The script includes basic processing steps, including,
- Processing darks and flats,
- Applying dark and flat correction to image data (for a single image),
- Identifying the location of bright lines on arc-lamp images, tracing them along the spatial axis, and applying an interpolation to rectify an image along the wavelength axis.
What's missing?
- I haven't calculated a wavelength calibration solution based on arc lamp observations.
- I haven't rectified images along the spatial axis.