Protoplanetary Disk Simulation (CASA 3.4)
- This guide is applicable to CASA version 3.4. For older versions of CASA see PPdisk_simdata_(CASA_3.3).
- To create a script of the Python code on this page see Extracting scripts from these tutorials.
Script with Explanation
Set simobserve as the current task and reset all parameters.
# In CASA default("simobserve")
Review the image coordinate system using task imhead.
# This reports image header parameters in the Log Messages window imhead("input50pc_672GHz.fits")
We now us the ia (image analysis) and qa (units and quantities) tools from the CASA Toolkit to find the image center. In comparison to tasks, tools are a more advanced way of manipulating data in CASA. You can learn more about tools using the tool reference manual.
When data are being manipulated with tools the data file must be explicitly opened and closed.
# In CASA ia.open("input50pc_672GHz.fits")
Next, get the right ascension and declination of the image center. We get the number of pixels along each axis using ia.shape. Then, we get the RA and Dec values for the center pixel using ia.toworld.
# In CASA axesLength = ia.shape() # Divide the first two elements of axesLength by 2. center_pixel = [ x / 2.0 for x in axesLength[:2] ] # Feed center_pixel to ia.toworld and and save the RA and Dec to ra_radians and dec_radians (ra_radians, dec_radians) = ia.toworld( center_pixel )['numeric'][:2] ia.close()
Use the qa tool to convert the image center from radians to sexagesimal coordinates.
ra_hms = qa.formxxx(str(ra_radians)+"rad",format='hms',prec=5) dec_dms = qa.formxxx(str(dec_radians)+"rad",format='dms',prec=5)
Brightness scale can be viewed with 'imstat' task
# Default parameters are adequate for this imstat("input50pc_672GHz.fits") # ... # 'max': array([ 6.52469971e-05]), # ... # that's 0.0652 mJy/pixel.
Let's call our project "psim2". This defines the root prefix for any output files from simobserve.
project = "psim2"
We'll set skymodel to the FITS file downloaded, above, and leave all skymodel subparameters at their default values. simobserve will create CASA image psim2.skymodel.
skymodel = "input50pc_672GHz.fits"
We will specify the sky position for the center of the observation and set the map size to the size of the model image. Since the model image is 2/3 arcseconds across, we should only need one pointing. In this case, pointingspacing and maptype can be left at their default values.
setpointings = True direction = "J2000 18h00m00.031s -22d59m59.6s" mapsize = "0.76arcsec"
We do want to simulate an interferometric observation, so we set obsmode accordingly. We'll set totaltime to a 20-minute snapshot observation.
obsmode = "int" totaltime = "1200s"
We want to use the appropriate antenna configuration for the desired angular resolution. Configuration 20, alma.out20.cfg, is the largest "compact" configuration.
antennalist = "alma.out20.cfg"
Now run simobserve.
Deconvolve the visibilities back into an image
default ("simanalyze") project = "psim2" image = True # Prior image to use in clean modelimage = "input50pc_672GHz.fits" vis = project+".alma.out20.ms" imsize = [192, 192]
Specify number of iteration of cleaning task with proper threshold and weighting
niter = 10000 threshold = "1e-7Jy" weighting = "natural"
We'd like to calculate a difference and fidelity image, and see some diagnostics:
analyze = True
And see the array but not the UV coverage:
showuv = False showresidual = True showconvolved = True
Plot both to the screen and the png files with lots of messages:
graphics = "both" verbose = True overwrite = True
# This commands CASA to execute simanalyze simanalyze()
- Output results:
Last checked on CASA Version 3.4.0.