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| NRAO Home > CASA > CasaDocument | |||
1.1.1 Convert from pixel to world coordinate wrapped as Measures
Description
You can use this function to get the world coordinates for a specified absolute
pixel coordinate in the image. You specify a pixel coordinate (0-rel) for each
axis in the image.
If you supply fewer pixel values then there are axes in the image, your value will be padded out with the reference pixel for the missing axes. Excess values will be ignored.
The world coordinate is returned as a record of measures. This function is just a wrapper for the Coordsys tool toworld function (invoked with argument format=’m’). Please see its documentation for discussion about the formatting and meaning of the measures.
This Image tool function adds two additional fields to the return record.
The mask field contains the value of the image pixel mask at the specified position. It is either T (pixel is good) or F (pixel is masked as bad or the specified position was off the image).
The intensity field contains the value of the image (at the nearest pixel to that given) and its units. This is actually stored as a Quantity. This field does not exist if the specified pixel coordinate is off the image.
Arguments
| Inputs |
| ||
| pixel |
| Absolute pixel coordinate. Default is reference pixel.
| |
| allowed: | doubleArray |
|
| Default: | -1 |
|
Example
"""
# print "\t----\t coordmeasures Ex 1 \t----" ia.maketestimage(’myimage’,overwrite=true) s = ia.shape() for i in range(len(s)): s[i] = 0.5*s[i] meas = ia.coordmeasures(s) print meas.keys() # Get names of fields in record #[’intensity’, ’mask’, ’measure’] print meas[’intensity’] #{’value’: 1.39924156665802, ’unit’: ’Jy/beam’} print meas[’measure’][’direction’] #{’type’: ’direction’, # ’m1’: {’value’: 5.817764003289323e-05, ’unit’: ’rad’}, # ’m0’: {’value’: -5.8177644130875234e-05, ’unit’: ’rad’}, ’refer’: ’J2000’} dir = meas[’measure’][’direction’] # Get direction coordinate me.doframe(me.observatory(’ATCA’)) # Set location on earth me.doframe(me.epoch(’utc’,’16jun1999/12:30:20’)) # Set epoch azel = me.measure(dir,’azel’) # Convert to azimuth/elevation print ’az,el=’, qa.angle(azel[’m0’]), qa.angle(azel[’m1’]) # Format nicely #az,el= +105.15.47 -024.22.57 meas2=ia.coordmeasures() # defaults to reference pixel print meas2[’intensity’] #{’value’: 2.5064315795898438, ’unit’: ’Jy/beam’} print meas2[’measure’][’direction’] #{’type’: ’direction’, # ’m1’: {’value’: 0.0, ’unit’: ’rad’}, # ’m0’: {’value’: 0.0, ’unit’: ’rad’}, ’refer’: ’J2000’} dir = meas2[’measure’][’direction’] # Get direction coordinate me.doframe(me.observatory(’ATCA’)) # Set location on earth me.doframe(me.epoch(’utc’,’16jun1999/12:30:20’)) # Set epoch azel = me.measure(dir,’azel’) # Convert to azimuth/elevation print ’az,el=’, qa.angle(azel[’m0’]), qa.angle(azel[’m1’]) #az,el= +105.16.05 -024.23.00 # """ |
In this example we first find the world coordinates of the centre of the image. Then we use the Measures tool me to convert the direction coordinate field from J2000 to an azimuth and elevation at a particular location at a particular time.
Please send any comments or questions about CASA or AIPS++ to aips2-requests@nrao.edu
Copyright © 2007 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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