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Frequency [wavenumbers]	Wavelength [microns]	Integrated cross-section [km/mol]	Symmetry	Scaling factor
3125	3.2	0.0059	A	0.9597
3125	3.2	2.817	B	0.9597
3117	3.208	0.0026	A	0.9597
3117	3.208	1.432	B	0.9597
3109	3.217	0.0037	A	0.9597
3109	3.217	1.457	B	0.9597
3107	3.219	2.57	B	0.9597
3106	3.219	0.0011	A	0.9597
3099	3.227	0.0387	A	0.9597
3099	3.227	0.2135	B	0.9597
3097	3.228	0.1521	A	0.9597
3097	3.228	0.9903	B	0.9597
3089	3.237	0.1835	A	0.9597
3089	3.237	0.0279	B	0.9597
3085	3.241	0.0529	B	0.9597
3085	3.241	0.0481	A	0.9597
3083	3.244	0.0081	A	0.9597
3083	3.244	1.227	B	0.9597
1583	6.318	5.999	A	0.9691
1569	6.372	5.061	A	0.9691
1568	6.376	729.5	B	0.9691
1562	6.401	1.5	A	0.9691
1561	6.407	562.1	B	0.9691
1548	6.46	69.03	B	0.9691
1545	6.473	215.6	B	0.9691
1539	6.499	0.1584	A	0.9691
1519	6.583	70.49	B	0.9691
1518	6.588	0.365	A	0.9691
1513	6.611	68.53	B	0.9691
1483	6.741	0.9376	A	0.9691
1474	6.782	0.001	A	0.9691
1465	6.828	0.1406	A	0.9691
1459	6.855	193.1	B	0.9691
1440	6.944	16.54	B	0.9691
1436	6.962	15.09	B	0.9691
1432	6.983	1.993	A	0.9691
1430	6.994	4.02	A	0.9691
1414	7.074	18.1	B	0.9691
1378	7.257	5.333	A	0.9691
1373	7.282	69.26	B	0.9691
1363	7.337	89.59	B	0.9691
1347	7.425	9.415	A	0.9691
1345	7.433	0.0171	A	0.9691
1334	7.494	116.8	B	0.9691
1315	7.607	1934	B	0.9691
1311	7.627	2.483	A	0.9691
1296	7.715	0.0717	A	0.9691
1287	7.768	188.8	B	0.9691
1286	7.777	1.071	A	0.9691
1260	7.934	150.5	B	0.9691
1254	7.975	13.46	A	0.9691
1243	8.043	272.4	B	0.9691
1229	8.136	2.385	A	0.9691
1227	8.152	71.92	B	0.9691
1222	8.184	35.04	A	0.9691
1197	8.358	4.309	B	0.9691
1173	8.522	1.173	A	0.9691
1170	8.546	69.14	B	0.9691
1170	8.547	0.001	A	0.9691
1160	8.619	0.0008	A	0.9691
1154	8.669	28.05	B	0.9691
1130	8.848	0.2029	A	0.9691
1124	8.897	9.623	B	0.9691
1106	9.039	7.719	B	0.9691
1103	9.069	0.5325	A	0.9691
1081	9.248	0.0104	A	0.9691
1081	9.252	137.6	B	0.9691
1052	9.51	14.06	B	0.9794
1049	9.535	0.5833	A	0.9794
1015	9.853	0.0444	A	0.9794
1006	9.942	30.27	B	0.9794
1006	9.945	0.0016	A	0.9794
997.5	10.02	22.02	B	0.9794
995.3	10.05	0.7598	A	0.9794
987.4	10.13	35.41	B	0.9794
981.3	10.19	17.72	B	0.9794
978.2	10.22	2.47	A	0.9794
970.6	10.3	1.641	A	0.9794
966.4	10.35	9.698	B	0.9794
964	10.37	11.11	B	0.9794
953	10.49	16.62	B	0.9794
950.6	10.52	0.3426	A	0.9794
912.4	10.96	10.41	B	0.9794
895.5	11.17	2.574	A	0.9794
894.3	11.18	31.1	B	0.9794
869.3	11.5	0.6926	A	0.9794
850.3	11.76	0.9054	A	0.9794
830.3	12.04	8.655	B	0.9794
829.8	12.05	34.99	A	0.9794
821.3	12.18	9.296	B	0.9794
812.6	12.31	30.93	B	0.9794
806.1	12.4	78.27	A	0.9794
780.3	12.82	0.4569	A	0.9794
770.2	12.98	11.02	B	0.9794
769.8	12.99	1.601	A	0.9794
760.6	13.15	48.49	A	0.9794
756.3	13.22	7.157	B	0.9794
740.2	13.51	18.03	B	0.9794
736.6	13.58	0	A	0.9794
723.2	13.83	8.108	B	0.9794
707.2	14.14	21.53	A	0.9794
686.9	14.56	25.97	B	0.9794
684.5	14.61	4.469	A	0.9794
668.9	14.95	5.727	B	0.9794
634.5	15.76	0.4875	A	0.9794
619.4	16.15	0.206	A	0.9794
617.9	16.18	6.353	B	0.9794
608.3	16.44	23.17	B	0.9794
581.8	17.19	10.42	B	0.9794
566.9	17.64	0.0032	A	0.9794
558.3	17.91	5.409	A	0.9794
538.1	18.59	26.82	B	0.9794
529.7	18.88	2.457	A	0.9794
517.3	19.33	5.834	B	0.9794
511.1	19.57	12.03	B	0.9794
507.4	19.71	0.0498	A	0.9794
501.2	19.95	31.64	B	0.9794
488.9	20.46	3.123	A	0.9794
476.8	20.97	2.625	B	0.9794
446.9	22.38	5.471	A	0.9794
440.1	22.72	5.326	A	0.9794
417.8	23.93	0.0967	A	0.9794
414.3	24.14	2.576	B	0.9794
407.8	24.52	2.248	B	0.9794
394.5	25.35	0	A	0.9794
353.5	28.29	0.7634	A	0.9794
353.5	28.29	5.732	B	0.9794
315.9	31.66	11.54	B	0.9794
295.2	33.87	7.338	B	0.9794
290.2	34.46	0.0136	A	0.9794
260.7	38.36	1.337	B	0.9794
257.6	38.81	0.9157	A	0.9794
243.7	41.04	0.1319	A	0.9794
220.7	45.3	0.1867	B	0.9794
177.4	56.38	3.133	A	0.9794
175.4	57.01	1.155	B	0.9794
166.9	59.9	0.0334	A	0.9794
123.4	81.07	0.8014	A	0.9794
107.3	93.21	3.591	A	0.9794
102.9	97.14	1.607	B	0.9794
86.36	115.8	2.221	B	0.9794
70.48	141.9	0.3844	B	0.9794
42.14	237.3	0.298	A	0.9794
28.72	348.1	0.3125	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