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The Review of Scientific Instruments|July 1, 1978
Synchronized flash photolysis and pulse deposition in matrix isolation experimentsL J Allamandola, D Lucas, G C PimentelJournal of Molecular Structure|March 1, 1987
Interstellar problems and matrix solutionsL J AllamandolaNature|July 2, 1992
Is a pyrene-like molecular ion the cause of the 4,430-angstroms diffuse interstellar absorption band?F Salama, L J AllamandolaAdvances in Space Research : the Official Journal of the Committee on Space Research (COSPAR)|March 1, 1995
Polycyclic aromatic hydrocarbon ions and the diffuse interstellar bandsF Salama, L J AllamandolaIcarus|January 1, 1990
The volume- and surface-binding energies of ice systems containing CO, CO2, and H2OS A Sandford, L J AllamandolaThe Astrophysical Journal|September 7, 2001
Interstellar PAH emission in the 11-14 micron region: new insights from laboratory data and a tracer of ionized PAHsD M Hudgins, L J AllamandolaThe Astrophysical Journal|June 1, 1993
H2 in interstellar and extragalactic ices: infrared characteristics, ultraviolet production, and implicationsS A Sandford, L J AllamandolaThe Journal of Physical Chemistry|June 1, 1995
Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. 3. The polyacenes anthracene, tetracene, and pentaceneD M Hudgins, L J AllamandolaThe Journal of Physical Chemistry|March 9, 1995
Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. 2. The members of the thermodynamically most favorable series through coroneneD M Hudgins, L J AllamandolaThe Astrophysical Journal|September 7, 2001
The spacing of the interstellar 6.2 and 7.7 micron emission features as an indicator of polycyclic aromatic hydrocarbon sizeD M Hudgins, L J AllamandolaPageof 52