This shell script
reads a three-dimensional IFU NDF as input and presents the user
with a white-light image of the cube. You can then select and
X-Y position using the cursor. The script will extract and
display this spectrum. You will then be prompted to specify
various fitting parameters, e.g. peak position, using the
cursor. The script will then attempt to fit the emission line.
The fit will be displayed and you are consulted regarding the
goodness of fit. If you consider the fit to be good enough, the
script will attempt to perform similar fits to all spectra
within the cube, building a two-dimensional NDF image of the
strength of the line.
If you do not force the fit to be considered ``good'' by using the
-f command-line option, the script will offer the opportunity to
manually refit the spectral feature for individual pixels, such as
those that were unsuccessfully fitted by the automatic procedure.