PlanetPlots: Difference between revisions
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alma_cycle=1,configs=None) | alma_cycle=1,configs=None) | ||
objects: comma-delimited string of planetary bodies (see | objects: comma-delimited string of planetary bodies (see [http://casa.nrao.edu/stable/docs/TaskRef/setjy-task.html setjy for a list) | ||
date: observing date, all plots are a 1-second snapshot at transit | date: observing date, all plots are a 1-second snapshot at transit (see [http://casa.nrao.edu/stable/docs/TaskRef/predictcomp-task.html predictcomp]) | ||
freqs: a list of frequencies, in GHz | freqs: a list of frequencies, in GHz | ||
standard: the model in casa to use | standard: the model in casa to use | ||
Revision as of 21:41, 8 October 2012
Return to Analysis Utilities
This page documents the planetPlots function of Python module analysisUtils.
This function will create uv amplitude vs. uvdistance visibility plots for the specified objects, date, frequencies and ALMA configurations. The output is a multipage collection of a grid of plots, one page per object, where rows are configurations and columns are frequencies.
Usage
au.planetPlots(objects='Venus,Ceres,Vesta,Pallas,Juno,Jupiter,Callisto,Europa,Ganymede,Io,Titan,Uranus,Neptune',
date='2013-01-01', freqs = [100,230,345,690], standard = 'Butler-JPL-Horizons 2012',
alma_cycle=1,configs=None)
objects: comma-delimited string of planetary bodies (see [http://casa.nrao.edu/stable/docs/TaskRef/setjy-task.html setjy for a list)
date: observing date, all plots are a 1-second snapshot at transit (see [http://casa.nrao.edu/stable/docs/TaskRef/predictcomp-task.html predictcomp])
freqs: a list of frequencies, in GHz
standard: the model in casa to use
alma_cycle: 0 or 1 (will automatically fill in the configs offered)
configs: alternative to alma_cycle, specify a list of configurations, such as: ['alma_cycle1_1.cfg','alma_cycle1_2.cfg']
Examples
CASA <3>: au.planetPlots(date='2012-10-20')
complete PDF
Single page extracted for Neptune:
