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NRAO Home > CASA > CASA Toolkit Reference Manual |
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vpmanager.setpbpoly - Function
2.3.2 Make a vp/pb from a polynomial
Description
The VP or PB is described as a polynomial of even powers:
![]() | (2.15) |
Arguments
Inputs |
| ||
telescope |
| Which telescope in the MS will use this vp/pb?
| |
| allowed: | string |
|
| Default: | VLA | |
othertelescope |
| If telescope==”OTHER”, specify name here
| |
| allowed: | string |
|
| Default: |
|
|
dopb |
| Should we apply the vp/pb to this telescope’s data?
| |
| allowed: | bool | |
| Default: | true |
|
coeff |
| Coefficients of even powered terms
| |
| allowed: | doubleArray |
|
| Default: | -1 |
|
maxrad |
| Maximum radial extent of the vp/pb (scales with 1/freq)
| |
| allowed: | any |
|
| Default: | variant 0.8deg |
|
reffreq |
| Frequency at which maxrad is specified
| |
| allowed: | any |
|
| Default: | variant 1.0GHz | |
isthispb |
| Do these parameters describe a PB or a VP?
| |
| allowed: | string |
|
| Default: | PB |
|
squintdir |
| Offset (Measure) of RR beam from pointing center, azel
frame (scales with 1/freq)
| |
| allowed: | any |
|
| Default: | variant
|
|
squintreffreq |
| Frequency at which the squint is specified
| |
| allowed: | any |
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| Default: | variant 1.0GHz |
|
dosquint |
| Enable the natural beam squint found in the common
vp model
| |
| allowed: | bool |
|
| Default: | false |
|
paincrement |
| Increment in Parallactic Angle for asymmetric (ie,
squinted) vp application
| |
| allowed: | any |
|
| Default: | variant 720 |
|
usesymmetricbeam |
| Not currently used
| |
| allowed: | bool |
|
| Default: | false |
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record
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