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fringeSearch.py
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fringeSearch.py
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#!/usr/bin/env python3
"""
Given a collection of .npz files search for course delays and rates.
"""
import os
import sys
import glob
import numpy as np
import argparse
import tempfile
from datetime import datetime
from lsl.statistics import robust
from lsl.misc.mathutils import to_dB
from lsl.misc import parser as aph
from utils import read_correlator_configuration
from matplotlib import pyplot as plt
def main(args):
# Parse the command line
## Search limits
args.delay_window = [float(v) for v in args.delay_window.split(',', 1)]
args.rate_window = [float(v) for v in args.rate_window.split(',', 1)]
## Filenames
filenames = args.filename
filenames.sort()
if args.limit != -1:
filenames = filenames[:args.limit]
nInt = len(filenames)
dataDict = np.load(filenames[0])
tInt = dataDict['tInt']
nBL, nchan = dataDict['vis1XX'].shape
freq = dataDict['freq1']
junk0, refSrc, junk1, junk2, junk3, junk4, antennas = read_correlator_configuration(dataDict)
antLookup = {ant.config_name: ant.stand.id for ant in antennas}
antLookup_inv = {ant.stand.id: ant.config_name for ant in antennas}
dataDict.close()
# Make sure the reference antenna is in there
if args.ref_ant is None:
args.ref_ant = antennas[0].stand.id
else:
found = False
for ant in antennas:
if ant.stand.id == args.ref_ant:
found = True
break
elif ant.config_name == args.ref_ant:
args.ref_ant = ant.stand.id
found = True
break
if not found:
raise RuntimeError("Cannot file reference antenna %s in the data" % args.ref_ant)
# Process the baseline list
if args.baseline is not None:
newBaselines = []
for bl in args.baseline.split(','):
## Split and sort out antenna number vs. name
pair = bl.split('-')
try:
pair[0] = int(pair[0], 10)
except ValueError:
try:
pair[0] = antLookup[pair[0]]
except KeyError:
continue
try:
pair[1] = int(pair[1], 10)
except ValueError:
try:
pair[1] = antLookup[pair[1]]
except KeyError:
continue
## Fill the baseline list with the conjugates, if needed
newBaselines.append(tuple(pair))
newBaselines.append((pair[1], pair[0]))
## Update
args.baseline = newBaselines
bls = []
l = 0
cross = []
for i in range(0, len(antennas), 2):
ant1 = antennas[i].stand.id
for j in range(i, len(antennas), 2):
ant2 = antennas[j].stand.id
if ant1 != ant2:
bls.append( (ant1,ant2) )
cross.append( l )
l += 1
nBL = len(cross)
if args.decimate > 1:
if nchan % args.decimate != 0:
raise RuntimeError("Invalid freqeunce decimation factor: %i %% %i = %i" % (nchan, args.decimate, nchan%args.decimate))
nchan //= args.decimate
freq.shape = (freq.size//args.decimate, args.decimate)
freq = freq.mean(axis=1)
times = np.zeros(nInt, dtype=np.float64)
visXX = np.zeros((nInt,nBL,nchan), dtype=np.complex64)
if not args.y_only:
visXY = np.zeros((nInt,nBL,nchan), dtype=np.complex64)
visYX = np.zeros((nInt,nBL,nchan), dtype=np.complex64)
visYY = np.zeros((nInt,nBL,nchan), dtype=np.complex64)
for i,filename in enumerate(filenames):
dataDict = np.load(filename)
tStart = dataDict['tStart']
cvisXX = dataDict['vis1XX'][cross,:]
cvisXY = dataDict['vis1XY'][cross,:]
cvisYX = dataDict['vis1YX'][cross,:]
cvisYY = dataDict['vis1YY'][cross,:]
if args.decimate > 1:
cvisXX.shape = (cvisXX.shape[0], cvisXX.shape[1]//args.decimate, args.decimate)
cvisXX = cvisXX.mean(axis=2)
cvisXY.shape = (cvisXY.shape[0], cvisXY.shape[1]//args.decimate, args.decimate)
cvisXY = cvisXY.mean(axis=2)
cvisYX.shape = (cvisYX.shape[0], cvisYX.shape[1]//args.decimate, args.decimate)
cvisYX = cvisYX.mean(axis=2)
cvisYY.shape = (cvisYY.shape[0], cvisYY.shape[1]//args.decimate, args.decimate)
cvisYY = cvisYY.mean(axis=2)
visXX[i,:,:] = cvisXX
if not args.y_only:
visXY[i,:,:] = cvisXY
visYX[i,:,:] = cvisYX
visYY[i,:,:] = cvisYY
times[i] = tStart
dataDict.close()
print("Got %i files from %s to %s (%.1f s)" % (len(filenames), datetime.utcfromtimestamp(times[0]).strftime("%Y/%m/%d %H:%M:%S"), datetime.utcfromtimestamp(times[-1]).strftime("%Y/%m/%d %H:%M:%S"), (times[-1]-times[0])))
iTimes = np.zeros(nInt-1, dtype=times.dtype)
for i in range(1, len(times)):
iTimes[i-1] = times[i] - times[i-1]
print(" -> Interval: %.3f +/- %.3f seconds (%.3f to %.3f seconds)" % (iTimes.mean(), iTimes.std(), iTimes.min(), iTimes.max()))
print("Number of frequency channels: %i (~%.1f Hz/channel)" % (len(freq), freq[1]-freq[0]))
dTimes = times - times[0]
dMax = 1.0/(freq[1]-freq[0])/4
dMax = int(dMax*1e6)*1e-6
if -dMax*1e6 > args.delay_window[0]:
args.delay_window[0] = -dMax*1e6
if dMax*1e6 < args.delay_window[1]:
args.delay_window[1] = dMax*1e6
rMax = 1.0/iTimes.mean()/4
rMax = int(rMax*1e2)*1e-2
if -rMax*1e3 > args.rate_window[0]:
args.rate_window[0] = -rMax*1e3
if rMax*1e3 < args.rate_window[1]:
args.rate_window[1] = rMax*1e3
dres = 0.010
nDelays = int((args.delay_window[1]-args.delay_window[0])/dres)
while nDelays < 50:
dres /= 10
nDelays = int((args.delay_window[1]-args.delay_window[0])/dres)
while nDelays > 15000:
dres *= 10
nDelays = int((args.delay_window[1]-args.delay_window[0])/dres)
nDelays += (nDelays + 1) % 2
rres = 10.0
nRates = int((args.rate_window[1]-args.rate_window[0])/rres)
while nRates < 50:
rres /= 10
nRates = int((args.rate_window[1]-args.rate_window[0])/rres)
while nRates > 15000:
rres *= 10
nRates = int((args.rate_window[1]-args.rate_window[0])/rres)
nRates += (nRates + 1) % 2
print("Searching delays %.1f to %.1f us in steps of %.2f us" % (args.delay_window[0], args.delay_window[1], dres))
print(" rates %.1f to %.1f mHz in steps of %.2f mHz" % (args.rate_window[0], args.rate_window[1], rres))
print(" ")
delay = np.linspace(args.delay_window[0]*1e-6, args.delay_window[1]*1e-6, nDelays) # s
drate = np.linspace(args.rate_window[0]*1e-3, args.rate_window[1]*1e-3, nRates ) # Hz
# Find RFI and trim it out. This is done by computing average visibility
# amplitudes (a "spectrum") and running a median filter in frequency to extract
# the bandpass. After the spectrum has been bandpassed, 3sigma features are
# trimmed. Additionally, area where the bandpass fall below 10% of its mean
# value are also masked.
spec = np.median(np.abs(visXX.mean(axis=0)), axis=0)
spec += np.median(np.abs(visYY.mean(axis=0)), axis=0)
smth = spec*0.0
winSize = int(250e3/(freq[1]-freq[0]))
winSize += ((winSize+1)%2)
for i in range(smth.size):
mn = max([0, i-winSize//2])
mx = min([i+winSize//2+1, smth.size])
smth[i] = np.median(spec[mn:mx])
smth /= robust.mean(smth)
bp = spec / smth
good = np.where( (smth > 0.1) & (np.abs(bp-robust.mean(bp)) < 3*robust.std(bp)) & np.logical_and(freq<=args.hf, freq>=args.lf) )[0]
nBad = nchan - len(good)
print("Masking %i of %i channels (%.1f%%)" % (nBad, nchan, 100.0*nBad/nchan))
if args.plot:
fig = plt.figure()
ax = fig.gca()
ax.plot(freq/1e6, np.log10(spec)*10)
ax.plot(freq[good]/1e6, np.log10(spec[good])*10)
ax.set_title('Mean Visibility Amplitude')
ax.set_xlabel('Frequency [MHz]')
ax.set_ylabel('PSD [arb. dB]')
plt.draw()
freq2 = freq*1.0
freq2.shape += (1,)
dTimes2 = dTimes*1.0
dTimes2.shape += (1,)
dirName = os.path.basename( os.path.dirname(filenames[0]) )
print("%3s %9s %2s %6s %9s %11s" % ('#', 'BL', 'Pl', 'S/N', 'Delay', 'Rate'))
for b in range(len(bls)):
## Skip over baselines that are not in the baseline list (if provided)
if args.baseline is not None:
if bls[b] not in args.baseline:
continue
## Skip over baselines that don't include the reference antenna
elif bls[b][0] != args.ref_ant and bls[b][1] != args.ref_ant:
continue
## Check and see if we need to conjugate the visibility, i.e., switch from
## baseline (*,ref) to baseline (ref,*)
doConj = False
if bls[b][1] == args.ref_ant:
doConj = True
## Figure out which polarizations to process
if antLookup_inv[bls[b][0]][:3] != 'LWA' and antLookup_inv[bls[b][1]][:3] != 'LWA':
### Standard VLA-VLA baseline
polToUse = ('XX', 'YY')
visToUse = (visXX, visYY)
else:
### LWA-LWA or LWA-VLA baseline
if args.y_only:
polToUse = ('YX', 'YY')
visToUse = (visYX, visYY)
else:
polToUse = ('XX', 'XY', 'YX', 'YY')
visToUse = (visXX, visXY, visYX, visYY)
if args.plot:
fig = plt.figure()
axs = {}
axs['XX'] = fig.add_subplot(2, 2, 1)
axs['YY'] = fig.add_subplot(2, 2, 2)
axs['XY'] = fig.add_subplot(2, 2, 3)
axs['YX'] = fig.add_subplot(2, 2, 4)
for pol,vis in zip(polToUse, visToUse):
subData = vis[:,b,good]*1.0
if doConj:
subData = subData.conj()
subData = np.dot(subData, np.exp(-2j*np.pi*freq2[good,:]*delay))
subData /= freq2[good,:].size
amp = np.dot(subData.T, np.exp(-2j*np.pi*dTimes2*drate))
amp = np.abs(amp / dTimes2.size)
blName = bls[b]
if doConj:
blName = (bls[b][1],bls[b][0])
blName = '%s-%s' % (antLookup_inv[blName[0]], antLookup_inv[blName[1]])
best = np.where( amp == amp.max() )
if amp.max() > 0:
bsnr = (amp[best]-amp.mean())[0]/amp.std()
bdly = delay[best[0][0]]*1e6
brat = drate[best[1][0]]*1e3
print("%3i %11s %2s %6.2f %6.2f us %7.2f mHz" % (b, blName, pol, bsnr, bdly, brat))
else:
print("%3i %11s %2s %6s %9s %11s" % (b, blName, pol, '----', '----', '----'))
if args.plot:
axs[pol].imshow(amp, origin='lower', interpolation='nearest',
extent=(drate[0]*1e3, drate[-1]*1e3, delay[0]*1e6, delay[-1]*1e6),
cmap='gray_r')
axs[pol].plot(drate[best[1][0]]*1e3, delay[best[0][0]]*1e6, linestyle='', marker='x', color='r', ms=15, alpha=0.75)
if args.plot:
fig.suptitle(dirName)
for pol in axs.keys():
ax = axs[pol]
ax.axis('auto')
ax.set_title(pol)
ax.set_xlabel('Rate [mHz]')
ax.set_ylabel('Delay [$\\mu$s]')
fig.suptitle("%s @ %s" % (blName, refSrc.name))
plt.draw()
if args.plot:
plt.show()
if __name__ == "__main__":
parser = argparse.ArgumentParser(
description='given a collection of .npz files generated by superCorrelator.py, search for fringes',
formatter_class=argparse.ArgumentDefaultsHelpFormatter,
)
parser.add_argument('filename', type=str, nargs='+',
help='filename to search')
parser.add_argument('-r', '--ref-ant', type=str,
help='limit plots to baselines containing the reference antenna')
parser.add_argument('-b', '--baseline', type=str,
help="limit plots to the specified baseline in 'ANT-ANT' format")
parser.add_argument('-d', '--decimate', type=int, default=1,
help='frequency decimation factor')
parser.add_argument('-l', '--limit', type=int, default=-1,
help='limit the data loaded to the first N files, -1 = load all')
parser.add_argument('-y', '--y-only', action='store_true',
help='limit the search on VLA-LWA baselines to the VLA Y pol. only')
parser.add_argument('-e', '--delay-window', type=str, default='-inf,inf',
help='delay search window in us; defaults to maximum allowed')
parser.add_argument('-a', '--rate-window', type=str, default='-inf,inf',
help='rate search window in mHz; defaults to maximum allowed')
parser.add_argument('-p', '--plot', action='store_true',
help='show search plots at the end')
parser.add_argument('--hf', type=aph.frequency, default='98.0',
help='High frequency (in MHz) cutoff to use in fringe searching correlated data. Note: May be useful when high frequency RFI is present')
parser.add_argument('--lf', type=aph.frequency, default='0.0',
help='Low frequency (in MHz) cutoff to use in fringe searching correlated data. Note: May be useful when low frequency RFI is present')
args = parser.parse_args()
try:
args.ref_ant = int(args.ref_ant, 10)
except (TypeError, ValueError):
pass
main(args)