SpheMakh

# the phase center PSF
self.phasePSF = phasePSF;
# Observed frequency
self.freq0 = freq0 or 1.;
# the compression in time
self.dtime = dtime or 1;
# the compression in frequency
self.dfreq = dfreq or 1;
# the resolution or the pixel size in radian
self.resolution = np.pi*(cellsize/3600.)/180.;

SpheMakh

#!/usr/bin/env python
# Convert s3-sex catalog to tigger LSM format
# Usage: ./s3-sex2tigger.py <s3 catalog> <output name> [freq for fluxes]
# The frequency is optional. It uses 1400 by default

import os
import sys 
import tempfile

s3model = sys.argv[1]

SpheMakh

## imaging Tut. 
## update Pyxis if you haven't done so since 05 Feb 2015.
## Also ensure that you have lwimager installed
# run as $ pyxis msname image[options] 
# options can be: cellsize,npix,gain,wprojplanes,column/data, etc 
# to make a per N channel image add im.IMAGE_CHANNELIZE=N
# Find the MSs at jake:~makhathini/ratt/imaging

import Pyxis
import ms

SpheMakh

import Pyxis
# once Pyxis is loaded, ms,mqt, im, lsm, std,stefcal become available
import ms # ms module
import im # imager module 
import mqt # meqtree-pipeliner wrap
import stefcal # self calibration module 
from Pyxis.ModSupport import * # I will make a note whenever I use something from here

define("MS_REDO",True,"Remake MS if it already exists")
 

SpheMakh

import numpy as np
from pyrap.tables import table
import pyrap.measures
  
def enu2itrf(xyz=None,casa_table=None,**kw):
  if casa_table:
      xyz = table(anttab).getcol("POSITION")
  import pyrap.measures
  dm = pyrap.measures.measures()
  dq = pyrap.measures.dq