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1. ICE CHEMISTRY ON OUTER SOLAR SYSTEM BODIES: ELECTRON RADIOLYSIS OF N

3. The Photochemistry of Purine in Ice Analogs Relevant to Dense Interstellar Clouds

4. The Detection of 6.9μm Emission Features in the Infrared Spectra of IRAS 04296+3429, IRAS 05341+0852, and IRAS 22272+5435: Evidence for the Presence of Hn-PAHs in Post-AGB Stars

5. OPTICAL CONSTANTS OF AMORPHOUS AND CRYSTALLINE H2O-ICE: 2.5-22 μm (4000-455 cm–1) OPTICAL CONSTANTS OF H2O-ICE

6. Near‐ and Mid‐Infrared Laboratory Spectra of PAH Cations in Solid H2O

7. Mechanisms of Amino Acid Formation in Interstellar Ice Analogs

8. Laboratory Infrared Spectra of Polycyclic Aromatic Nitrogen Heterocycles: Quinoline and Phenanthridine in Solid Argon and H2O

9. The Impact of Deuteration on the Infrared Spectra of Interstellar Polycyclic Aromatic Hydrocarbons

10. The Mid‐Infrared Laboratory Spectra of Naphthalene (C10H8) in Solid H2O

11. Deuterated Interstellar Polycyclic Aromatic Hydrocarbons

12. The Lifetimes of Nitriles (CN) and Acids (COOH) during Ultraviolet Photolysis and Their Survival in Space

13. Side Group Addition to the Polycyclic Aromatic Hydrocarbon Coronene by Proton Irradiation in Cosmic Ice Analogs

14. Side Group Addition to the Polycyclic Aromatic Hydrocarbon Coronene by Ultraviolet Photolysis in Cosmic Ice Analogs

15. The Photostability of Amino Acids in Space

16. The Abundances of Solid N2and Gaseous CO2in Interstellar Dense Molecular Clouds

17. H, C, N, and O Isotopic Substitution Studies of the 2165 Wavenumber (4.62 Micron) 'XCN' Feature Produced by Ultraviolet Photolysis of Mixed Molecular Ices

18. The Infrared Spectra of Nitriles and Related Compounds Frozen in Ar and H2O

19. ICE CHEMISTRY ON OUTER SOLAR SYSTEM BODIES: ELECTRON RADIOLYSIS OF N2-, CH4-, AND CO-CONTAINING ICES

20. N- ANDO-HETEROCYCLES PRODUCED FROM THE IRRADIATION OF BENZENE AND NAPHTHALENE IN H2O/NH3-CONTAINING ICES

21. THE PHOTOCHEMISTRY OF PYRIMIDINE IN REALISTIC ASTROPHYSICAL ICES AND THE PRODUCTION OF NUCLEOBASES

22. ICE CHEMISTRY ON OUTER SOLAR SYSTEM BODIES: CARBOXYLIC ACIDS, NITRILES, AND UREA DETECTED IN REFRACTORY RESIDUES PRODUCED FROM THE UV PHOTOLYSIS OF N2:CH4:CO-CONTAINING ICES

23. Deuterium enrichment of polycyclic aromatic hydrocarbons by photochemically induced exchange with deuterium-rich cosmic ices

24. Modeling the unidentified infrared emission with combinations of polycyclic aromatic hydrocarbons

25. Unraveling the 10 micron 'silicate' feature of protostars: the detection of frozen interstellar ammonia

26. The 2140 cm-1 (4.673 microns) solid CO band: the case for interstellar O2 and N2 and the photochemistry of nonpolar interstellar ice analogs

27. The galactic distribution of aliphatic hydrocarbons in the diffuse interstellar medium

28. Detection of the 2165 inverse centimeter (4.619 micron) XCN band in the spectrum of L1551 IRS 5

29. The physical and infrared spectral properties of CO2 in astrophysical ice analogs

30. Organic Compounds Produced by Photolysis of Realistic Interstellar and Cometary Ice Analogs Containing Methanol

31. Near-infrared absorption spectroscopy of interstellar hydrocarbon grains

32. Condensation and vaporization studies of CH3OH and NH3 ices: Major implications for astrochemistry

33. Spectral imaging of the 3.3 and 11.3 micron emission bands in NGC 1333 - Discovery of spatially separate band emissions

34. H2 in interstellar and extragalactic ices - Infrared characteristics, ultraviolet production, and implications

35. Infrared spectroscopy of dense clouds in the C-H stretch region - Methanol and 'diamonds'

36. 10 micron spectra of protostars and the solid methanol abundance

37. The spectrum of NGC 7027 from 3080 to 2630 wavenumbers (3.25-3.80 microns) - Detection of new atomic and molecular hydrogen lines and new constraints on the chemical sidegroups on polycyclic aromatic hydrocarbons

38. The discovery of a new infrared emission feature at 1905 wavenumbers (5.25 microns) in the spectrum of BD + 30 deg 3639 and its relation to the polycyclic aromatic hydrocarbon model

39. Laboratory infrared transmission spectra of individual interplanetary dust particles from 2.5 to 25 microns

40. Infrared emission from comets

41. New emission features in the 11-13 micron region and their relationship to polycyclic aromatic hydrocarbons

42. Laboratory studies of the infrared spectral propertries of CO in astrophysical ices

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