
Note that the "Pickles" A0V spectrum I used for my image response curve is low resolution and goes just short of 8405A,
but this is good enough to see if the spectrum is radiometrically accurate on the balmer lines and it seems like it is.
I will re-image a A type star in the NOAO Indo-US Library (CFLIB) catalog to get a better image response curve. Progress was
also made to optimize the ISIS eshel bin (16 to 13 pixels high), which increased the resolution slightly and lowered
the noise(ThAr image centered on Order 34):

Now to reduce non-vega eShel spectra!
James