NASA Ames PAH IR Spectroscopic Database

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showing PAHs 701 - 800

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C₂₈H₁₄⁺

uid	729
id	24085
symmetry	₂-A"
scaling factor	multiple (3)

C₂₈H₁₄⁺

uid	3158
id	28666
symmetry	₂-BG
scaling factor	multiple (3)

C₂₉

uid	2504
id	25860
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2505
id	25861
symmetry	₇-A"
scaling factor	multiple (3)

C₂₉

uid	2507
id	25863
symmetry	₃-A'
scaling factor	multiple (2)

C₂₉

uid	2509
id	25865
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2510
id	25866
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2511
id	25867
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2513
id	25869
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2514
id	25870
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2516
id	25872
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2517
id	25873
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2518
id	25874
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2519
id	25875
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2520
id	25876
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2521
id	25877
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2522
id	25878
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2524
id	25880
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2525
id	25881
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2527
id	25883
symmetry	₇-B₁
scaling factor	multiple (3)

C₂₉

uid	2528
id	25884
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2529
id	25885
symmetry	₇-A"
scaling factor	multiple (3)

C₂₉

uid	2530
id	25886
symmetry	₇-B₁
scaling factor	multiple (2)

C₂₉

uid	2531
id	25887
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2532
id	25888
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2533
id	25889
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2534
id	25890
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2535
id	25891
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2536
id	25892
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2537
id	25893
symmetry	₁-A₁
scaling factor	multiple (3)

C₂₉

uid	2538
id	25894
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2539
id	25895
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2540
id	25896
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2541
id	25897
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2542
id	25898
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2543
id	25899
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2544
id	25900
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2545
id	25901
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2546
id	25902
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2547
id	25903
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2548
id	25904
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2549
id	25905
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2550
id	25906
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2551
id	25907
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2552
id	25908
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2553
id	25909
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2554
id	25910
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2555
id	25911
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2556
id	25912
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2557
id	25913
symmetry	₇-A"
scaling factor	multiple (3)

C₂₉

uid	2558
id	25914
symmetry	₇-A"
scaling factor	multiple (3)

C₂₉

uid	2559
id	25915
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2560
id	25916
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2561
id	25917
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2562
id	25918
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2563
id	25919
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2565
id	25921
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2566
id	25922
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2567
id	25923
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2568
id	25924
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2569
id	25925
symmetry	₃-A
scaling factor	multiple (3)

C₂₉

uid	2570
id	25926
symmetry	₇-A
scaling factor	multiple (3)

C₂₉

uid	2571
id	25927
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2572
id	25928
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2573
id	25929
symmetry	₅-A
scaling factor	multiple (3)

C₂₉

uid	2564
id	28573
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉

uid	2526
id	28572
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2523
id	28571
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2515
id	28570
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2512
id	28569
symmetry	₅-A"
scaling factor	multiple (3)

C₂₉

uid	2508
id	28568
symmetry	₃-A'
scaling factor	multiple (3)

C₂₉

uid	2506
id	28567
symmetry	₁-A'
scaling factor	multiple (3)

C₂₉H₁₅

uid	2166
id	25522
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2165
id	25521
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2164
id	25520
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₅

uid	2163
id	25519
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2162
id	25518
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2161
id	25517
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2160
id	25516
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₅

uid	2159
id	25515
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₅

uid	2158
id	25514
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2157
id	25513
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2156
id	25512
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2155
id	25511
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2154
id	25510
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₅

uid	2153
id	25509
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2152
id	25508
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₅

uid	2151
id	25507
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2150
id	25506
symmetry	₂-B₁
scaling factor	multiple (3)

C₂₉H₁₅

uid	2149
id	25505
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2148
id	25504
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2147
id	25503
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₅

uid	2146
id	25502
symmetry	₂-A"
scaling factor	multiple (3)

C₂₉H₁₇

uid	2145
id	25501
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₇

uid	2144
id	25500
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₇

uid	2143
id	25499
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₇

uid	2142
id	25498
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₇

uid	2141
id	25497
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₇

uid	2140
id	25496
symmetry	₂-A
scaling factor	multiple (3)

C₂₉H₁₇

uid	2139
id	25495
symmetry	₂-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)