def create_blockvisibility(config: Configuration,
times: numpy.array,
frequency: numpy.array,
phasecentre: SkyCoord,
weight: float,
polarisation_frame=None,
integration_time=1.0,
channel_bandwidth=1e6) -> BlockVisibility:
""" Create a BlockVisibility from Configuration, hour angles, and direction of source
Note that we keep track of the integration time for BDA purposes
:param config: Configuration of antennas
:param times: hour angles in radians
:param frequency: frequencies (Hz] Shape [nchan]
:param weight: weight of a single sample
:param phasecentre: phasecentre of observation
:param npol: Number of polarizations
:param integration_time: Integration time ('auto' or value in s)
:returns: BlockVisibility
"""
assert phasecentre is not None, "Must specify phase centre"
if polarisation_frame is None:
polarisation_frame = correlate_polarisation(config.receptor_frame)
nch = len(frequency)
ants_xyz = config.data['xyz']
nants = len(config.data['names'])
nbaselines = int(nants * (nants - 1) / 2)
ntimes = len(times)
npol = polarisation_frame.npol
visshape = [ntimes, nants, nants, nch, npol]
rvis = numpy.zeros(visshape, dtype='complex')
rweight = weight * numpy.ones(visshape)
rtimes = numpy.zeros([ntimes])
ruvw = numpy.zeros([ntimes, nants, nants, 3])
# Do each hour angle in turn
for iha, ha in enumerate(times):
# Calculate the positions of the antennas as seen for this hour angle
# and declination
ant_pos = xyz_to_uvw(ants_xyz, ha, phasecentre.dec.rad)
rtimes[iha] = ha * 43200.0 / numpy.pi
# Loop over all pairs of antennas. Note that a2>a1
for a1 in range(nants):
for a2 in range(a1 + 1, nants):
ruvw[iha, a2, a1, :] = (ant_pos[a2, :] - ant_pos[a1, :])
ruvw[iha, a1, a2, :] = (ant_pos[a1, :] - ant_pos[a2, :])
rintegration_time = numpy.full_like(rtimes, integration_time)
rchannel_bandwidth = numpy.full_like(frequency, channel_bandwidth)
vis = BlockVisibility(uvw=ruvw,
time=rtimes,
frequency=frequency,
vis=rvis,
weight=rweight,
integration_time=rintegration_time,
channel_bandwidth=rchannel_bandwidth,
polarisation_frame=polarisation_frame)
vis.phasecentre = phasecentre
vis.configuration = config
log.info("create_visibility: %s" % (vis_summary(vis)))
assert type(
vis) is BlockVisibility, "vis is not a BlockVisibility: %r" % vis
return vis
def create_visibility(config: Configuration,
times: numpy.array,
frequency: numpy.array,
channel_bandwidth,
phasecentre: SkyCoord,
weight: float,
polarisation_frame=PolarisationFrame('stokesI'),
integration_time=1.0) -> Visibility:
""" Create a Visibility from Configuration, hour angles, and direction of source
Note that we keep track of the integration time for BDA purposes
:param config: Configuration of antennas
:param times: hour angles in radians
:param frequency: frequencies (Hz] Shape [nchan]
:param weight: weight of a single sample
:param phasecentre: phasecentre of observation
:param npol: Number of polarizations
:param integration_time: Integration time ('auto' or value in s)
:returns: Visibility
"""
assert phasecentre is not None, "Must specify phase centre"
if polarisation_frame is None:
polarisation_frame = correlate_polarisation(config.receptor_frame)
nch = len(frequency)
ants_xyz = config.data['xyz']
nants = len(config.data['names'])
nbaselines = int(nants * (nants - 1) / 2)
ntimes = len(times)
npol = polarisation_frame.npol
nrows = nbaselines * ntimes * nch
nrowsperintegration = nbaselines * nch
row = 0
rvis = numpy.zeros([nrows, npol], dtype='complex')
rweight = weight * numpy.ones([nrows, npol])
rtimes = numpy.zeros([nrows])
rfrequency = numpy.zeros([nrows])
rchannel_bandwidth = numpy.zeros([nrows])
rantenna1 = numpy.zeros([nrows], dtype='int')
rantenna2 = numpy.zeros([nrows], dtype='int')
ruvw = numpy.zeros([nrows, 3])
# Do each hour angle in turn
for iha, ha in enumerate(times):
# Calculate the positions of the antennas as seen for this hour angle
# and declination
ant_pos = xyz_to_uvw(ants_xyz, ha, phasecentre.dec.rad)
rtimes[row:row + nrowsperintegration] = ha * 43200.0 / numpy.pi
# Loop over all pairs of antennas. Note that a2>a1
for a1 in range(nants):
for a2 in range(a1 + 1, nants):
rantenna1[row:row + nch] = a1
rantenna2[row:row + nch] = a2
# Loop over all frequencies and polarisations
for ch in range(nch):
# noinspection PyUnresolvedReferences
k = frequency[ch] / constants.c.value
ruvw[row, :] = (ant_pos[a2, :] - ant_pos[a1, :]) * k
rfrequency[row] = frequency[ch]
rchannel_bandwidth[row] = channel_bandwidth[ch]
row += 1
assert row == nrows
rintegration_time = numpy.full_like(rtimes, integration_time)
vis = Visibility(uvw=ruvw,
time=rtimes,
antenna1=rantenna1,
antenna2=rantenna2,
frequency=rfrequency,
vis=rvis,
weight=rweight,
imaging_weight=rweight,
integration_time=rintegration_time,
channel_bandwidth=rchannel_bandwidth,
polarisation_frame=polarisation_frame)
vis.phasecentre = phasecentre
vis.configuration = config
log.info("create_visibility: %s" % (vis_summary(vis)))
assert type(vis) is Visibility, "vis is not a Visibility: %r" % vis
return vis
def test_correlate(self):
for frame in ["linear", "circular", "stokesI"]:
rec_frame = ReceptorFrame(frame)
assert correlate_polarisation(rec_frame) == PolarisationFrame(frame)