|
|||
NRAO Home > CASA > CASA Cookbook and User Reference Manual |
|
6.17 Using the CASA Toolkit for Image Analysis
Although this cookbook is aimed at general users employing the tasks, we include here a more detailed description of doing image analysis in the CASA toolkit. This is because there are currently only a few tasks geared towards image analysis, as well as due to the breadth of possible manipulations that the toolkit allows that more sophisticated users will appreciate.
To see a list of the ia methods available, use the CASA help command:
--------> help(ia)
Help on image object:
class image(__builtin__.object)
| image object
|
| Methods defined here:
|
| __init__(...)
| x.__init__(...) initializes x; see x.__class__.__doc__ for signature
|
| __str__(...)
| x.__str__() <==> str(x)
|
| adddegaxes(...)
| Add degenerate axes of the specified type to the image‘ :
| outfile
| direction = false
| spectral = false
| stokes
| linear = false
| tabular = false
| overwrite = false
| ----------------------------------------
|
| addnoise(...)
...
|
| unlock(...)
| Release any lock on the image‘ :
| ----------------------------------------
|
| ----------------------------------------------------------------------
| Data and other attributes defined here:
|
| __new__ = <built-in method __new__ of type object at 0x55d0f20>
| T.__new__(S, ...) -> a new object with type S, a subtype of T
or for a compact listing use <TAB> completion on ia., e.g.
Display all 105 possibilities? (y or n)
ia.__class__ ia.deconvolvecomponentlist ia.ispersistent ia.reorder
ia.__delattr__ ia.deconvolvefrombeam ia.lock ia.replacemaskedpixels
ia.__doc__ ia.done ia.makearray ia.restoringbeam
ia.__getattribute__ ia.echo ia.makecomplex ia.rotate
ia.__hash__ ia.fft ia.maketestimage ia.sepconvolve
ia.__init__ ia.findsources ia.maskhandler ia.set
ia.__new__ ia.fitallprofiles ia.maxfit ia.setboxregion
ia.__reduce__ ia.fitcomponents ia.miscinfo ia.setbrightnessunit
ia.__reduce_ex__ ia.fitpolynomial ia.modify ia.setcoordsys
ia.__repr__ ia.fitprofile ia.moments ia.sethistory
ia.__setattr__ ia.fromarray ia.name ia.setmiscinfo
ia.__str__ ia.fromascii ia.newimage ia.setrestoringbeam
ia.adddegaxes ia.fromfits ia.newimagefromarray ia.shape
ia.addnoise ia.fromimage ia.newimagefromfile ia.statistics
ia.boundingbox ia.fromrecord ia.newimagefromfits ia.subimage
ia.brightnessunit ia.fromshape ia.newimagefromimage ia.summary
ia.calc ia.getchunk ia.newimagefromshape ia.toASCII
ia.calcmask ia.getregion ia.open ia.tofits
ia.close ia.getslice ia.outputvariant ia.topixel
ia.collapse ia.hanning ia.pixelvalue ia.torecord
ia.continuumsub ia.haslock ia.putchunk ia.toworld
ia.convertflux ia.histograms ia.putregion ia.twopointcorrelation
ia.convolve ia.history ia.rebin ia.type
ia.convolve2d ia.imagecalc ia.regrid ia.unlock
ia.coordmeasures ia.imageconcat ia.remove
ia.coordsys ia.insert ia.removefile
ia.decompose ia.isopen ia.rename
A common use of the ia tool is to do region statistics on an image. The imhead task has mode=’stats’ to do this quickly over the entire image cube. The tool can do this on specific planes or sub-regions. For example, in the Jupiter 6cm example script (§ F.2), the ia tool is used to get on-source and off-source statistics for regression:
# Pull the max and rms from the clean image
ia.open(clnimage)
on_statistics=ia.statistics()
thistest_immax=on_statistics[’max’][0]
oldtest_immax = 1.07732224464
print ’ Clean image ON-SRC max should be ’,oldtest_immax
print ’ Found : Max in image = ’,thistest_immax
diff_immax = abs((oldtest_immax-thistest_immax)/oldtest_immax)
print ’ Difference (fractional) = ’,diff_immax
print ’’
# Now do stats in the lower right corner of the image
box = ia.setboxregion([0.75,0.00],[1.00,0.25],frac=true)
off_statistics=ia.statistics(region=box)
thistest_imrms=off_statistics[’rms’][0]
oldtest_imrms = 0.0010449
print ’ Clean image OFF-SRC rms should be ’,oldtest_imrms
print ’ Found : rms in image = ’,thistest_imrms
diff_imrms = abs((oldtest_imrms-thistest_imrms)/oldtest_imrms)
print ’ Difference (fractional) = ’,diff_imrms
print ’’
print ’ Final Clean image Dynamic Range = ’,thistest_immax/thistest_imrms
print ’’
print ’ =============== ’
ia.close()
Note: If you don’t close the file with, e.g., ia.close() the file will stay in a ’locked’ state. Other processes won’t be able to access the file until the file is properly closed.
More information about CASA may be found at the
CASA web page
Copyright © 2010 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
Home |
Contact Us |
Directories |
Site Map |
Help |
Privacy Policy |
Search