This page lists some tips and tools for looking at and interpreting the data at the telescope.
Imaging
Pixel Scale:
Blue: 0.120 arcsec/pixel
Red: 0.123 arcsec/pixel
Rough guide to locating features in the 2-D spectra
Blue Grating spectrum:
wavelength increases with increasing x.
centered at ~4410 angstroms.
5577 OI auroral line at x=6410
linear dispersion ~ 0.5 angstroms/pix for unbinned spectra
Red spectrum:
wavelength decreases with increasing x.
centered at ~7730 angstroms.
5577 OI auroral line at X= 6710.
linear dispersion ~ 0.8 angstroms/pix for unbinned spectra
Dichroic cuts off at 5650 angstroms
Blue is transmitted
Red is reflected
Non-linearity and saturation
For flats, keep counts per pixel under 50,000 ADU (see manual, 1% non-linear at 55,000 ADU).
Aim for per pixel counts of 30,000-40,000 for flats, as above that there is no gain in S/N as you are in the fixed pattern regime where poisson statistics no longer hold true.