added a table and some logic to calculate G from IFIR#83
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This might be what you're looking for in #81. I added a new table (called IFIR.fits) which is equal to the G0 axis of the table multiplied by two to account for half the dust heating coming from sources other than the FUV (Which is a value appropriate for B stars, Wolfire et al. 1989). To use this table, add a$L_{FIR}$ .
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