[BUNDLES\]KEPLER [?|DataCube|INIT|SHOW [Arg]] [/MASK File Threshold]
[/RESET [Script] [/VSYSTEM Value] [/VELOCITY R function(R)]
[/HFS File [Opacity]]
Re-align spectra from a rotating thin disk according to the projected
rotation velocity at any point in the disk, and computes the combined
integrated spectrum and brightness radial distribution. The projection
assumes a thin disk (no flaring). By default, the disk is assumed to be
in Keplerian rotation.
The command is controlled by a set of KEPLER_* variables, whose values
can be verified by KEPLER ? and modified by the user. In addition to
the built-in KEPLER_* variables, KEPLER_RMAX indicates the radius
DataCube is the name of the data cube to be used. It can a SIC 3-D vari-
able or the name of a GILDAS (or FITS) data file. The default is CLEAN.
Subsections
Gildas manager
2023-06-01