vpmanager.setpbimage

Description Experimental: Supply an image of the E Jones elements. The format of the image is:

Shape: nx by ny by 4 complex polarizations (RR, RL, LR, LL or XX, XY, YX, YY) by 1 channel.
Direction coordinate: Az, El
Stokes coordinate: All four ``stokes'' parameters must be present in the sequence RR, RL, LR, LL or XX, XY, YX, YY.
Frequency: Only one channel is currently needed - frequency dependence beyond that is ignored.

One or two images may be specified - the real (must be present) and imaginary parts (optional).

Note that beamsquint must be intrinsic to the images themselves. This will be accounted for correctly by regridding of the images from Az-El to Ra-Dec according to the parallactic angle.

Arguments

`telescope`	Which telescope in the MS will use this vp/pb?
	`Allowed:`	`String`
`othertelescope`	If telescope=="OTHER", specify name here
	`Allowed:`	`String`
`dopb`	Should we apply the vp/pb to this telescope's data?
	`Allowed:`	`Bool`
	`Default:`	`T`
`realimage`	Real part of vp as an image
	`Allowed:`	`String`
	`Default:`	``''
`imagimage`	Imaginary part of vp as an image
	`Allowed:`	`String`
	`Default:`	``''

Returns itemcontainer

Next: vpmanager.setpbpoly - Function Up: vpmanager - Tool Previous: vpmanager.setpbnumeric - Function Contents Index

	`Package`	`synthesis`
	`Module`	`imager`
	`Tool`	`vpmanager`

vpmanager.setpbimage - Function