Sim Outputs: Difference between revisions
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Created page with '== Early Science Simulation Examples == I chose a scaled image of M51 that would work for all of these with the same angular size, but of course once a larger array is ready at …' |
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Revision as of 17:47, 24 May 2010
Early Science Simulation Examples
I chose a scaled image of M51 that would work for all of these with the same angular size, but of course once a larger array is ready at the end of early science, one would not choose to only 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 :)
Early in CSV
Late in CSV
Early Science "medium" configuration
Early Science "large" configuration
Other Arrays and Miscellany
simdata2 SMA observation and example of how to turn a Gaussian component into an image:
File:SMAtest.py
[[File::SMAtest.png]]
A Galactic SNR from a very early version of simdata:
