21.3 KEPLER

[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 variable or the name of a GILDAS (or FITS) data file. The default is CLEAN.