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  • ...looks like that. I haven't seen such behaviour in simdata2) [[File:Ppdisk.simdata.txt]]
    242 bytes (40 words) - 11:23, 24 May 2010
  • ...ly use this configuration and resolve out most of the flux. i.e. this is a simdata demonstration, not a suggestion of what you should do with ALMA :) <tt>simdata2</tt> SMA observation and example of how to turn a Gaussian component into a
    939 bytes (155 words) - 13:48, 24 May 2010
  • ...convolved with the synthesized beam, and calculate a fidelity image. <tt>simdata</tt> can add thermal noise (from receiver, atmosphere, and ground) to the v ...tt>simdata</tt>, for example for new observatories that are unknown to <tt>simdata</tt>.
    10 KB (1,479 words) - 13:28, 30 April 2011
  • ''A new version of this page exists for CASA 3.3: [[N891 simdata (CASA 3.3)]].'' ...ut probably not very thoroughly explained. Updated for CASA 3.1 (simdata2->simdata)
    4 KB (609 words) - 10:38, 4 November 2011
  • ...convolved with the synthesized beam, and calculate a fidelity image. <tt>simdata</tt> can add thermal noise (from receiver, atmosphere, and ground) to the v ...tt>simdata</tt>, for example for new observatories that are unknown to <tt>simdata</tt>.
    8 KB (1,321 words) - 14:34, 1 November 2011