Synopsis
setpbnumeric(telescope, othertelescope, dopb, vect, maxrad, reffreq, isthispb, squintdir, squintreffreq, dosquint, paincrement, usesymmetricbeam)
Description
Supply a vector of vp/pb sample values taken on a regular grid between x=0 and
x=maxrad. We perform sinc interpolation to fill in the lookup table.
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 |
| vect |
|
Vector of vp/pb samples uniformly spaced from 0 to maxrad |
|
|
Allowed: |
Vector of Doubles |
|
|
Default: |
0 |
| maxrad |
|
Maximum radial extent of the vp/pb (scales with 1/freq) |
|
|
Allowed: |
Quantity |
|
|
Default: |
0.8deg |
| reffreq |
|
Frequency at which maxrad is specified |
|
|
Allowed: |
Quantity |
|
|
Default: |
1GHz |
| isthispb |
|
Do these parameters describe a PB or a VP? |
|
|
Allowed: |
String: 'PB'|'VP' |
| squintdir |
|
Offset of RR beam from pointing center, azel frame (scales with 1/freq) |
|
|
Allowed: |
Measure |
|
|
Default: |
Measure |
| squintreffreq |
|
Frequency at which the squint is specified |
|
|
Allowed: |
Quantity |
|
|
Default: |
1GHz |
| dosquint |
|
Enable the natural beam squint found in the common vp model |
|
|
Allowed: |
Bool |
|
|
Default: |
F |
| paincrement |
|
Increment in Parallactic Angle for asymmetric (ie, squinted) vp application |
|
|
Allowed: |
Quantity |
|
|
Default: |
360deg |
| usesymmetricbeam |
|
Not currently used |
|
|
Allowed: |
Bool |
|
|
Default: |
F |
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