  Exoplanets are now being discovered in profusion. However, to understand
their character requires spectral models and data. These elements of remote
sensing can yield temperatures, compositions, and even weather patterns, but
only if significant improvements in both the parameter retrieval process and
measurements are achieved. Despite heroic efforts to garner constraining data
on exoplanet atmospheres and dynamics, reliable interpretation has oftimes
lagged ambition. I summarize the most productive, and at times novel, methods
employed to probe exoplanet atmospheres, highlight some of the most interesting
results obtained, and suggest various broad theoretical topics in which further
work could pay significant dividends.
