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 Measurement to your model containing the emitting area of the source with identifier "Area" along with your Measurement of $L_{FIR}$.
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
Measurementto your model containing the emitting area of the source with identifier "Area" along with yourMeasurementof $L_{FIR}$.