PlanetPlots: Difference between revisions
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==Usage== | ==Usage== | ||
au.planetPlots(objects='Venus,Ceres,Vesta,Pallas,Juno,Jupiter,Callisto,Europa,Ganymede,Io,Titan,Uranus,Neptune', | 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 help setjy) | objects: comma-delimited string of planetary bodies (see help setjy) | ||
date: observing date, all plots are a 1-second snapshot at transit | date: observing date, all plots are a 1-second snapshot at transit | ||
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alma_cycle: 0 or 1 (will automatically fill in the configs) | alma_cycle: 0 or 1 (will automatically fill in the configs) | ||
configs: alternative to alma_cycle, specify a list of configurations | configs: alternative to alma_cycle, specify a list of configurations | ||
==Examples== | ==Examples== | ||
Revision as of 21:17, 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 help setjy) date: observing date, all plots are a 1-second snapshot at transit 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) configs: alternative to alma_cycle, specify a list of configurations
Examples
CASA <3>: au.planetPlots(date='2012-10-20')
