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uid 537

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This species has a counterpart in the theoretical library

Transitions

Frequency
[wavenumbers]
Wavelength
[microns]
Integrated cross-section
[km/mol]
3112 3.213 12.48
3091 3.235 40.7
3070 3.257 51.83
3025 3.306 7.791
2983 3.352 1.572
1947 5.136 2.93
1942 5.149 2.869
1926 5.192 4.164
1921 5.206 0.3166
1906 5.245 1.014
1902 5.257 0.9609
1884 5.307 1.177
1856 5.388 3.636
1836 5.448 1.049
1812 5.519 1.663
1803 5.545 1.215
1783 5.609 2.265
1760 5.683 0.7972
1734 5.765 0.7977
1692 5.909 5.178
1600 6.25 8.375
1590 6.291 1.492
1585 6.308 4.357
1570 6.368 1.068
1554 6.433 13
1510 6.622 0.7904
1505 6.645 2.582
1490 6.712 12.54
1471 6.797 7.364
1444 6.926 47.05
1437 6.958 21.97
1426 7.013 2.353
1419 7.047 4.066
1405 7.117 15
1353 7.393 6.444
1344 7.438 5.958
1334 7.493 1.904
1316 7.599 3.165
1274 7.847 1.06
1261 7.93 8.679
1228 8.145 0.6906
1211 8.256 8.854
1198 8.344 1.267
1174 8.522 0.7506
1171 8.543 1.7
1153 8.672 4.705
1120 8.929 4.755
1057 9.46 4.39
1004 9.959 3.898
964.9 10.36 0.7823
954.1 10.48 0.532
951.8 10.51 2.151
914.3 10.94 0.8474
890.5 11.23 1.364
876.8 11.41 29.85
828.1 12.08 1.988
800.1 12.5 26.86
769.3 13 1.054
752.5 13.29 121.1
742.6 13.47 8.945
704.3 14.2 18.98
667.8 14.97 0.6512
650.3 15.38 3.365
624.9 16 0.5282
605 16.53 3.678
577.4 17.32 22.23
461.7 21.66 6.445

Laboratory Spectrum

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This spectrum was measured using the matrix isolation technique. Samples are prepared by co-deposition of the PAH in the gaseous state with an overabundance of argon onto a cold CsI window suspended in a high vacuum chamber (p ~ 10-8 mtorr). The CsI window temperature is held between 10 and 15 K for the duration of the experiment. The infrared spectrum of the cold CsI window is recorded prior to (I0) and immediately after sample deposition (In). The absorbance spectrum for a neutral, matrix isolated PAH is log(In/I0).

By irradiating this matrix with ultraviolet radiation from a microwave powered hydrogen discharge lamp produces ionized PAHs. The infrared spectrum is again measured (Ii), now having absorption bands due to both the neutral and ionized PAH. This absorbance spectrum (log (I/Ii)) is compared with that of the neutral PAH. Most of the new bands produced by ultraviolet irradiation are due to the ionized form of the PAH. See the provided reference for the specific details regarding the data presented here. In some cases a few bands near 1600 cm-1 may be due to H2O.

Note(s):


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75 species present in version 2.00 of the experimental database (Nov 13, 2013)