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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==== Early in CSV ==== | ==== Early in CSV ==== | ||
[[File:Csv.mid.png]]<br> | [[File:Csv.mid.png|200px]]<br> | ||
==== Late in CSV ==== | ==== Late in CSV ==== | ||
[[File:Csv.late.png]]<br> | [[File:Csv.late.png|200px]]<br> | ||
==== Early Science "medium" configuration ==== | ==== Early Science "medium" configuration ==== | ||
[[File:Early.med.png]]<br> | [[File:Early.med.png|200px]]<br> | ||
==== Early Science "large" configuration ==== | ==== Early Science "large" configuration ==== | ||
[[File:Early.large.png]]<br> | [[File:Early.large.png|200px]]<br> | ||
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<tt>simdata2</tt> SMA observation and example of how to turn a Gaussian component into an image: | <tt>simdata2</tt> SMA observation and example of how to turn a Gaussian component into an image: | ||
[[File:SMAtest.py]]<br> | [[File:SMAtest.py]]<br> | ||
[[File | [[File:SMAtest.png|200px]] | ||
A Galactic SNR from a very early version of <tt>simdata</tt>:<br> | A Galactic SNR from a very early version of <tt>simdata</tt>:<br> | ||
[[File:Crystal6.png]] | [[File:Crystal6.png|200px]] | ||
Latest revision as of 17:48, 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
A Galactic SNR from a very early version of simdata:
