.9691
1257	7.956	84.8	A	0.9691
1239	8.074	25.45	A	0.9691
1234	8.103	36.05	A	0.9691
1225	8.16	2.817	A	0.9691
1222	8.185	227.4	A	0.9691
1218	8.211	31.49	A	0.9691
1204	8.307	45.48	A	0.9691
1195	8.368	27.91	A	0.9691
1186	8.434	29.88	A	0.9691
1174	8.517	39.81	A	0.9691
1168	8.562	3.457	A	0.9691
1149	8.707	84.98	A	0.9691
1142	8.76	8.276	A	0.9691
1111	9.001	2.61	A	0.9691
1106	9.044	17.84	A	0.9691
1098	9.104	22.62	A	0.9691
1082	9.238	12.82	A	0.9691
1056	9.467	2.813	A	0.9794
1045	9.572	2.949	A	0.9794
1007	9.927	3.953	A	0.9794
1006	9.936	0.0337	A	0.9794
1005	9.949	4.096	A	0.9794
1003	9.975	0.3037	A	0.9794
997.5	10.03	1.111	A	0.9794
989	10.11	0.8576	A	0.9794
980.8	10.2	9.759	A	0.9794
972.4	10.28	6.062	A	0.9794
962.2	10.39	5.949	A	0.9794
957.9	10.44	7.592	A	0.9794
942.2	10.61	2.488	A	0.9794
930.3	10.75	15.84	A	0.9794
926.8	10.79	3.12	A	0.9794
923.5	10.83	5.76	A	0.9794
905.8	11.04	7.797	A	0.9794
887.4	11.27	1.995	A	0.9794
877.1	11.4	2.719	A	0.9794
870.6	11.49	13.8	A	0.9794
836.4	11.96	2.898	A	0.9794
836.1	11.96	41.41	A	0.9794
810.7	12.34	28.11	A	0.9794
808.4	12.37	11.79	A	0.9794
793.9	12.6	7.975	A	0.9794
793.8	12.6	5.461	A	0.9794
786.5	12.71	4.852	A	0.9794
769.6	12.99	6.238	A	0.9794
765.3	13.07	9.563	A	0.9794
758.1	13.19	21.29	A	0.9794
755.4	13.24	22.61	A	0.9794
742.9	13.46	23.15	A	0.9794
721.4	13.86	5.138	A	0.9794
716	13.97	15.21	A	0.9794
712.1	14.04	5.424	A	0.9794
684.2	14.62	0.1598	A	0.9794
651.8	15.34	1.48	A	0.9794
630.8	15.85	1.168	A	0.9794
628.3	15.92	4.274	A	0.9794
619.2	16.15	4.307	A	0.9794
614.4	16.28	0.5626	A	0.9794
583.2	17.15	3.212	A	0.9794
563.2	17.75	3.226	A	0.9794
547.4	18.27	20.29	A	0.9794
532.2	18.79	12.9	A	0.9794
515.8	19.39	13.52	A	0.9794
512.6	19.51	1.288	A	0.9794
510.2	19.6	9.266	A	0.9794
504.6	19.82	1.024	A	0.9794
497.6	20.1	7.42	A	0.9794
485.2	20.61	1.431	A	0.9794
472	21.19	4.935	A	0.9794
461.7	21.66	1.306	A	0.9794
446.2	22.41	9.896	A	0.9794
432	23.15	8.479	A	0.9794
418	23.92	5.571	A	0.9794
415.1	24.09	1.321	A	0.9794
399.8	25.01	1.502	A	0.9794
375.8	26.61	2.288	A	0.9794
354.2	28.23	0.4002	A	0.9794
338.3	29.56	3.976	A	0.9794
314.7	31.77	1.185	A	0.9794
295.3	33.87	1.304	A	0.9794
275	36.36	1.466	A	0.9794
258.5	38.68	2.572	A	0.9794
232.3	43.04	2.258	A	0.9794
217.1	46.07	3.153	A	0.9794
191.3	52.27	0.672	A	0.9794
168.5	59.36	2.445	A	0.9794
155.7	64.23	1.103	A	0.9794
146.4	68.32	0.3677	A	0.9794
112.4	88.97	1.103	A	0.9794
90.17	110.9	0.1488	A	0.9794
79.77	125.4	1.819	A	0.9794
57.88	172.8	0.6294	A	0.9794
41.61	240.4	0.3011	A	0.9794
29.05	344.2	0.3132	A	0.9794

Vibrations

• Bauschlicher, Jr., C.W., Ricca, A., Boersma, C., Allamandola, L.J., "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
• Boersma, C., Bauschlicher, Jr., C.W., Ricca, A., Mattioda, A.L., Cami, J., Peeters, E., Sánchez de Armas, F., Puerta Saborido, G., Hudgins, D.M., Allamandola, L.J., "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
• Ricca, A., Boersma, C., Maragkoudakis, A., Roser, J.E., Shannon, M.J., Allamandola, L.J., Bauschlicher Jr., C.W., "THE NASA AMES PAH IR SPECTROSCOPIC DATABASE: COMPUTATIONAL VERSION 4.00, SOFTWARE TOOLS, WEBSITE, AND DOCUMENTATION", The Astrophysical Journal Supplement Series, XXX, YYY, 2025 10.3847/1538-4365/ae1c38 — BibTeX - RIS