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Wagner DR, Kim HS, Saykally RJ 
Peripherally hydrogenated neutral polycyclic aromatic hydrocarbons as carriers of the 3 micron interstellar infrared emission complex: results from single-photon infrared emission spectroscopy. [Journal Article]
Astrophys J 2000 Dec 20; 545(2 Pt 1):854-60.
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Allamandola LJ, Tielens AG, Barker JR 
Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications. [Journal Article, Review]
Astrophys J Suppl Ser 1989 Dec.:733-75.
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Bernstein MP, Sandford SA, Allamandola LJ 
Hydrogenated polycyclic aromatic hydrocarbons and the 2940 and 2850 wavenumber (3.40 and 3.51 micron) infrared emission features. [Journal Article]
Astrophys J 1996 Dec 1; 472(2):L127-30.
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Cook DJ, Schlemmer S, Balucani N, et al. 
Single photon infrared emission spectroscopy: a study of IR emission from UV laser excited PAHs between 3 and 15 micrometers. [Journal Article]
J Phys Chem A Mol Spectrosc Kinet Environ Gen Theory 1998 Feb 26; 102(9):1465-81.
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Schlemmer S, Cook DJ, Harrison JA, et al. 
The unidentified interstellar infrared bands: PAHs as carriers? [Journal Article]
Science 1994 Sep 16.:1686-9.
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Sloan GC, Bregman JD, Geballe TR, et al. 
Variations in the 3 micron spectrum across the Orion Bar: polycyclic aromatic hydrocarbons and related molecules. [Journal Article]
Astrophys J 1997 Jan 10; 474(2 Pt 1):735-40.
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Allamandola LJ, Bregman JD, Sandford SA, et al. 
The discovery of a new infrared emission feature at 1905 wavenumbers (5.25 microns) in the spectrum of BD +30 degrees 3639 and its relation to the polycyclic aromatic hydrocarbon model. [Journal Article]
Astrophys J 1989 Oct 1; 345(1):L59-62.
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Hudgins DM, Allamandola LJ, Sandford SA 
Complex organic molecules in space: the carriers of the interstellar infrared emission features. [Journal Article]
Adv Space Res 1997; 19(7):999-1008.
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Cook DJ, , Schlemmer S, Balucani N, et al. 
Infrared emission spectra of candidate interstellar aromatic molecules. [Journal Article]
Nature 1996 Mar 21; 380(6571):227-9.
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