Quick DEIMOS longslit data reduction.
Contact: Asher Wasserman, adwasser@ucsc.edu
What this does:
- combines flat and bias frames
- obtains a trace of a continuum source
- extracts a spectrum and subtracts sky flux
- calibrates wavelength solution
What this does not do (yet!):
- any quality checks
- flux calibration
Dependencies:
- Numpy
- Scipy
- Astropy
- astroscrappy (https://github.com/astropy/astroscrappy)