Wu, Schiminovich, and I met to discuss the progress of the S5 data reduction, which involves the assembly and unified reduction of a large number of galaxy spectra in the mid-infrared. We discussed progress and to-do items, but spent a bit of time understanding the geometry of the focal plane and spectral apertures, so that we could make informative figures and diagrams showing the relationship between the spectroscopy and our imaging data.
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