State-of-the-art in observations: what are the limits? when do we reach the confusion limit?
Variation of dust extinction curves in and out of translucent cloud
Observations of CH+, CH, CN, C2, C3 and other simple molecular absorptions in interstellar gas; their basic properties and mutual relations
Depletion patterns in interstellar clouds
The Observational Status of the Diffuse Interstellar Bands
Correlations among diffuse bands and their relation to physical conditions
Absorption band profiles and whether they can provide sufficient diagnostic criteria for identifying particular molecules, or classes of molecules, in the interstellar medium
Connecting observations in various wavelength regions
The physical and chemical conditions in translucent IS clouds
The electronic and general structural properties of molecules that could be formed and/or survive under the conditions of translucent interstellar clouds
Update and overview of the work on the most popular diffuse band carrier candidates; polycyclic aromatic hydrocarbons, carbon chains and rings, fullerenes
Overview of current astrophysical models — discussion of limits of models of translucent clouds
Shock waves in translucent clouds
H3+ absorption in interstellar clouds: implications for ionization rates
Chemical and physical ingredients of PDR models
Computational chemistry — update on new capabilities in quantum chemistry calculations
The contributions of PAHs to extinction and the thermal equilibrium of dust
Observational evidence for the response of grain properties to their physical environments
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