Sim Outputs

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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:

A Galactic SNR from a very early version of simdata: