Handling 2 and 3D data

If you have images or cubes that contain data that you want to view as spectra in some fashion, then SPLAT-VO will attempt to do this for you. There are three fundamental modes for doing this:

The default is to collapse. When collapsing cubes you have the option of which axis to step along selecting image planes, this is known as the select axis. To determine which option is used to handle your cubes or images you can either set values on the command-line, along with your spectra, or choose options in the open file dialogue. A command line that uses axis 3 as the dispersion axis and steps along axis 2 when choosing image planes might look like:

 % splat --ndaction collapse --dispax 3 --selectax 2 <spectral_cube> &
or in shorthand:
 % splat -n c -d 3 -s 2 <spectral_cube> &
If you don't choose a dispersion axis SPLAT-VO will make a good intelligent guess about this and step along the first axis that isn't the dispersion axis.



SPLAT-VO -- A VO-enabled Spectral Analysis Tool
Starlink User Note 243
Peter W. Draper
04 October 2005
E-mail:splat@star.rl.ac.uk

Copyright © 2001-2005 Council for the Central Laboratory of the Research Councils \& \ 2005 Particle Physics and Astronomy Research Council