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Finishing Reduction
Once you have a wavelength-calibrated spectrum you may (again)
be happy enough and not need to go any further.
It is more likely that you will want to do one of two things,
either flux calibrate, or normalise the spectrum.
Subsections
Next: Flux Calibration & Extinction Correction
Up: Basic Steps in 1-D Data Reduction
Previous: Wavelength Calibration
Simple Spectroscopy Reductions
Starlink Cookbook 7
Martin Clayton and Anthony Holloway
15 June 1998
E-mail:starlink@jiscmail.ac.uk
Copyright © 2013 Science and Technology Facilities Council