NASA Ames PAH IR Spectroscopic Database

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showing PAHs 1801 - 1900

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C₃₂H₁₈

uid	1517
id	24873
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1516
id	24872
symmetry	₃-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1515
id	24871
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1514
id	24870
symmetry	₃-A'
scaling factor	multiple (3)

C₃₂H₁₈

uid	1513
id	24869
symmetry	₁-A'
scaling factor	multiple (3)

C₃₂H₁₈

uid	1512
id	24868
symmetry	₃-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1511
id	24867
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1510
id	24866
symmetry	₃-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1509
id	24865
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1508
id	24864
symmetry	₃-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1507
id	24863
symmetry	₃-B
scaling factor	multiple (3)

C₃₂H₁₈

uid	1506
id	24862
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1505
id	24861
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1504
id	24860
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₈

uid	1503
id	24859
symmetry	₃-A'
scaling factor	multiple (3)

C₃₂H₁₈

uid	1502
id	24858
symmetry	₁-A'
scaling factor	multiple (3)

C₃₂H₁₈

uid	536
id	23900
symmetry	???
scaling factor	multiple (3)

C₃₂H₁₈

uid	535
id	23899
symmetry	???
scaling factor	multiple (3)

C₃₂H₁₈

uid	1762
id	28551
symmetry	₁-A
scaling factor	multiple (3)

C₃₂H₁₄⁺

uid	592
id	23952
symmetry	₂-A₂
scaling factor	multiple (3)

C₃₂H₁₄⁺

uid	5
id	28139
symmetry	₂-B₂G
scaling factor	multiple (3)

C₃₂H₁₄Mg⁺

uid	573
id	23933
symmetry	₂-A'
scaling factor	multiple (3)

C₃₂H₁₄Mg⁺

uid	572
id	23932
symmetry	₂-A
scaling factor	multiple (3)

C₃₂H₁₄Mg⁺

uid	571
id	23931
symmetry	₂-A'
scaling factor	multiple (3)

C₃₂H₁₄Mg⁺

uid	570
id	23930
symmetry	₂-A'
scaling factor	multiple (3)

C₃₂H₁₅⁺

uid	9
id	28143
symmetry	₁-A'
scaling factor	multiple (3)

C₃₂H₁₅⁺

uid	8
id	28142
symmetry	₁-A'
scaling factor	multiple (3)

C₃₂H₁₅⁺

uid	7
id	28141
symmetry	₁-A'
scaling factor	multiple (3)

C₃₂H₁₅⁺

uid	6
id	28140
symmetry	₁-A₁
scaling factor	multiple (3)

C₃₂H₁₈⁺

uid	546
id	23909
symmetry	₂-B
scaling factor	multiple (3)

C₃₂H₁₈⁺

uid	544
id	23907
symmetry	₂-
scaling factor	multiple (3)

C₃₂H₁₄⁺²

uid	10
id	28144
symmetry	₁-AG
scaling factor	multiple (3)

C₃₃

uid	2922
id	26278
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2923
id	26279
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2924
id	26280
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2925
id	26281
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2926
id	26282
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2927
id	26283
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2928
id	26284
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2929
id	26285
symmetry	₃-A"
scaling factor	multiple (3)

C₃₃

uid	2930
id	26286
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2931
id	26287
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2932
id	26288
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2933
id	26289
symmetry	₃-A'
scaling factor	multiple (3)

C₃₃

uid	2935
id	26291
symmetry	₇-A
scaling factor	multiple (3)

C₃₃

uid	2936
id	26292
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2937
id	26293
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2938
id	26294
symmetry	₃-A'
scaling factor	multiple (3)

C₃₃

uid	2939
id	26295
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2940
id	26296
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2941
id	26297
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2943
id	26299
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2944
id	26300
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2945
id	26301
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2946
id	26302
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2947
id	26303
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2948
id	26304
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2949
id	26305
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2950
id	26306
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2951
id	26307
symmetry	₁-A
scaling factor	multiple (3)

C₃₃

uid	2952
id	26308
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2953
id	26309
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2954
id	26310
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2955
id	26311
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2956
id	26312
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2957
id	26313
symmetry	₁-A
scaling factor	multiple (3)

C₃₃

uid	2958
id	26314
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2959
id	26315
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2960
id	26316
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2961
id	26317
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2962
id	26318
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2963
id	26319
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2964
id	26320
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2966
id	26322
symmetry	₃-A'
scaling factor	multiple (3)

C₃₃

uid	2967
id	26323
symmetry	₃-A'
scaling factor	multiple (3)

C₃₃

uid	2969
id	26325
symmetry	₁-A
scaling factor	multiple (3)

C₃₃

uid	2971
id	26327
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2972
id	26328
symmetry	₇-A"
scaling factor	multiple (3)

C₃₃

uid	2973
id	26329
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2974
id	26330
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2976
id	26332
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2977
id	26333
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2978
id	26334
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2979
id	26335
symmetry	₁-A'
scaling factor	multiple (3)

C₃₃

uid	2980
id	26336
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2982
id	26338
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2983
id	26339
symmetry	₅-A"
scaling factor	multiple (3)

C₃₃

uid	2984
id	26340
symmetry	₃-A'
scaling factor	multiple (3)

C₃₃

uid	2985
id	26341
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2986
id	26342
symmetry	₁-A
scaling factor	multiple (3)

C₃₃

uid	2987
id	26343
symmetry	₇-A
scaling factor	multiple (3)

C₃₃

uid	2988
id	26344
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2989
id	26345
symmetry	₇-A
scaling factor	multiple (3)

C₃₃

uid	2990
id	26346
symmetry	₁-A
scaling factor	multiple (3)

C₃₃

uid	2991
id	26347
symmetry	₅-A
scaling factor	multiple (3)

C₃₃

uid	2993
id	26349
symmetry	₁-A
scaling factor	multiple (3)

C₃₃

uid	2994
id	26350
symmetry	₇-A
scaling factor	multiple (3)

C₃₃

uid	2996
id	26352
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2997
id	26353
symmetry	₃-A
scaling factor	multiple (3)

C₃₃

uid	2999
id	26355
symmetry	₅-A
scaling factor	multiple (3)

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You are kindly asked to consider the following references for citation when using the database:

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, 282, 7, 2026 10.3847/1538-4365/ae1c38 — 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
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

4,233 species present in version 3.20 of the theoretical database (Sep 12, 2019)