def fixCyclicDedisp(fname, nchan=32, overwrite=False, ext='fix'):
# copied from paul's fix_cyclic_dedisp script
import psrchive
import os
import psr_utils
arch = psrchive.Archive_load(fname)
cf = arch.get_centre_frequency()
bw = arch.get_bandwidth()
f_lo = cf - bw/2.0
nch = arch.get_nchan()
pfb_nch = nchan
pfb_bw = bw / pfb_nch
chan_per_pfb = nch / pfb_nch
dm = arch.get_dispersion_measure()
for isub in range(arch.get_nsubint()):
sub = arch[isub]
per = sub.get_folding_period()
for ichan in range(nch):
pfb_cf = f_lo + ((ichan/chan_per_pfb)+0.5)*pfb_bw
dt = psr_utils.delay_from_DM(dm,pfb_cf) - psr_utils.delay_from_DM(dm,cf)
for ipol in range(sub.get_npol()):
prof = sub.get_Profile(ipol,ichan)
prof.rotate_phase(dt/per)
#arch.set_dedispersed(True) # doesn't work, lame...
if (overwrite):
outf = fname
else:
outf = fname + '.' + ext
arch.unload(outf)
os.system("psredit -m -c dmc=1 %s" % outf)
def dedisperse(self, dm=0, padval=0, ref_freq=None):
"""Shift channels according to the delays predicted by
the given DM.
Inputs:
dm: The DM (in pc/cm^3) to use.
padval: The padding value to use when shifting
channels during dedispersion. See documentation
of Spectra.shift_channels. (Default: 0)
Outputs:
None
*** Dedispersion happens in place ***
"""
if ref_freq is None:
ref_freq = 0.5*(self.freqs[0]+self.freqs[-1])
assert dm >= 0
ref_delay = psr_utils.delay_from_DM(dm-self.dm, ref_freq)
delays = psr_utils.delay_from_DM(dm-self.dm, self.freqs)
rel_delays = delays-ref_delay # Relative delay
rel_bindelays = np.round(rel_delays/self.dt).astype('int')
# Shift channels
self.shift_channels(rel_bindelays, padval)
self.dm=dm
def dedisperse(self, dm=0, padval=0, trim=False):
"""Shift channels according to the delays predicted by
the given DM.
Inputs:
dm: The DM (in pc/cm^3) to use.
padval: The padding value to use when shifting
channels during dedispersion. See documentation
of Spectra.shift_channels. (Default: 0)
trim: Remove spectra that are no longer complete
(Default: False)
Outputs:
None
*** Dedispersion happens in place ***
"""
assert dm >= 0
ref_delay = psr_utils.delay_from_DM(dm - self.dm, np.max(self.freqs))
delays = psr_utils.delay_from_DM(dm - self.dm, self.freqs)
rel_delays = delays - ref_delay # Relative delay
rel_bindelays = np.round(rel_delays / self.dt).astype('int')
# Shift channels
self.shift_channels(rel_bindelays, padval)
self.dm = dm
if trim:
ntrim = max(rel_bindelays)
if ntrim > 0:
self.data = self.data[:, :-ntrim]
self.numspectra -= ntrim
def shift(self,p=None,pdot=None,dm=None):
if dm is None:
dm = self.current_dm
if p is None:
p = self.current_p
if pdot is None:
pdot = self.current_pdot
f = rfft(self.profs,axis=-1)
# the sample at phase p is moved to phase p-dmdelays
dmdelays = (psr_utils.delay_from_DM(dm,self.pfd.subfreqs) -
psr_utils.delay_from_DM(self.current_dm,self.pfd.subfreqs))/self.original_fold_p
start_times = self.pfd.start_secs
pdelays = (start_times/self.original_fold_p) * (p-self.current_p)/self.original_fold_p
pdotdelays = ((pdot-self.current_pdot)*start_times**2/2.)/self.original_fold_p
f *= np.exp((2.j*np.pi)*
dmdelays[np.newaxis,:,np.newaxis]*
np.arange(f.shape[-1])[np.newaxis,np.newaxis,:])
f *= np.exp((2.j*np.pi)*
(pdelays+pdotdelays)[:,np.newaxis,np.newaxis]*
np.arange(f.shape[-1])[np.newaxis,np.newaxis,:])
self.profs = irfft(f)
self.current_p = p
self.current_dm = dm
self.current_pdt = pdot
def dedisperse(self, dm=0, padval=0, trim=False):
"""Shift channels according to the delays predicted by
the given DM.
Inputs:
dm: The DM (in pc/cm^3) to use.
padval: The padding value to use when shifting
channels during dedispersion. See documentation
of Spectra.shift_channels. (Default: 0)
trim: Remove spectra that are no longer complete
(Default: False)
Outputs:
None
*** Dedispersion happens in place ***
"""
assert dm >= 0
ref_delay = psr_utils.delay_from_DM(dm-self.dm, np.max(self.freqs))
delays = psr_utils.delay_from_DM(dm-self.dm, self.freqs)
rel_delays = delays-ref_delay # Relative delay
rel_bindelays = np.round(rel_delays/self.dt).astype('int')
# Shift channels
self.shift_channels(rel_bindelays, padval)
self.dm=dm
if trim:
ntrim = max(rel_bindelays)
if ntrim > 0:
self.data = self.data[:,:-ntrim]
self.numspectra -= ntrim
def fixCyclicDedisp(fname, nchan=32, overwrite=False, ext='fix'):
# copied from paul's fix_cyclic_dedisp script
import psrchive
import os
import psr_utils
arch = psrchive.Archive_load(fname)
cf = arch.get_centre_frequency()
bw = arch.get_bandwidth()
f_lo = cf - bw / 2.0
nch = arch.get_nchan()
pfb_nch = nchan
pfb_bw = bw / pfb_nch
chan_per_pfb = nch / pfb_nch
dm = arch.get_dispersion_measure()
for isub in range(arch.get_nsubint()):
sub = arch[isub]
per = sub.get_folding_period()
for ichan in range(nch):
pfb_cf = f_lo + ((ichan / chan_per_pfb) + 0.5) * pfb_bw
dt = psr_utils.delay_from_DM(dm, pfb_cf) - psr_utils.delay_from_DM(
dm, cf)
for ipol in range(sub.get_npol()):
prof = sub.get_Profile(ipol, ichan)
prof.rotate_phase(dt / per)
#arch.set_dedispersed(True) # doesn't work, lame...
if (overwrite):
outf = fname
else:
outf = fname + '.' + ext
arch.unload(outf)
os.system("psredit -m -c dmc=1 %s" % outf)
def write_toa(summed_pulse, template_profile, debug=False):
"""Given a SummedPulse generate a TOA and write it to stdout.
'template_profile' is simply a numpy array.
'debug' is a boolean value that determines if debugging
info should be displayed.
Returns shift required to line up template and pulse.
"""
if template_profile is None:
raise ValueError("A template profile MUST be provided.")
# This code is taken from Scott Ransom's PRESTO's get_TOAs.py
mjdi = int(summed_pulse.mjd) # integer part of MJD
mjdf = summed_pulse.mjd - mjdi # fractional part of MJD
# Period is duration of profile in seconds
period = summed_pulse.dt*len(summed_pulse.profile)
# Caclulate offset due to shifting channels to account for DM
# Hifreq doesn't have a half-channel offset
# (why? because get_TOAs.py doesn't. Why...)
# Why subtract 1 channel to get hifreq?
hifreq = summed_pulse.lofreq + summed_pulse.bw - summed_pulse.chan_width
midfreq = summed_pulse.lofreq - 0.5*summed_pulse.chan_width + 0.5*summed_pulse.bw
dmdelay = psr_utils.delay_from_DM(summed_pulse.dm, midfreq) - \
psr_utils.delay_from_DM(summed_pulse.dm, hifreq)
dmdelay_mjd = dmdelay/float(psr_utils.SECPERDAY)
if debug:
colour.cprint("High frequency (MHz): %f" % hifreq, 'debug')
colour.cprint("Mid frequency (MHz): %f" % midfreq, 'debug')
colour.cprint("DM delay added to TOAs (s): %g" % dmdelay, 'debug')
colour.cprint("DM delay added to TOAs (MJD): %g" % dmdelay_mjd, 'debug')
t0f = mjdf + dmdelay_mjd
t0i = mjdi
shift,eshift,snr,esnr,b,errb,ngood,tphs = measure_phase(summed_pulse.profile, \
template_profile)
# tphs is amount template is rotated by. It is originally
# measured in radians, convert to rotational phase
tphs = tphs/(np.pi*2.0) % 1.0
# tau and tau_err are the predicted phase of the pulse arrival
tau, tau_err = shift/summed_pulse.N, eshift/summed_pulse.N
if debug:
colour.cprint("FFTFIT: Shift (bins): %f, Tau (phase): %f" % (shift, tau), 'debug')
colour.cprint("FFTFIT: Shift error (bins): %f, Tau error (phase): %f" % \
(eshift, tau_err), 'debug')
# Note: "error" flags are shift = 0.0 and eshift = 999.0
if (np.fabs(shift) < 1e-7 and np.fabs(eshift-999.0) < 1e-7):
raise FFTFitError("Error in FFTFIT. Bad return values.")
# Send the TOA to STDOUT
toaf = t0f + tau*period/float(psr_utils.SECPERDAY)
if debug:
colour.cprint("t0f (MJD): %r" % t0f, 'debug')
colour.cprint("period (s): %r" % period, 'debug')
colour.cprint("toaf (MJD): %r" % toaf, 'debug')
newdays = int(np.floor(toaf))
obs_code = telescopes.telescope_to_id[summed_pulse.telescope]
psr_utils.write_princeton_toa(t0i+newdays, toaf-newdays, \
tau_err*period*1e6, midfreq, \
summed_pulse.dm, obs=obs_code)
return tau, tphs
def subband(self, nsub, subdm=None, padval=0):
"""Reduce the number of channels to 'nsub' by subbanding.
The channels within a subband are combined using the
DM 'subdm'. 'padval' is passed to the call to
'Spectra.shift_channels'.
Inputs:
nsub: Number of subbands. Must be a factor of
the number of channels.
subdm: The DM with which to combine channels within
each subband (Default: don't shift channels
within each subband)
padval: The padding value to use when shifting
channels during dedispersion. See documentation
of Spectra.shift_channels. (Default: 0)
Outputs:
None
*** Subbanding happens in-place ***
"""
assert (self.numchans % nsub) == 0
assert (subdm is None) or (subdm >= 0)
nchan_per_sub = self.numchans / nsub
sub_hifreqs = self.freqs[np.arange(nsub) * nchan_per_sub]
sub_lofreqs = self.freqs[(1 + np.arange(nsub)) * nchan_per_sub - 1]
sub_ctrfreqs = 0.5 * (sub_hifreqs + sub_lofreqs)
if subdm is not None:
# Compute delays
ref_delays = psr_utils.delay_from_DM(subdm - self.dm, sub_ctrfreqs)
delays = psr_utils.delay_from_DM(subdm - self.dm, self.freqs)
rel_delays = delays - ref_delays.repeat(
nchan_per_sub) # Relative delay
rel_bindelays = np.round(rel_delays / self.dt).astype('int')
# Shift channels
self.shift_channels(rel_bindelays, padval)
# Subband
self.data = np.array([np.sum(sub, axis=0) for sub in \
np.vsplit(self.data, nsub)])
self.freqs = sub_ctrfreqs
self.numchans = nsub
def subband(self, nsub, subdm=None, padval=0):
"""Reduce the number of channels to 'nsub' by subbanding.
The channels within a subband are combined using the
DM 'subdm'. 'padval' is passed to the call to
'Spectra.shift_channels'.
Inputs:
nsub: Number of subbands. Must be a factor of
the number of channels.
subdm: The DM with which to combine channels within
each subband (Default: don't shift channels
within each subband)
padval: The padding value to use when shifting
channels during dedispersion. See documentation
of Spectra.shift_channels. (Default: 0)
Outputs:
None
*** Subbanding happens in-place ***
"""
assert (self.numchans % nsub) == 0
assert (subdm is None) or (subdm >= 0)
nchan_per_sub = self.numchans/nsub
sub_hifreqs = self.freqs[np.arange(nsub)*nchan_per_sub]
sub_lofreqs = self.freqs[(1+np.arange(nsub))*nchan_per_sub-1]
sub_ctrfreqs = 0.5*(sub_hifreqs+sub_lofreqs)
if subdm is not None:
# Compute delays
ref_delays = psr_utils.delay_from_DM(subdm-self.dm, sub_hifreqs)
delays = psr_utils.delay_from_DM(subdm-self.dm, self.freqs)
rel_delays = delays-ref_delays.repeat(nchan_per_sub) # Relative delay
rel_bindelays = np.round(rel_delays/self.dt).astype('int')
# Shift channels
self.shift_channels(rel_bindelays, padval)
# Subband
self.data = np.array([np.sum(sub, axis=0) for sub in \
np.vsplit(self.data, nsub)])
self.freqs = sub_ctrfreqs
self.numchans = nsub
def getDMcurve(
M): # return the normalized DM curve downsampled to M points
feature = '%s:%s' % ('DMbins', M)
if M == 0:
return np.array([])
if not feature in self.extracted_feature:
ddm = (self.dms.max() - self.dms.min()) / 2.
loDM, hiDM = (self.bestdm - ddm, self.bestdm + ddm)
loDM = max((0, loDM)) #make sure cut off at 0 DM
hiDM = max((ddm, hiDM)) #make sure cut off at 0 DM
N = 100
interp = False
sumprofs = self.profs.sum(0)
if not interp:
profs = sumprofs
else:
profs = np.zeros(np.shape(sumprofs), dtype='d')
DMs = psr_utils.span(loDM, hiDM, N)
chis = np.zeros(N, dtype='f')
subdelays_bins = self.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, self.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * self.binspersec - subdelays_bins
if interp:
interp_factor = 16
for jj in range(self.nsub):
profs[jj] = psr_utils.interp_rotate(
sumprofs[jj],
delaybins[jj],
zoomfact=interp_factor)
# Note: Since the interpolation process slightly changes the values of the
# profs, we need to re-calculate the average profile value
avgprof = (profs / self.proflen).sum()
else:
new_subdelays_bins = np.floor(delaybins + 0.5)
for jj in range(self.nsub):
#profs[jj] = psr_utils.rotate(profs[jj], new_subdelays_bins[jj])
delay_bins = int(new_subdelays_bins[jj] %
len(profs[jj]))
if not delay_bins == 0:
profs[jj] = np.concatenate(
(profs[jj][delay_bins:],
profs[jj][:delay_bins]))
subdelays_bins += new_subdelays_bins
avgprof = self.avgprof
sumprof = profs.sum(0)
chis[ii] = self.calc_redchi2(prof=sumprof, avg=avgprof)
DMcurve = normalize(downsample(chis, M))
self.extracted_feature[feature] = DMcurve
return self.extracted_feature[feature]
def baseline_search(prof_2d, nchan, off_pulse_size, subfreqs, LOFAR=True):
nbin = prof_2d.shape[1]
binspersec = nbin / 0.0016627
tmp_fp = np.empty(np.shape(prof_2d))
mask = np.zeros(np.shape(prof_2d), dtype=bool)
mask[:, :off_pulse_size] = 1
binstep = 3
binshift_range = np.arange(0, nbin, binstep)
if LOFAR is False:
dmstep = 0.002 ## WSRT
dm_range = np.arange(0, 0.05, dmstep) ## WSRT
else:
dmstep = 0.0005 ## LOFAR
dm_range = np.arange(0, 0.01, dmstep) ## LOFAR
fit = np.empty((binshift_range.size, dm_range.size))
for binshift in binshift_range:
for dm in dm_range:
subdelays = psr_utils.delay_from_DM(dm, subfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * binspersec + binshift
for jj in range(nchan):
tmp_prof = prof_2d[jj, :].copy()
tmp_fp[jj] = psr_utils.fft_rotate(tmp_prof, delaybins[jj])
fit[binshift / binstep,
int(dm / dmstep)] = np.nanmean(tmp_fp[mask])
best = np.unravel_index(fit.argmin(), fit.shape)
Bin = best[0] * binstep
DM = best[1] * dmstep
subdelays = psr_utils.delay_from_DM(DM, subfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * binspersec + Bin
for jj in range(nchan):
tmp_prof = prof_2d[jj, :].copy()
tmp_fp[jj] = psr_utils.fft_rotate(tmp_prof, delaybins[jj])
base_perchan = np.nanmean(tmp_fp[:, :off_pulse_size], axis=1)
return base_perchan, DM
def dedisperse(self, dm=0, padval=0):
"""Shift channels according to the delays predicted by
the given DM.
Inputs:
dm: The DM (in pc/cm^3) to use.
padval: The padding value to use when shifting
channels during dedispersion. See documentation
of Spectra.shift_channels. (Default: 0)
Outputs:
None
*** Dedispersion happens in place ***
"""
assert dm >= 0
ref_delay = psr_utils.delay_from_DM(dm-self.dm, np.max(self.freqs))
delays = psr_utils.delay_from_DM(dm-self.dm, self.freqs)
rel_delays = delays-ref_delay # Relative delay
rel_bindelays = np.round(rel_delays/self.dt).astype('int')
# Shift channels
self.shift_channels(rel_bindelays, padval)
self.dm=dm
def plot(data,
cmap='gist_yarg',
show_cb=False,
sweep_dms=None,
sweep_posns=None):
if sweep_dms is None:
sweep_dms = []
if sweep_posns is None:
sweep_posns = []
ax = plt.axes((0.15, 0.15, 0.8, 0.7))
plot_spectra(data, cmap=cmap)
if show_cb:
cb = plt.colorbar()
cb.set_label("Scaled signal intensity (arbitrary units)")
plt.axis('tight')
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt * data.numspectra * sweep_posn + data.starttime
sty = SWEEP_STYLES[ii % len(SWEEP_STYLES)]
plt.plot(delays + sweepstart, data.freqs, sty, lw=4, alpha=0.5)
# Dressing it up
plt.xlabel("Time")
plt.ylabel("Observing frequency (MHz)")
#plt.suptitle("Frequency vs. Time")
sumax = plt.axes((0.15, 0.85, 0.8, 0.1), sharex=ax)
plot_timeseries(data)
plt.setp(sumax.get_xticklabels() + sumax.get_yticklabels(), visible=False)
plt.ylabel("Intensity")
plt.ticklabel_format(style='plain', useOffset=False)
plt.axis('tight')
return sumax, ax
def getDMcurve(M): # return the normalized DM curve downsampled to M points
feature = '%s:%s' % ('DMbins', M)
if M == 0:
return np.array([])
if not feature in self.extracted_feature:
ddm = (self.dms.max() - self.dms.min())/2.
loDM, hiDM = (self.bestdm - ddm , self.bestdm + ddm)
loDM = max((0, loDM)) #make sure cut off at 0 DM
hiDM = max((ddm, hiDM)) #make sure cut off at 0 DM
N = 100
interp = False
sumprofs = self.profs.sum(0)
if not interp:
profs = sumprofs
else:
profs = np.zeros(np.shape(sumprofs), dtype='d')
DMs = psr_utils.span(loDM, hiDM, N)
chis = np.zeros(N, dtype='f')
subdelays_bins = self.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, self.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays*self.binspersec - subdelays_bins
if interp:
interp_factor = 16
for jj in range(self.nsub):
profs[jj] = psr_utils.interp_rotate(sumprofs[jj], delaybins[jj],
zoomfact=interp_factor)
# Note: Since the interpolation process slightly changes the values of the
# profs, we need to re-calculate the average profile value
avgprof = (profs/self.proflen).sum()
else:
new_subdelays_bins = np.floor(delaybins+0.5)
for jj in range(self.nsub):
#profs[jj] = psr_utils.rotate(profs[jj], new_subdelays_bins[jj])
delay_bins = int(new_subdelays_bins[jj] % len(profs[jj]))
if not delay_bins==0:
profs[jj] = np.concatenate((profs[jj][delay_bins:], profs[jj][:delay_bins]))
subdelays_bins += new_subdelays_bins
avgprof = self.avgprof
sumprof = profs.sum(0)
chis[ii] = self.calc_redchi2(prof=sumprof, avg=avgprof)
DMcurve = normalize(downsample(chis, M))
self.extracted_feature[feature] = DMcurve
return self.extracted_feature[feature]
def dedisperse(self, DM=None, interp=0, doppler=1):
"""
dedisperse(DM=self.bestdm, interp=0, doppler=1):
Rotate (internally) the profiles so that they are de-dispersed
at a dispersion measure of DM. Use FFT-based interpolation if
'interp' is non-zero (NOTE: It is off by default!).
Doppler shift subband frequencies if doppler is non-zero.
(NOTE: It is *ON* by default. This default behaviour is
different with respect to PRESTO's prepfold.py)
"""
if DM is None:
DM = self.bestdm
# Note: Since TEMPO Doppler corrects observing frequencies, for
# TOAs, at least, we need to de-disperse using topocentric
# observing frequencies.
if doppler:
freqs = psr_utils.doppler(self.subfreqs, self.avgvoverc)
else:
freqs = self.subfreqs
self.subdelays = psr_utils.delay_from_DM(DM, freqs)
self.hifreqdelay = self.subdelays[-1]
self.subdelays = self.subdelays - self.hifreqdelay
delaybins = self.subdelays * self.binspersec - self.subdelays_bins
if interp:
new_subdelays_bins = delaybins
for ii in range(self.npart):
for jj in range(self.nsub):
tmp_prof = self.profs[ii, jj, :]
self.profs[ii, jj] = psr_utils.fft_rotate(
tmp_prof, delaybins[jj])
# Note: Since the rotation process slightly changes the values of the
# profs, we need to re-calculate the average profile value
self.avgprof = (self.profs / self.proflen).sum()
else:
new_subdelays_bins = Num.floor(delaybins + 0.5)
#print "DEBUG: in myprepfold.py -- DM, new_subdelays_bins:", DM, new_subdelays_bins
for ii in range(self.nsub):
rotbins = int(new_subdelays_bins[ii]) % self.proflen
if rotbins: # i.e. if not zero
subdata = self.profs[:, ii, :]
self.profs[:, ii] = Num.concatenate(
(subdata[:, rotbins:], subdata[:, :rotbins]), 1)
self.subdelays_bins += new_subdelays_bins
self.sumprof = self.profs.sum(0).sum(0)
if Num.fabs((self.sumprof / self.proflen).sum() - self.avgprof) > 1.0:
print "self.avgprof is not the correct value!"
self.currdm = DM
def plot_chi2_vs_DM(self, loDM, hiDM, N=100, interp=0, device='/xwin'):
"""
plot_chi2_vs_DM(self, loDM, hiDM, N=100, interp=0, device='/xwin'):
Plot (and return) an array showing the reduced-chi^2 versus
DM (N DMs spanning loDM-hiDM). Use sinc_interpolation
if 'interp' is non-zero.
"""
# Sum the profiles in time
sumprofs = self.profs.sum(0)
if not interp:
profs = sumprofs
else:
profs = Num.zeros(Num.shape(sumprofs), dtype='d')
DMs = psr_utils.span(loDM, hiDM, N)
chis = Num.zeros(N, dtype='f')
subdelays_bins = self.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, self.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * self.binspersec - subdelays_bins
if interp:
interp_factor = 16
for jj in range(self.nsub):
profs[jj] = psr_utils.interp_rotate(sumprofs[jj],
delaybins[jj],
zoomfact=interp_factor)
# Note: Since the interpolation process slightly changes the values of the
# profs, we need to re-calculate the average profile value
avgprof = (profs / self.proflen).sum()
else:
new_subdelays_bins = Num.floor(delaybins + 0.5)
for jj in range(self.nsub):
profs[jj] = psr_utils.rotate(profs[jj],
int(new_subdelays_bins[jj]))
subdelays_bins += new_subdelays_bins
avgprof = self.avgprof
sumprof = profs.sum(0)
chis[ii] = self.calc_redchi2(prof=sumprof, avg=avgprof)
# Now plot it
Pgplot.plotxy(chis,
DMs,
labx="DM",
laby="Reduced-\gx\u2\d",
device=device)
return (chis, DMs)
def dedisperse(self, DM=None, interp=0, doppler=1):
"""
dedisperse(DM=self.bestdm, interp=0, doppler=1):
Rotate (internally) the profiles so that they are de-dispersed
at a dispersion measure of DM. Use FFT-based interpolation if
'interp' is non-zero (NOTE: It is off by default!).
Doppler shift subband frequencies if doppler is non-zero.
(NOTE: It is *ON* by default. This default behaviour is
different with respect to PRESTO's prepfold.py)
"""
if DM is None:
DM = self.bestdm
# Note: Since TEMPO Doppler corrects observing frequencies, for
# TOAs, at least, we need to de-disperse using topocentric
# observing frequencies.
if doppler:
freqs = psr_utils.doppler(self.subfreqs, self.avgvoverc)
else:
freqs = self.subfreqs
self.subdelays = psr_utils.delay_from_DM(DM, freqs)
self.hifreqdelay = self.subdelays[-1]
self.subdelays = self.subdelays-self.hifreqdelay
delaybins = self.subdelays*self.binspersec - self.subdelays_bins
if interp:
new_subdelays_bins = delaybins
for ii in range(self.npart):
for jj in range(self.nsub):
tmp_prof = self.profs[ii,jj,:]
self.profs[ii,jj] = psr_utils.fft_rotate(tmp_prof, delaybins[jj])
# Note: Since the rotation process slightly changes the values of the
# profs, we need to re-calculate the average profile value
self.avgprof = (self.profs/self.proflen).sum()
else:
new_subdelays_bins = Num.floor(delaybins+0.5)
#print "DEBUG: in myprepfold.py -- DM, new_subdelays_bins:", DM, new_subdelays_bins
for ii in range(self.nsub):
rotbins = int(new_subdelays_bins[ii])%self.proflen
if rotbins: # i.e. if not zero
subdata = self.profs[:,ii,:]
self.profs[:,ii] = Num.concatenate((subdata[:,rotbins:],
subdata[:,:rotbins]), 1)
self.subdelays_bins += new_subdelays_bins
self.sumprof = self.profs.sum(0).sum(0)
if Num.fabs((self.sumprof/self.proflen).sum() - self.avgprof) > 1.0:
print "self.avgprof is not the correct value!"
self.currdm = DM
def plot(data, cmap='gist_yarg', show_cb=False, sweep_dms=None, sweep_posns=None):
if sweep_dms is None:
sweep_dms = []
if sweep_posns is None:
sweep_posns = []
ax = plt.axes((0.15, 0.15, 0.8, 0.7))
plot_spectra(data, cmap=cmap)
if show_cb:
cb = plt.colorbar()
cb.set_label("Scaled signal intensity (arbitrary units)")
plt.axis('tight')
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt*data.numspectra*sweep_posn+data.starttime
sty = SWEEP_STYLES[ii%len(SWEEP_STYLES)]
plt.plot(delays+sweepstart, data.freqs, sty, lw=4, alpha=0.5)
# Dressing it up
plt.xlabel("Time")
plt.ylabel("Observing frequency (MHz)")
#plt.suptitle("Frequency vs. Time")
sumax = plt.axes((0.15, 0.85, 0.8, 0.1), sharex=ax)
plot_timeseries(data)
plt.setp(sumax.get_xticklabels()+sumax.get_yticklabels(), visible=False)
plt.ylabel("Intensity")
plt.ticklabel_format(style='plain', useOffset=False)
plt.axis('tight')
return sumax, ax
def get_phasedelays(dm, freqs, period):
"""Return phase delays corresponding to a particular DM.
Inputs:
dm: DM (in pc cm-3)
freqs: The list of frequencies (in MHz)
period: The profiles period (in seconds)
Outputs:
phasedelays: The corresponding phase delays.
"""
# Prepare delays
timedelays = psr_utils.delay_from_DM(dm, freqs)
# Reference all delays to highest frequency channel, which remains
# unchanged
# TODO: Do we really want to refer to high freq?
timedelays -= timedelays[np.argmax(freqs)]
phasedelays = timedelays/period
return phasedelays
def get_phasedelays(dm, freqs, period):
"""Return phase delays corresponding to a particular DM.
Inputs:
dm: DM (in pc cm-3)
freqs: The list of frequencies (in MHz)
period: The profiles period (in seconds)
Outputs:
phasedelays: The corresponding phase delays.
"""
# Prepare delays
timedelays = psr_utils.delay_from_DM(dm, freqs)
# Reference all delays to highest frequency channel, which remains
# unchanged
# TODO: Do we really want to refer to high freq?
timedelays -= timedelays[np.argmax(freqs)]
phasedelays = timedelays/period
return phasedelays
def main():
fn = args[0]
rawdatafile = open_data_file(fn)
if options.dm:
dmtime = psr_utils.delay_from_DM(options.dm, np.min(rawdatafile.freqs))
data = get_data(rawdatafile, start=options.start, duration=options.duration+dmtime,
mask=options.maskfile)
data = prepare_data(data, options.width_bins, options.downsamp, options.dm,
options.nsub, options.subdm, options.scaleindep)
# Ploting it up
fig = plt.figure()
fig.canvas.set_window_title("Frequency vs. Time")
plot(data, options.cmap, options.sweep_dms, options.sweep_posns)
fig.canvas.mpl_connect('key_press_event', \
lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
plt.show()
def plot_chi2_vs_DM(self, loDM, hiDM, N=100, interp=0, device='/xwin'):
"""
plot_chi2_vs_DM(self, loDM, hiDM, N=100, interp=0, device='/xwin'):
Plot (and return) an array showing the reduced-chi^2 versus
DM (N DMs spanning loDM-hiDM). Use sinc_interpolation
if 'interp' is non-zero.
"""
# Sum the profiles in time
sumprofs = self.profs.sum(0)
if not interp:
profs = sumprofs
else:
profs = Num.zeros(Num.shape(sumprofs), dtype='d')
DMs = psr_utils.span(loDM, hiDM, N)
chis = Num.zeros(N, dtype='f')
subdelays_bins = self.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, self.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays*self.binspersec - subdelays_bins
if interp:
interp_factor = 16
for jj in range(self.nsub):
profs[jj] = psr_utils.interp_rotate(sumprofs[jj], delaybins[jj],
zoomfact=interp_factor)
# Note: Since the interpolation process slightly changes the values of the
# profs, we need to re-calculate the average profile value
avgprof = (profs/self.proflen).sum()
else:
new_subdelays_bins = Num.floor(delaybins+0.5)
for jj in range(self.nsub):
profs[jj] = psr_utils.rotate(profs[jj], int(new_subdelays_bins[jj]))
subdelays_bins += new_subdelays_bins
avgprof = self.avgprof
sumprof = profs.sum(0)
chis[ii] = self.calc_redchi2(prof=sumprof, avg=avgprof)
# Now plot it
Pgplot.plotxy(chis, DMs, labx="DM", laby="Reduced-\gx\u2\d", device=device)
return (chis, DMs)
def main():
fn = args[0]
rawdatafile = open_data_file(fn)
if options.dm:
dmtime = psr_utils.delay_from_DM(options.dm, np.min(rawdatafile.freqs))
data = get_data(rawdatafile,
start=options.start,
duration=options.duration + dmtime,
mask=options.maskfile)
data = prepare_data(data, options.width_bins, options.downsamp, options.dm,
options.nsub, options.subdm, options.scaleindep)
# Ploting it up
fig = plt.figure()
fig.canvas.set_window_title("Frequency vs. Time")
plot(data, options.cmap, options.sweep_dms, options.sweep_posns)
fig.canvas.mpl_connect('key_press_event', \
lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
plt.show()
def make_spd_from_man_params(spdcand, rawdatafile, \
txtfile, maskfile, \
plot, just_waterfall, \
subdm, dm, sweep_dm, \
sigma, \
start_time, duration, \
width_bins, nbins, downsamp, \
nsub, \
scaleindep, \
spec_width, loc_pulse, \
integrate_ts, integrate_spec, disp_pulse, \
basename, \
mask, bandpass_corr, barytime, man_params):
"""
Makes spd files from output files of rratrap.
Inputs:
spdcand: spcand parameters instance (read in spcand.params)
rawdatafile: psrfits file instance
txtfile: rratrap output file (groups.txt file)
maskfile: rfifind mask file. need this file if you want to remove the bandpass
or use rfifind mask information.
plot: do you want to produce the plots as well?
just_waterfall: Do you just want to make the waterfall plots.
subdm: DM to use when subbanding.
dm: DM to use when dedispersing data for plot.
sweep_dm: Show the frequency sweep using this DM.
sigma: signal-to-noise of the pulse
start_time: start time of the data to be read in for waterfalling.
duration: duration of data to be waterfalled.
width_bins: Smooth each channel/subband with a boxcar width_bins wide.
nbins: Number of time bins to plot. This option overrides
the duration argument.
downsamp: Factor to downsample in time by. Default: Don't downsample.
nsub: Number of subbands to use. Must be a factor of number of channels.
scaleindep:Do you want to scale each subband independently?(Type: Boolean)
spec_width: Twice this number times the pulse_width around the pulse to consider for the spectrum
loc_pulse: Fraction of the window length where the pulse is located.(eg. 0.25 = 1/4th of the way in.
0.5 = middle of the plot)
integrate_ts: Do you want to display the dedispersed time series in the plot?
integrate_spec: Do you want to display the pulse spectrum in the plot?
disp_pulse: Do you want to see the inset dispersed pulse in the plot?
basename: output basename of the file. Appended with _DM_TIME(s)_RANK.spd
mask: Do you want to mask out rfi contaminated channels?
bandpass_corr: Do you want to remove the bandpass?
barytime: Is the given time(s) barycentric?
man_params: Do you want to specify the parameters for waterfalling
manually? If yes, I suggest using the function make_spd_from_man_params().
(I suggest giving it the rratrap output file)
Outputs:
Binary npz file containing the necessary arrays and header information to generate the spd plots.
"""
rank = None
if not nsub:
nsub = rawdatafile.nchan
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
spdcand.manual_params(subdm, dm, sweep_dm, sigma, start_time, \
width_bins, downsamp, duration, nbins, nsub, rawdatafile.tsamp, \
rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], rawdatafile, \
loc_pulse=loc_pulse, dedisp=True, scaleindep=False, zerodm=False, \
mask=mask, barytime=barytime, bandpass_corr=bandpass_corr)
#make an array to store header information for the spd files
temp_filename = basename+"_DM%.1f_%.1fs"%(spdcand.subdm, spdcand.topo_start_time)
print_debug("Running waterfaller with Zero-DM OFF...")
data, Data_dedisp_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
# Add additional information to the header information array
text_array = np.array([args[0], rawdatafile.specinfo.telescope, \
rawdatafile.specinfo.ra_str, rawdatafile.specinfo.dec_str, \
rawdatafile.specinfo.start_MJD[0], rank, \
spdcand.nsub, spdcand.nbins, \
spdcand.subdm, spdcand.sigma, spdcand.sample_number, \
spdcand.duration, spdcand.width_bins, spdcand.pulse_width, \
rawdatafile.tsamp, rawdatafile.specinfo.T, spdcand.topo_start_time, \
data.starttime, data.dt,data.numspectra, data.freqs.min(), \
data.freqs.max()])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
zerodm=True
data, Data_dedisp_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
####Sweeped without zerodm
spdcand.manual_params(subdm, dm, sweep_dm, sigma, start_time, \
width_bins, downsamp, duration, nbins, nsub, rawdatafile.tsamp, \
rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], rawdatafile, \
loc_pulse=loc_pulse, dedisp=None, scaleindep=None, zerodm=None, mask=mask, \
barytime=barytime, bandpass_corr=bandpass_corr)
data, Data_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
text_array = np.append(text_array, spdcand.sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, spdcand.bary_start_time)
text_array = np.append(text_array, man_params)
# Array to Construct the sweep
if spdcand.sweep_dm is not None:
ddm = spdcand.sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
#downsamp_temp = 1
data, Data_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
with open(temp_filename+".spd", 'wb') as f:
np.savez_compressed(f, \
Data_dedisp_nozerodm = Data_dedisp_nozerodm.astype(np.float16),\
Data_dedisp_zerodm = Data_dedisp_zerodm.astype(np.float16),\
Data_nozerodm = Data_nozerodm.astype(np.float16),\
delays_nozerodm = delays_nozerodm, \
freqs_nozerodm = freqs_nozerodm,\
Data_zerodm = Data_zerodm.astype(np.float16), \
text_array = text_array)
#### Arrays for Plotting DM vs Time is in plot_spd.plot(...)
if plot:
print_debug("Now plotting...")
plot_spd.plot(temp_filename+".spd", args[1:], \
spec_width=spec_width, loc_pulse=loc_pulse, xwin=False, \
outfile = basename, just_waterfall=just_waterfall, \
integrate_spec=integrate_spec, integrate_ts=integrate_ts, \
disp_pulse=disp_pulse, tar = None)
# Combine the profiles as required
profs = fold_pfd.combine_profs(numtoas, numsubbands)
# PRESTO de-disperses at the high frequency channel so determine a
# correction to the middle of the band
if not events:
subpersumsub = fold_pfd.nsub/numsubbands
# Calculate the center of the summed subband freqs and delays
sumsubfreqs = (Num.arange(numsubbands)+0.5)*subpersumsub*fold_pfd.subdeltafreq + \
(fold_pfd.lofreq-0.5*fold_pfd.chan_wid)
# Note: In the following, we cannot use fold_pfd.hifreqdelay since that
# is based on the _barycentric_ high frequency (if the barycentric
# conversion was available). For TOAs, we need a topocentric
# delay, which is based on the topocentric frequency fold_pfd.hifreq
sumsubdelays = (psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs) -
psr_utils.delay_from_DM(fold_pfd.bestdm, fold_pfd.hifreq))/SECPERDAY
else:
fold_pfd.subfreqs = Num.asarray([0.0])
sumsubfreqs = Num.asarray([0.0])
sumsubdelays = Num.asarray([0.0])
# Read the template profile
if templatefilenm is not None:
template = psr_utils.read_profile(templatefilenm, normalize=1)
else:
if (gaussfitfile):
template = psr_utils.read_gaussfitfile(gaussfitfile, fold_pfd.proflen)
else:
template = psr_utils.gaussian_profile(fold_pfd.proflen, 0.0, gaussianwidth)
template = template / max(template)
# Combine the profiles as required
profs = fold_pfd.combine_profs(numtoas, numsubbands)
# PRESTO de-disperses at the high frequency channel so determine a
# correction to the middle of the band
if not events:
subpersumsub = fold_pfd.nsub/numsubbands
# Calculate the center of the summed subband freqs and delays
sumsubfreqs = (Num.arange(numsubbands)+0.5)*subpersumsub*fold_pfd.subdeltafreq + \
(fold_pfd.lofreq-0.5*fold_pfd.chan_wid)
# Note: In the following, we cannot use fold_pfd.hifreqdelay since that
# is based on the _barycentric_ high frequency (if the barycentric
# conversion was available). For TOAs, we need a topocentric
# delay, which is based on the topocentric frequency fold_pfd.hifreq
sumsubdelays = (psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs) -
psr_utils.delay_from_DM(fold_pfd.bestdm, fold_pfd.hifreq))
sumsubdelays_phs = Num.fmod(sumsubdelays / p_dedisp, 1.0)
# Save the "higest channel within a subband" freqs/delays for use in
# later DM/timing correction. PBD 2011/11/03
sumsubfreqs_hi = sumsubfreqs + \
fold_pfd.subdeltafreq/2.0 - fold_pfd.chan_wid/2.0
subdelays2 = psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs) - \
psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs_hi)
else:
fold_pfd.subfreqs = Num.asarray([0.0])
sumsubfreqs = Num.asarray([0.0])
sumsubdelays = Num.asarray([0.0])
# Read the template profile
def dm_curve_check(self, spec_index=0.):
# Sum the profiles in time
profs = self.pfd.profs.sum(0)
### Generate simulated profiles ###
# prof_avg: median profile value per subint per subband
# Sum over subint axis to get median per subband
prof_avg = self.pfd.stats[:, :, 4].sum(0)
# prof_var: variance of profile per subint per subband
# Sum over subint axis to get variance per subband
prof_var = self.pfd.stats[:, :, 5].sum(0)
# The standard deviation in each subband is proportional to the median
# value of that subband. Here we scale all subbands to equal levels.
#scaled_vars = prof_var / prof_avg**2
scaled_vars = np.array(np.abs(prof_var),
dtype=np.float64) / prof_avg**2
scaled_vars[scaled_vars <= 0] = np.random.rand(
1
) ## This is new, to avoir errors when noise calculates <=0 inside the sqrt
scaled_profs = (profs.T / prof_avg).T - 1.
# The mean profile (after scaling) will be our "clean" profile--hardly
# true in most cases, but we pretend it's noiseless for what follows
scaled_mean_prof = scaled_profs.mean(0)
# Extend this "clean" profile across the number of subbands
sim_profs_clean = np.tile(scaled_mean_prof,\
scaled_profs.shape[0]).reshape(scaled_profs.shape)
# Scale these subbands according to the input spectral index
spec_mult = (self.pfd.subfreqs / self.pfd.subfreqs[0])**spec_index
spec_mult /= spec_mult.mean()
sim_profs_spec = (sim_profs_clean.T * spec_mult).T
# For consistency, set a seed for generating noise
np.random.seed(1967)
# Add white noise that matches the variance of the real subbands
# on a subband by subband basis
noise = np.random.normal(scale=np.sqrt(scaled_vars),
size=scaled_profs.T.shape).T
# sim_profs_noisy is the simulated equivalent of scaled_profs
sim_profs_noisy = sim_profs_spec + noise
# sim_profs_final is the simulated equivalent of profs
sim_profs = ((sim_profs_noisy + 1.).T * prof_avg).T
# The rest of this is essentially code from the prepfold.pfd class
# in which we loop over DM values and see how strong a signal we
# get by dedispersing at each of these values
# Go to higher DMs than the original curve to try to better exclude noise
DMs = np.linspace(self.pfd.dms[0], self.pfd.dms[-1]+4.*\
(self.pfd.dms[-1]-self.pfd.dms[0]), len(self.pfd.dms))
chis = np.zeros_like(DMs)
sim_chis = np.zeros_like(DMs)
subdelays_bins = self.pfd.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, self.pfd.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * self.pfd.binspersec - subdelays_bins
new_subdelays_bins = np.floor(delaybins + 0.5)
for jj in range(self.pfd.nsub):
profs[jj] = psr_utils.rotate(profs[jj],
int(new_subdelays_bins[jj]))
sim_profs[jj] = psr_utils.rotate(sim_profs[jj],\
int(new_subdelays_bins[jj]))
subdelays_bins += new_subdelays_bins
# The set of reduced chi2s like those in the prepfold plot
# (should be the same if the same DMs are used)
chis[ii] = self.pfd.calc_redchi2(prof=profs.sum(0),
avg=self.pfd.avgprof)
# The same thing but for our "simulated" data
sim_chis[ii] = self.pfd.calc_redchi2(prof=sim_profs.sum(0),
avg=self.pfd.avgprof)
return DMs, chis, sim_chis
def write_toa(summed_pulse, polycos, template_profile, \
timeseries, start_phase=0.0, debug=False):
"""Given a SummedPulse generate a TOA and write it to stdout.
A polycos file is required. 'template_profile' is simply
a numpy array. 'timeseries' is a Datfile object.
'start_phase' is the phase at the start of the profile.
'debug' is a boolean value that determines if debugging
info should be displayed.
Returns shift required to line up template and pulse.
"""
if template_profile is None:
raise ValueError("A template profile MUST be provided.")
# This code is taken from Scott Ransom's PRESTO's get_TOAs.py
mjdi = int(summed_pulse.mjd) # integer part of MJD
mjdf = summed_pulse.mjd - mjdi # fractional part of MJD
(phs, freq) = polycos.get_phs_and_freq(mjdi, mjdf)
phs -= start_phase
period = 1.0/freq
# Caclulate offset due to shifting channels to account for DM
# Hifreq doesn't have a half-channel offset
# (why? because get_TOAs.py doesn't. Why...)
# Why subtract 1 channel to get hifreq?
hifreq = timeseries.infdata.lofreq + timeseries.infdata.BW - \
timeseries.infdata.chan_width
midfreq = timeseries.infdata.lofreq - 0.5*timeseries.infdata.chan_width + \
0.5*timeseries.infdata.BW
dmdelay = psr_utils.delay_from_DM(timeseries.infdata.DM, midfreq) - \
psr_utils.delay_from_DM(timeseries.infdata.DM, hifreq)
dmdelay_mjd = dmdelay/float(psr_utils.SECPERDAY)
if debug:
colour.cprint("High frequency (MHz): %f" % hifreq, 'debug')
colour.cprint("Mid frequency (MHz): %f" % midfreq, 'debug')
colour.cprint("DM delay added to TOAs (s): %g" % dmdelay, 'debug')
colour.cprint("DM delay added to TOAs (MJD): %g" % dmdelay_mjd, 'debug')
t0f = mjdf - phs*period/psr_utils.SECPERDAY + dmdelay_mjd
t0i = mjdi
shift,eshift,snr,esnr,b,errb,ngood,tphs = measure_phase(summed_pulse.profile, \
template_profile)
# tphs is amount template is rotated by. It is originally
# measured in radians, convert to rotational phase
tphs = tphs/(np.pi*2.0) % 1.0
# tau and tau_err are the predicted phase of the pulse arrival
tau, tau_err = shift/summed_pulse.N, eshift/summed_pulse.N
if debug:
colour.cprint("FFTFIT: Shift (bins): %f, Tau (phase): %f" % (shift, tau), 'debug')
colour.cprint("FFTFIT: Shift error (bins): %f, Tau error (phase): %f" % \
(eshift, tau_err), 'debug')
# Note: "error" flags are shift = 0.0 and eshift = 999.0
if (np.fabs(shift) < 1e-7 and np.fabs(eshift-999.0) < 1e-7):
raise FFTFitError("Error in FFTFIT. Bad return values.")
# Send the TOA to STDOUT
toaf = t0f + tau*period/float(psr_utils.SECPERDAY)
if debug:
colour.cprint("t0f (MJD): %r" % t0f, 'debug')
colour.cprint("period (s): %r" % period, 'debug')
colour.cprint("toaf (MJD): %r" % toaf, 'debug')
newdays = int(np.floor(toaf))
obs_code = telescopes.telescope_to_id[timeseries.infdata.telescope]
psr_utils.write_princeton_toa(t0i+newdays, toaf-newdays, \
tau_err*period*1e6, midfreq, \
timeseries.infdata.DM, obs=obs_code)
return tau, tphs
def plot_waterfall(data,
start,
duration,
dm,
ofile,
integrate_ts=False,
integrate_spec=False,
show_cb=False,
cmap_str="gist_yarg",
sweep_dms=[],
sweep_posns=[],
ax_im=None,
ax_ts=None,
ax_spec=None,
interactive=True,
downsamp=1,
nsub=None,
subdm=None):
""" I want a docstring too!
"""
# Set up axes
fig = plt.figure(figsize=(8, 12))
#fig.canvas.set_window_title("Frequency vs. Time")
'''
im_width = 0.6 if integrate_spec else 0.8
im_height = 0.6 if integrate_ts else 0.8
if not ax_im:
ax_im = plt.axes((0.15, 0.15, im_width, im_height))
if integrate_ts and not ax_ts:
ax_ts = plt.axes((0.15, 0.75, im_width, 0.2),sharex=ax_im)
if integrate_spec and not ax_spec:
ax_spec = plt.axes((0.75, 0.15, 0.2, im_height),sharey=ax_im)
'''
ax_ts = plt.axes((0.15, 0.76, 0.8, 0.19))
ax_im = plt.axes((0.15, 0.455, 0.8, 0.29), sharex=ax_ts)
ax_dmvstm = plt.axes((0.15, 0.15, 0.8, 0.29))
# Ploting it up
nbinlim = np.int(duration / data.dt)
# DM-vs-time plot
dmvstm_array = []
lodm = int(dm - (dm * 0.15))
if lodm < 0: lodm = 0
hidm = int(dm + (dm * 0.15))
dmstep = (hidm - lodm) / 50.0
datacopy = copy.deepcopy(data)
#print lodm,hidm
for ii in np.arange(lodm, hidm, dmstep):
#for ii in range(400,600,10):
#Without this, dispersion delay with smaller DM step does not produce delay close to bin width
data.dedisperse(0, padval='mean')
data.dedisperse(ii, padval='mean')
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
dmvstm_array.append(Dedisp_ts)
dmvstm_array = np.array(dmvstm_array)
#print np.shape(dmvstm_array)
#np.save('dmvstm_1step.npz',dmvstm_array)
ax_dmvstm.set_xlabel("Time")
ax_dmvstm.set_ylabel("DM")
ax_dmvstm.imshow(dmvstm_array,
aspect='auto',
cmap=matplotlib.cm.cmap_d[cmap_str],
origin='lower',
extent=(data.starttime,
data.starttime + nbinlim * data.dt, lodm, hidm))
#cmap=matplotlib.cm.cmap_d[cmap_str])
#interpolation='nearest', origin='upper')
plt.setp(ax_im.get_xticklabels(), visible=False)
plt.setp(ax_ts.get_xticklabels(), visible=False)
#extent=(data.starttime, data.starttime+ nbinlim*data.dt, 500, 700)
#plt.show()
#fig2 = plt.figure(2)
#plt.imshow(dmvstm_array,aspect='auto')
data = copy.deepcopy(datacopy)
data.downsample(downsamp)
data.dedisperse(dm)
nbinlim = np.int(duration / data.dt)
#Freq-vs-time plot
img = ax_im.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
if show_cb:
cb = ax_im.get_figure().colorbar(img)
cb.set_label("Scaled signal intensity (arbitrary units)")
#plt.axis('tight')
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt * data.numspectra * sweep_posn + data.starttime
sty = SWEEP_STYLES[ii % len(SWEEP_STYLES)]
ax_im.plot(delays + sweepstart, data.freqs, sty, lw=4, alpha=0.5)
# Dressing it up
ax_im.xaxis.get_major_formatter().set_useOffset(False)
#ax_im.set_xlabel("Time")
ax_im.set_ylabel("Frequency (MHz)")
# Plot Time series
if integrate_ts:
#Data = np.array(data.data[..., :nbinlim])
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data.numspectra) * data.dt + start)[..., :nbinlim]
ax_ts.plot(times, Dedisp_ts, "k")
ax_ts.set_xlim([times.min(), times.max()])
plt.setp(ax_ts.get_xticklabels(), visible=False)
plt.setp(ax_ts.get_yticklabels(), visible=False)
# Plot Spectrum
if integrate_spec:
spectrum_window = 0.05 * duration
window_width = int(spectrum_window / data.dt) # bins
burst_bin = nbinlim / 2
on_spec = np.array(data.data[..., burst_bin - window_width:burst_bin +
window_width])
Dedisp_spec = on_spec.sum(axis=1)[::-1]
freqs = np.linspace(data.freqs.min(), data.freqs.max(),
len(Dedisp_spec))
ax_spec.plot(Dedisp_spec, freqs, "k")
plt.setp(ax_spec.get_xticklabels(), visible=False)
plt.setp(ax_spec.get_yticklabels(), visible=False)
ax_spec.set_ylim([data.freqs.min(), data.freqs.max()])
if integrate_ts:
ax_ts.axvline(times[burst_bin] - spectrum_window,
ls="--",
c="grey")
ax_ts.axvline(times[burst_bin] + spectrum_window,
ls="--",
c="grey")
#if interactive:
# fig.suptitle("Frequency vs. Time")
# fig.canvas.mpl_connect('key_press_event', \
# lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
#oname = "%.3f_%s.png" % (start,str(dm))
if ofile is "unknown_cand":
ofile = ofile + "_%.3f_%s.pdf" % (start, str(dm))
plt.savefig(ofile)
else:
plt.savefig(ofile)
def main():
fn = args[0]
#if fn.endswith(".fil"):
# # Filterbank file
# filetype = "filterbank"
# rawdatafile = filterbank.filterbank(fn)
if fn.endswith(".fits"):
# PSRFITS file
filetype = "psrfits"
rawdatafile = psrfits.PsrfitsFile(fn)
else:
raise ValueError("Cannot recognize data file type from "
"extension. (Only '.fits' and '.fil' "
"are supported.)")
# Read data
start_bin = np.round(options.start/rawdatafile.tsamp).astype('int')
#dmfac = 4.15e3 * np.abs(1./rawdatafile.fch1**2 - 1./(rawdatafile.frequencies[-1])**2)
dmfac = 4.15e3 * np.abs(1./rawdatafile.frequencies[0]**2 - 1./rawdatafile.frequencies[-1]**2)
if options.nbins is None:
nbins = np.round(options.duration/rawdatafile.tsamp).astype('int')
else:
nbins = options.nbins
binratio = 50
if options.dm:
nbinsextra = np.round((options.duration + dmfac * options.dm)/rawdatafile.tsamp).astype('int')
else:
nbinsextra = nbins
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskfile(data, start_bin, nbinsextra)
data, bins = waterfall(start_bin, dmfac, options.duration, nbins, options.zerodm, options.nsub, options.subdm, options.dm, options.integrate_dm, options.downsamp, options.scaleindep, options.width_bins, rawdatafile, binratio, data)
# Ploting it up
fig = plt.figure()
fig.canvas.set_window_title("Frequency vs. Time")
ax = plt.axes((0.15, 0.15, 0.8, 0.60))
ragfac = float(nbins)/bins
dmrange, trange = data.data.shape
nbinlim = np.int(trange * ragfac)
print data.dt, rawdatafile.tsamp
#np.save('data',data.data[..., :nbinlim])
plt.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[options.cmap], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
if options.show_cb:
cb = plt.colorbar()
cb.set_label("Scaled signal intensity (arbitrary units)")
#plt.axis('tight')
# Sweeping it up
for ii, sweep_dm in enumerate(options.sweep_dms):
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if options.sweep_posns is None:
sweep_posn = 0.0
elif len(options.sweep_posns) == 1:
sweep_posn = options.sweep_posns[0]
else:
sweep_posn = options.sweep_posns[ii]
sweepstart = data.dt*data.numspectra*sweep_posn+data.starttime
sty = SWEEP_STYLES[ii%len(SWEEP_STYLES)]
plt.plot(delays+sweepstart, data.freqs, sty, lw=4, alpha=0.5)
# Dressing it up
plt.xlabel("Time")
plt.ylabel("Observing frequency (MHz)")
plt.suptitle("Frequency vs. Time")
# Plot Time series
if options.integrate_dm is not None:
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data.numspectra)*data.dt + options.start)[..., :nbinlim]
ax = plt.axes((0.15, 0.75, 0.8, 0.2))
plt.plot(times, Dedisp_ts)
plt.setp(ax.get_xticklabels(), visible = False)
plt.setp(ax.get_yticklabels(), visible = False)
fig.canvas.mpl_connect('key_press_event', \
lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
plt.show()
def calc_features_from_pfd(pfd_filepath):
pfd_data = prepfold.pfd(str(pfd_filepath))
if pfd_filepath.parent.name == 'positive':
label = 1
elif pfd_filepath.parent.name == 'negative':
label = 0
else:
label = -1
# raise RuntimeError('unable to decide the label of pfd file: {}'.format(
# str(pfd_filepath)))
pfd_data.dedisperse()
#### As done in: prepfold.pfd.plot_sumprofs
profile = pfd_data.sumprof
profile = normalise_1d(profile)
####
profile_mean = np.mean(profile)
profile_std_dev = np.std(profile)
profile_skewness = scipy.stats.skew(profile)
profile_excess_kurtosis = scipy.stats.kurtosis(profile)
profiles_sum_axis0 = pfd_data.profs.sum(0)
#### As done in: prepfold.pfd.plot_chi2_vs_DM
loDM = 0
hiDM = pfd_data.numdms
N = pfd_data.numdms
profs = profiles_sum_axis0.copy() # = pfd_data.profs.sum(0)
DMs = psr_utils.span(loDM, hiDM, N)
chis = np.zeros(N, dtype='f')
subdelays_bins = pfd_data.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, pfd_data.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * pfd_data.binspersec - subdelays_bins
new_subdelays_bins = np.floor(delaybins + 0.5)
for jj in range(pfd_data.nsub):
profs[jj] = psr_utils.rotate(profs[jj],
int(new_subdelays_bins[jj]))
subdelays_bins += new_subdelays_bins
sumprof = profs.sum(0)
chis[ii] = pfd_data.calc_redchi2(prof=sumprof, avg=pfd_data.avgprof)
####
best_dm = pfd_data.bestdm
# crop_radius = 100
# best_dm_index = np.searchsorted(DMs, best_dm) # Not accurate, but close.
# bloated_chis = np.insert(chis, N, np.full(crop_radius, chis[-1]))
# bloated_chis = np.insert(bloated_chis, 0, np.full(crop_radius, chis[0]))
# cropped_chis = bloated_chis[ best_dm_index : best_dm_index+2*crop_radius ]
# chis = cropped_chis
chis_mean = np.mean(chis)
chis_std_dev = np.std(chis)
chis_skewness = scipy.stats.skew(chis)
chis_excess_kurtosis = scipy.stats.kurtosis(chis)
#### As done in: prepfold.pfd.plot_intervals
intervals = pfd_data.profs.sum(1)
intervals = normalise_2d_rowwise(intervals)
####
#### As done in: prepfold.pfd.plot_subbands
subbands = profiles_sum_axis0.copy() # = pfd_data.profs.sum(0)
subbands = normalise_2d_rowwise(subbands)
####
return (label, profile_mean, profile_std_dev, profile_skewness,
profile_excess_kurtosis, chis_mean, chis_std_dev, chis_skewness,
chis_excess_kurtosis, best_dm, profile, intervals, subbands, chis)
def plot_waterfall(data,
start,
source_name,
duration,
dm,
ofile,
integrate_ts=False,
integrate_spec=False,
show_cb=False,
cmap_str="gist_yarg",
sweep_dms=[],
sweep_posns=[],
ax_im=None,
ax_ts=None,
ax_spec=None,
interactive=True,
downsamp=1,
nsub=None,
subdm=None,
width=None,
snr=None):
""" I want a docstring too!
"""
if source_name is None:
source_name = "Unknown"
#Output file
if ofile is "unknown_cand":
title = "%s_" + ofile + "_%.3f_%s" % (source_name, start, str(dm))
else:
title = source_name + "_" + ofile
# Set up axes
fig = plt.figure(figsize=(10, 14))
#fig.canvas.set_window_title("Frequency vs. Time")
'''
im_width = 0.6 if integrate_spec else 0.8
im_height = 0.6 if integrate_ts else 0.8
if not ax_im:
ax_im = plt.axes((0.15, 0.15, im_width, im_height))
if integrate_ts and not ax_ts:
ax_ts = plt.axes((0.15, 0.75, im_width, 0.2),sharex=ax_im)
if integrate_spec and not ax_spec:
ax_spec = plt.axes((0.75, 0.15, 0.2, im_height),sharey=ax_im)
'''
ax_ts = plt.axes((0.1, 0.835, 0.71, 0.145))
ax_im = plt.axes((0.1, 0.59, 0.71, 0.24), sharex=ax_ts)
ax_dmvstm = plt.axes((0.1, 0.345, 0.71, 0.24), sharex=ax_ts)
ax_spec = plt.axes((0.815, 0.59, 0.16, 0.24), sharey=ax_im)
ax_dmsnr = plt.axes((0.815, 0.345, 0.16, 0.24), sharey=ax_dmvstm)
ax_orig = plt.axes((0.1, 0.1, 0.71, 0.21))
data.downsample(downsamp)
nbinlim = np.int(duration / data.dt)
# DM-vs-time plot
dmvstm_array = []
#Old way
'''
lodm = int(dm-(dm*0.15))
if lodm < 0: lodm = 0
hidm = int(dm+(dm*0.15))
'''
band = (data.freqs.max() - data.freqs.min())
centFreq = (data.freqs.min() + band / 2.0) / (10**3) # To get it in GHz
print width, centFreq, band
#This comes from Cordes and McLaughlin (2003) Equation 13.
FWHM_DM = 506 * float(width) * pow(centFreq, 3) / band
#The candidate DM might not be exact so using a longer range
FWHM_DM = 3 * FWHM_DM
lodm = dm - FWHM_DM
if lodm < 0:
lodm = 0
hidm = 2 * dm # If low DM is zero then range should be 0 to 2*DM
else:
hidm = dm + FWHM_DM
print FWHM_DM, dm, lodm, hidm
dmstep = (hidm - lodm) / 48.0
datacopy = copy.deepcopy(data)
#print lodm,hidm
for ii in np.arange(lodm, hidm, dmstep):
#for ii in range(400,600,10):
#Without this, dispersion delay with smaller DM step does not produce delay close to bin width
data.dedisperse(0, padval='rotate')
data.dedisperse(ii, padval='rotate')
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
dmvstm_array.append(Dedisp_ts)
dmvstm_array = np.array(dmvstm_array)
#print np.shape(dmvstm_array)
#np.save('dmvstm_1step.npz',dmvstm_array)
ax_dmvstm.set_xlabel("Time (sec) ")
ax_dmvstm.set_ylabel("DM")
#ax_dmvstm.imshow(dmvstm_array, aspect='auto', cmap=matplotlib.cm.cmap_d[cmap_str], origin='lower',extent=(data.starttime, data.starttime+ nbinlim*data.dt, lodm, hidm))
ax_dmvstm.imshow(dmvstm_array,
aspect='auto',
origin='lower',
extent=(data.starttime,
data.starttime + nbinlim * data.dt, lodm, hidm))
#cmap=matplotlib.cm.cmap_d[cmap_str])
#interpolation='nearest', origin='upper')
plt.setp(ax_im.get_xticklabels(), visible=False)
plt.setp(ax_ts.get_xticklabels(), visible=False)
ax_dmvstm.set_ylim(lodm, hidm)
#extent=(data.starttime, data.starttime+ nbinlim*data.dt, 500, 700)
#plt.show()
#fig2 = plt.figure(2)
#plt.imshow(dmvstm_array,aspect='auto')
#Plot Freq-vs-time
data = copy.deepcopy(datacopy)
#data.downsample(downsamp)
data.dedisperse(dm, padval='rotate')
nbinlim = np.int(duration / data.dt)
img = ax_im.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
#ax_im.axvline(x=(data.starttime + nbinlim*data.dt)/2.0,ymin=data.freqs.min(),ymax=data.freqs.max(),lw=3,color='b')
if show_cb:
cb = ax_im.get_figure().colorbar(img)
cb.set_label("Scaled signal intensity (arbitrary units)")
# Dressing it up
ax_im.xaxis.get_major_formatter().set_useOffset(False)
#ax_im.set_xlabel("Time")
ax_im.set_ylabel("Frequency (MHz)")
# Plot Time series
#Data = np.array(data.data[..., :nbinlim])
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data.numspectra) * data.dt + start)[..., :nbinlim]
ax_ts.plot(times, Dedisp_ts, "k")
ax_ts.set_xlim([times.min(), times.max()])
text1 = "DM: " + "%.2f" % float(data.dm)
plt.text(1.1,
0.9,
text1,
fontsize=15,
ha='center',
va='center',
transform=ax_ts.transAxes)
text2 = "Width: " + "%.2f" % float(width)
plt.text(1.1,
0.75,
text2,
fontsize=15,
ha='center',
va='center',
transform=ax_ts.transAxes)
text3 = "SNR: " + "%.2f" % float(snr)
plt.text(1.1,
0.6,
text3,
fontsize=15,
ha='center',
va='center',
transform=ax_ts.transAxes)
ax_ts.set_title(title, fontsize=14)
plt.setp(ax_ts.get_xticklabels(), visible=False)
plt.setp(ax_ts.get_yticklabels(), visible=False)
#Spectrum and DM-vs-SNR plot
#Get window
spectrum_window = 0.02 * duration
window_width = int(spectrum_window / data.dt) # bins
burst_bin = nbinlim / 2
ax_ts.axvline(times[burst_bin] - spectrum_window, ls="--", c="grey")
ax_ts.axvline(times[burst_bin] + spectrum_window, ls="--", c="grey")
#Get spectrum and DM-vs-SNR for the on-pulse window
on_spec = np.array(data.data[..., burst_bin - window_width:burst_bin +
window_width])
on_dmsnr = np.array(dmvstm_array[..., burst_bin - window_width:burst_bin +
window_width])
Dedisp_spec = np.mean(on_spec, axis=1)
Dedisp_dmsnr = np.mean(on_dmsnr, axis=1)
#Get off-pulse and DM-vs-SNR for range outside on-pulse window
off_spec1 = np.array(data.data[..., 0:burst_bin - window_width])
off_spec = np.mean(off_spec1, axis=1)
off_dmsnr1 = np.array(dmvstm_array[..., 0:burst_bin - window_width])
off_dmsnr = np.mean(off_dmsnr1, axis=1)
#Get Y-axis for both plots
dms = np.linspace(lodm, hidm, len(Dedisp_dmsnr))
freqs = np.linspace(data.freqs.max(), data.freqs.min(), len(Dedisp_spec))
#Spectrum plot
ax_spec.plot(Dedisp_spec, freqs, color="red", lw=2)
ax_spec.plot(off_spec, freqs, color="grey", alpha=0.5, lw=1)
ttest = float(stats.ttest_ind(Dedisp_spec, off_spec)[0].tolist())
ttestprob = float(stats.ttest_ind(Dedisp_spec, off_spec)[1].tolist())
text3 = "t-test"
plt.text(1.1,
0.45,
text3,
fontsize=12,
ha='center',
va='center',
transform=ax_ts.transAxes)
text4 = " %.2f" % (ttest) + "(%.2f" % ((1 - ttestprob) * 100) + "%)"
plt.text(1.1,
0.3,
text4,
fontsize=12,
ha='center',
va='center',
transform=ax_ts.transAxes)
#DMvsSNR plot
ax_dmsnr.plot(Dedisp_dmsnr, dms, color="red", lw=2)
ax_dmsnr.plot(off_dmsnr, dms, color="grey", alpha=0.5, lw=1)
Dedisp_dmsnr_split = np.array_split(Dedisp_dmsnr, 3)
#Sub-array could be different sizes that's why
Dedisp_dmsnr_split[0] = Dedisp_dmsnr_split[0].sum()
Dedisp_dmsnr_split[1] = Dedisp_dmsnr_split[1].sum()
Dedisp_dmsnr_split[2] = Dedisp_dmsnr_split[2].sum()
#Plot settings
plt.setp(ax_spec.get_xticklabels(), visible=True)
plt.setp(ax_dmsnr.get_xticklabels(), visible=False)
plt.setp(ax_spec.get_yticklabels(), visible=False)
plt.setp(ax_dmsnr.get_yticklabels(), visible=False)
ax_spec.set_ylim([data.freqs.min(), data.freqs.max()])
ax_dmsnr.set_ylim(lodm, hidm)
#Plot original data
data.dedisperse(0, padval='rotate')
ax_im.set_ylabel("Frequency (MHz)")
ax_orig.set_ylabel("Frequency (MHz)")
ax_orig.set_xlabel("Time (sec)")
FTdirection = source_name.split("_")[0]
if FTdirection == 'nT':
ndata = data.data[..., ::-1]
print "Will be flipped in Time"
elif FTdirection == 'nF':
ndata = data.data[::-1, ...]
print "Will be flipped in freq"
elif FTdirection == 'nTnF':
ndata = data.data[::-1, ::-1]
print "Will be flipped in time and freq"
else:
ndata = data.data
print "No flip"
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm - data.dm
#delays = psr_utils.delay_from_DM(ddm, data.freqs)
#delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt * data.numspectra * sweep_posn + data.starttime
#sweepstart = data.dt*data.numspectra + data.starttime
sty = "b-"
if FTdirection == 'nT':
ddm = (-1) * ddm # Negative DM
nfreqs = data.freqs
elif FTdirection == 'nF':
nfreqs = data.freqs[::-1]
elif FTdirection == 'nTnF':
ddm = (-1) * ddm # Negative DM
nfreqs = data.freqs[::-1]
else:
nfreqs = data.freqs
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
ndelay = (delays + sweepstart)
ndelay2 = (delays + sweepstart + duration)
ax_orig.set_xlim(data.starttime,
data.starttime + len(data.data[0]) * data.dt)
ax_orig.set_ylim(data.freqs.min(), data.freqs.max())
ax_orig.plot(ndelay, nfreqs, "b-", lw=2, alpha=0.7)
ax_orig.plot(ndelay2, nfreqs, "b-", lw=2, alpha=0.7)
ax_orig.imshow(ndata, aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime + len(data.data[0])*data.dt, \
data.freqs.min(), data.freqs.max()))
#if interactive:
# fig.suptitle("Frequency vs. Time")
# fig.canvas.mpl_connect('key_press_event', \
# lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
#oname = "%.3f_%s.png" % (start,str(dm))
if ofile is "unknown_cand":
ofile = ofile + "_%.3f_%s.png" % (start, str(dm))
if ttest > 2 and Dedisp_dmsnr_split[1] > Dedisp_dmsnr_split[
0] and Dedisp_dmsnr_split[1] > Dedisp_dmsnr_split[2]:
ofile = "A_" + ofile #If t-test good then put those candidate first
plt.text(1.1,
0.2,
"cat: A",
fontsize=12,
ha='center',
va='center',
transform=ax_ts.transAxes)
if ttest <= 2 and ttest > 1 and Dedisp_dmsnr_split[1] > Dedisp_dmsnr_split[
0] and Dedisp_dmsnr_split[1] > Dedisp_dmsnr_split[2]:
ofile = "B_" + ofile
plt.text(1.1,
0.2,
"cat: B",
fontsize=12,
ha='center',
va='center',
transform=ax_ts.transAxes)
if ttest <= 1 and Dedisp_dmsnr_split[1] > Dedisp_dmsnr_split[
0] and Dedisp_dmsnr_split[1] > Dedisp_dmsnr_split[2]:
plt.text(1.1,
0.2,
"cat: C",
fontsize=12,
ha='center',
va='center',
transform=ax_ts.transAxes)
ofile = "C_" + ofile
plt.savefig(ofile)
def dm_curve_check(self, spec_index=0.0):
# Sum the profiles in time
profs = self.pfd.profs.sum(0)
### Generate simulated profiles ###
# prof_avg: median profile value per subint per subband
# Sum over subint axis to get median per subband
prof_avg = self.pfd.stats[:, :, 4].sum(0)
# prof_var: variance of profile per subint per subband
# Sum over subint axis to get variance per subband
prof_var = self.pfd.stats[:, :, 5].sum(0)
# The standard deviation in each subband is proportional to the median
# value of that subband. Here we scale all subbands to equal levels.
scaled_vars = prof_var / prof_avg ** 2
scaled_profs = (profs.T / prof_avg).T - 1.0
# The mean profile (after scaling) will be our "clean" profile--hardly
# true in most cases, but we pretend it's noiseless for what follows
scaled_mean_prof = scaled_profs.mean(0)
# Extend this "clean" profile across the number of subbands
sim_profs_clean = np.tile(scaled_mean_prof, scaled_profs.shape[0]).reshape(scaled_profs.shape)
# Scale these subbands according to the input spectral index
spec_mult = (self.pfd.subfreqs / self.pfd.subfreqs[0]) ** spec_index
spec_mult /= spec_mult.mean()
sim_profs_spec = (sim_profs_clean.T * spec_mult).T
# For consistency, set a seed for generating noise
np.random.seed(1967)
# Add white noise that matches the variance of the real subbands
# on a subband by subband basis
noise = np.random.normal(scale=np.sqrt(scaled_vars), size=scaled_profs.T.shape).T
# sim_profs_noisy is the simulated equivalent of scaled_profs
sim_profs_noisy = sim_profs_spec + noise
# sim_profs_final is the simulated equivalent of profs
sim_profs = ((sim_profs_noisy + 1.0).T * prof_avg).T
# The rest of this is essentially code from the prepfold.pfd class
# in which we loop over DM values and see how strong a signal we
# get by dedispersing at each of these values
# Go to higher DMs than the original curve to try to better exclude noise
DMs = np.linspace(
self.pfd.dms[0], self.pfd.dms[-1] + 4.0 * (self.pfd.dms[-1] - self.pfd.dms[0]), len(self.pfd.dms)
)
chis = np.zeros_like(DMs)
sim_chis = np.zeros_like(DMs)
subdelays_bins = self.pfd.subdelays_bins.copy()
for ii, DM in enumerate(DMs):
subdelays = psr_utils.delay_from_DM(DM, self.pfd.barysubfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * self.pfd.binspersec - subdelays_bins
new_subdelays_bins = np.floor(delaybins + 0.5)
for jj in range(self.pfd.nsub):
profs[jj] = psr_utils.rotate(profs[jj], int(new_subdelays_bins[jj]))
sim_profs[jj] = psr_utils.rotate(sim_profs[jj], int(new_subdelays_bins[jj]))
subdelays_bins += new_subdelays_bins
# The set of reduced chi2s like those in the prepfold plot
# (should be the same if the same DMs are used)
chis[ii] = self.pfd.calc_redchi2(prof=profs.sum(0), avg=self.pfd.avgprof)
# The same thing but for our "simulated" data
sim_chis[ii] = self.pfd.calc_redchi2(prof=sim_profs.sum(0), avg=self.pfd.avgprof)
return DMs, chis, sim_chis
def main():
filfns = args # addtional argument is fileterbank files
if options.debug:
print "Input filterbank files:", filfns
obs = fbobs.fbobs(filfns)
# filfile.print_header()
obslen = obs.obslen
# Determine start and end of interval (in seconds and samples)
if options.start < 0:
options.start = 0
if (options.end is None) or (options.end > obslen):
# set to end of filterbank file
options.end = obslen
reqstartsamp = int(options.start / obs.tsamp) # requested
# Round down to a multiple of downsamp bins
reqstartsamp = reqstartsamp - (reqstartsamp % options.downsamp)
# Get extra bins for smoothing
startsamp = reqstartsamp - options.width*options.downsamp
reqendsamp = int(options.end / obs.tsamp) # requested
# Round up to a multiple of downsamp bins
reqendsamp = reqendsamp - (reqendsamp % options.downsamp) + options.downsamp
# Get extra bins for smoothing
endsamp = reqendsamp + options.width*options.downsamp
if options.dm:
# Get extra bins for dedispersion
# Compute DM delays
delay_seconds = psr_utils.delay_from_DM(options.dm, obs.frequencies)
delay_seconds -= np.min(delay_seconds)
delay_samples = delay_seconds/(options.downsamp*obs.tsamp)
maxsamps = np.max(delay_samples*options.downsamp)
maxsamps = int(np.round(float(maxsamps)/options.downsamp))*options.downsamp
endsamp += maxsamps
reqnumsaps = reqendsamp - reqstartsamp
numsamps = endsamp - startsamp
if options.debug:
print "Requested start time: %s s (%d samples)" % \
(options.start, reqstartsamp)
print "Actual start time: %s s (%d samples)" % \
(startsamp*obs.tsamp, startsamp)
print "Requested end time: %s s (%d samples)" % \
(options.end, reqendsamp)
print "Actual end time: %s s (%d samples)" % \
(endsamp*obs.tsamp, endsamp)
# read data
data = obs.get_sample_interval(startsamp, endsamp).astype('float32')
obs.close_all()
data.shape = (numsamps, obs.nchans)
if options.mask is not None:
if options.debug:
print "Masking channels using %s" % options.mask
# Mask channels
mask = rfifind.rfifind(options.mask)
maskchans = mask.mask_zap_chans
maskchans = obs.nchans - 1 - np.array(list(maskchans))
data = mask_channels(data, maskchans)
# Modify data
if options.downsamp > 1:
if options.debug:
print "Downsampling by %d bins" % options.downsamp
data = downsample(data, factor=options.downsamp)
if options.width > 1:
if options.debug:
print "Smoothing with boxcar %d bins wide" % options.width
data = smooth(data, factor=options.width)[options.width:-options.width,:]
startsamp += options.width*options.downsamp
endsamp -= options.width*options.downsamp
# plot data as an image
fig = plt.figure()
fig.canvas.set_window_title("Frequency vs. Time")
ax = plt.axes((0.15, 0.15, 0.8, 0.7))
data_scaled = scale(data, indep=options.scaleindep)
data_scaled = data_scaled[:-maxsamps/options.downsamp]
endsamp -= maxsamps
plt.imshow(data_scaled.transpose(), \
aspect='auto', cmap=matplotlib.cm.binary, interpolation='nearest', \
extent=(startsamp/options.downsamp, endsamp/options.downsamp, \
obs.frequencies[-1], obs.frequencies[0]))
plt.xlabel("Sample")
plt.ylabel("Observing frequency (MHz)")
plt.suptitle("Frequency vs. Time")
fig.text(0.05, 0.02, \
r"Start time: $\sim$ %s s, End time: $\sim$ %s s; " \
"Downsampled: %d bins, Smoothed: %d bins; " \
"DM trace: %g $cm^{-3}pc$" % \
(options.start, options.end, options.downsamp, \
options.width, options.dm), \
ha="left", va="center", size="x-small")
if options.dm is not None:
xlim = plt.xlim()
ylim = plt.ylim()
# Plot dispersion delay trace
plt.plot(startsamp/options.downsamp+delay_samples, obs.frequencies, \
'r-', lw=5, alpha=0.25)
plt.xlim(xlim)
plt.ylim(ylim)
profax = plt.axes((0.15, 0.85, 0.8, 0.1), sharex=ax)
dedisp_prof = dedisperse(data, delay_samples)[:-maxsamps/options.downsamp]
plt.plot(np.linspace(xlim[0],xlim[1],dedisp_prof.size), dedisp_prof, 'k-')
plt.setp(profax.xaxis.get_ticklabels(), visible=False)
plt.setp(profax.yaxis.get_ticklabels(), visible=False)
plt.xlim(xlim)
fig.canvas.mpl_connect('key_press_event', keypress)
plt.show()
# Combine the profiles as required
profs = fold_pfd.combine_profs(numtoas, numsubbands)
# PRESTO de-disperses at the high frequency channel so determine a
# correction to the middle of the band
if not events:
subpersumsub = fold_pfd.nsub / numsubbands
# Calculate the center of the summed subband freqs and delays
sumsubfreqs = (Num.arange(numsubbands)+0.5)*subpersumsub*fold_pfd.subdeltafreq + \
(fold_pfd.lofreq-0.5*fold_pfd.chan_wid)
# Note: In the following, we cannot use fold_pfd.hifreqdelay since that
# is based on the _barycentric_ high frequency (if the barycentric
# conversion was available). For TOAs, we need a topocentric
# delay, which is based on the topocentric frequency fold_pfd.hifreq
sumsubdelays = (psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs) -
psr_utils.delay_from_DM(fold_pfd.bestdm,
fold_pfd.hifreq)) / SECPERDAY
else:
fold_pfd.subfreqs = Num.asarray([0.0])
sumsubfreqs = Num.asarray([0.0])
sumsubdelays = Num.asarray([0.0])
# Read the template profile
if templatefilenm is not None:
template = psr_utils.read_profile(templatefilenm, normalize=1)
else:
if (gaussfitfile):
template = psr_utils.read_gaussfitfile(gaussfitfile,
fold_pfd.proflen)
else:
def make_spd_from_file(spdcand, rawdatafile, \
txtfile, maskfile, \
min_rank, group_rank, \
plot, just_waterfall, \
integrate_ts, integrate_spec, disp_pulse, \
loc_pulse, nsub, \
maxnumcands, \
basename, \
mask=False, bandpass_corr=True, barytime=True, \
man_params=None):
"""
Makes spd files from output files of rratrap.
Inputs:
spdcand: spcand parameters instance (read in spcand.params)
rawdatafile: psrfits file instance
txtfile: rratrap output file (groups.txt file)
maskfile: rfifind mask file. need this file if you want to remove the bandpass
or use rfifind mask information.
min_rank: plot all groups with rank more than this. min 1, max 6
group_rank: plot groups ranked whatever you specify
plot: do you want to produce the plots as well?
just_waterfall: Do you just want to make the waterfall plots.
integrate_ts: Do you want to display the dedispersed time series in the plot?
integrate_spec: Do you want to display the pulse spectrum in the plot?
disp_pulse: Do you want to see the inset dispersed pulse in the plot?
loc_pulse: Fraction of the window length where the pulse is located.(eg. 0.25 = 1/4th of the way in.
0.5 = middle of the plot)
maxnumcands: What is the maximum number of candidates you would like to generate?
basename: output basename of the file. Appended with _DM_TIME(s)_RANK.spd
Optional arguments:
mask: Do you want to mask out rfi contaminated channels?
bandpass_corr: Do you want to remove the bandpass?
barytime: Is the given time(s) barycentric?
man_params: Do you want to specify the parameters for waterfalling
manually? If yes, I suggest using the function make_spd_from_man_params().
(I suggest giving it the rratrap output file)
Outputs:
Binary npz file containing the necessary arrays and header information to generate the spd plots.
"""
numcands = 0 # counter for max number of candidates
loop_must_break = False # dont break the loop unless num of cands >100.
files = spio.get_textfile(options.txtfile)
if group_rank:
groups = [group_rank - 1]
else:
groups = [i for i in range(6) if (i >= min_rank)][::-1]
for group in groups:
rank = group + 1
if files[group] != "Number of rank %i groups: 0 " % rank:
values = spio.split_parameters(rank, txtfile)
lis = np.where(files == '\tRank: %i.000000' % rank)[0]
for ii in range(len(values)):
#### Arrays for Plotting DM vs SNR
dm_list, time_list, dm_arr, sigma_arr, width_arr = spio.read_RRATrap_info(
txtfile, lis[ii], rank)
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
spdcand.read_from_file(values[ii], rawdatafile.tsamp, rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], \
rawdatafile, loc_pulse=loc_pulse, dedisp = True, \
scaleindep = None, zerodm = None, mask = mask, \
barytime=barytime, \
nsub = nsub, bandpass_corr = bandpass_corr)
#make an array to store header information for the spd files
temp_filename = basename+"_DM%.1f_%.1fs_rank_%i"%(spdcand.subdm, \
spdcand.topo_start_time, rank)
print_debug("Running waterfaller with Zero-DM OFF...")
# Add additional information to the header information array
data, Data_dedisp_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
text_array = np.array([args[0], rawdatafile.specinfo.telescope, \
rawdatafile.specinfo.ra_str, rawdatafile.specinfo.dec_str, \
rawdatafile.specinfo.start_MJD[0], \
rank, spdcand.nsub, spdcand.nbins, spdcand.subdm, \
spdcand.sigma, spdcand.sample_number, spdcand.duration, \
spdcand.width_bins, spdcand.pulse_width, rawdatafile.tsamp,\
rawdatafile.specinfo.T, spdcand.topo_start_time, data.starttime, \
data.dt,data.numspectra, data.freqs.min(), data.freqs.max()])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
zerodm = True
data, Data_dedisp_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
####Sweeped without zerodm
spdcand.read_from_file(values[ii], rawdatafile.tsamp, rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], \
rawdatafile, loc_pulse=loc_pulse, dedisp = None, \
scaleindep = None, zerodm = None, mask = mask, \
barytime=barytime, \
nsub = nsub, bandpass_corr = bandpass_corr)
data, Data_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
text_array = np.append(text_array, spdcand.sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, spdcand.bary_start_time)
text_array = np.append(text_array, man_params)
# Array to Construct the sweep
if spdcand.sweep_dm is not None:
ddm = spdcand.sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
#downsamp_temp = 1
data, Data_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
# Saving the arrays into the .spd file.
with open(temp_filename + ".spd", 'wb') as f:
np.savez_compressed(f, \
Data_dedisp_nozerodm = Data_dedisp_nozerodm.astype(np.float16),\
Data_dedisp_zerodm = Data_dedisp_zerodm.astype(np.float16),\
Data_nozerodm = Data_nozerodm.astype(np.float16),\
delays_nozerodm = delays_nozerodm, \
freqs_nozerodm = freqs_nozerodm,\
Data_zerodm = Data_zerodm.astype(np.float16), \
dm_arr= list(map(np.float16, dm_arr)),\
sigma_arr = list(map(np.float16, sigma_arr)), \
width_arr =list(map(np.uint8, width_arr)),\
dm_list= list(map(np.float16, dm_list)), \
time_list = list(map(np.float16, time_list)), \
text_array = text_array)
#### Arrays for Plotting DM vs Time is in plot_spd.plot(...)
if plot:
print_debug("Now plotting...")
plot_spd.plot(temp_filename+".spd", args[1:], \
spec_width=1.5, loc_pulse=loc_pulse, \
xwin=False, outfile=basename, \
just_waterfall=just_waterfall, \
integrate_spec=integrate_spec, \
integrate_ts=integrate_ts, \
disp_pulse=disp_pulse, tar = None)
print_debug("Finished plot %i " % ii +
strftime("%Y-%m-%d %H:%M:%S"))
numcands += 1
print_debug('Finished sp_candidate : %i' % numcands)
if numcands >= maxnumcands: # Max number of candidates to plot 100.
loop_must_break = True
break
if loop_must_break:
break
print_debug("Finished group %i... " % rank +
strftime("%Y-%m-%d %H:%M:%S"))
print_debug("Finished running waterfaller... " +
strftime("%Y-%m-%d %H:%M:%S"))
def inject(infile, outfn, prof, period, dm, nbitsout=None,
block_size=BLOCKSIZE, pulsar_only=False, inplace=False):
if isinstance(infile, filterbank.FilterbankFile):
fil = infile
elif inplace:
fil = filterbank.FilterbankFile(infile, 'readwrite')
else:
fil = filterbank.FilterbankFile(infile, 'read')
print "Injecting pulsar signal into: %s" % fil.filename
if False:
delays = psr_utils.delay_from_DM(dm, fil.frequencies)
delays -= delays[np.argmax(fil.frequencies)]
get_phases = lambda times: (times-delays)/period % 1
else:
get_phases = lambda times: times/period % 1
# Create the output filterbank file
if nbitsout is None:
nbitsout = fil.nbits
if inplace:
warnings.warn("Injecting pulsar signal *in-place*")
outfil = fil
else:
# Start an output file
print "Creating out file: %s" % outfn
outfil = filterbank.create_filterbank_file(outfn, fil.header, \
nbits=nbitsout, mode='append')
if outfil.nbits == 8:
raise NotImplementedError("This code is out of date. 'delays' is not " \
"done in this way anymore..")
# Read the first second of data to get the global scaling to use
onesec = fil.get_timeslice(0, 1).copy()
onesec_nspec = onesec.shape[0]
times = np.atleast_2d(np.arange(onesec_nspec)*fil.tsamp).T+delays
phases = times/period % 1
onesec += prof(phases)
minimum = np.min(onesec)
median = np.median(onesec)
# Set median to 1/3 of dynamic range
global_scale = (256.0/3.0) / median
del onesec
else:
# No scaling to be performed
# These values will cause scaling to keep data unchanged
minimum = 0
global_scale = 1
sys.stdout.write(" %3.0f %%\r" % 0)
sys.stdout.flush()
oldprogress = -1
# Loop over data
lobin = 0
spectra = fil.get_spectra(0, block_size)
numread = spectra.shape[0]
while numread:
if pulsar_only:
# Do not write out data from input file
# zero it out
spectra *= 0
hibin = lobin+numread
# Sample at middle of time bin
times = (np.arange(lobin, hibin, 1.0/NINTEG_PER_BIN)+0.5/NINTEG_PER_BIN)*fil.dt
#times = (np.arange(lobin, hibin)+0.5)*fil.dt
phases = get_phases(times)
profvals = prof(phases)
shape = list(profvals.shape)
shape[1:1] = [NINTEG_PER_BIN]
shape[0] /= NINTEG_PER_BIN
profvals.shape = shape
toinject = profvals.mean(axis=1)
#toinject = profvals
if np.ndim(toinject) > 1:
injected = spectra+toinject
else:
injected = spectra+toinject[:,np.newaxis]
scaled = (injected-minimum)*global_scale
if inplace:
outfil.write_spectra(scaled, lobin)
else:
outfil.append_spectra(scaled)
# Print progress to screen
progress = int(100.0*hibin/fil.nspec)
if progress > oldprogress:
sys.stdout.write(" %3.0f %%\r" % progress)
sys.stdout.flush()
oldprogress = progress
# Prepare for next iteration
lobin = hibin
spectra = fil.get_spectra(lobin, block_size)
numread = spectra.shape[0]
sys.stdout.write("Done \n")
sys.stdout.flush()
def main():
parser = optparse.OptionParser(prog="sp_pipeline..py", \
version=" Chitrang Patel (May. 12, 2015)", \
usage="%prog INFILE(PsrFits FILE, SINGLEPULSE FILES)", \
description="Create single pulse plots to show the " \
"frequency sweeps of a single pulse, " \
"DM vs time, and SNR vs DM,"\
"in psrFits data.")
parser.add_option('--infile', dest='infile', type='string', \
help="Give a .inf file to read the appropriate header information.")
parser.add_option('--groupsfile', dest='txtfile', type='string', \
help="Give the groups.txt file to read in the groups information.")
parser.add_option('--mask', dest='maskfile', type='string', \
help="Mask file produced by rfifind. (Default: No Mask).", \
default=None)
options, args = parser.parse_args()
if not hasattr(options, 'infile'):
raise ValueError("A .inf file must be given on the command line! ")
if not hasattr(options, 'txtfile'):
raise ValueError(
"The groups.txt file must be given on the command line! ")
files = get_textfile(options.txtfile)
print_debug("Begining waterfaller... " + strftime("%Y-%m-%d %H:%M:%S"))
Detrendlen = 50
if not args[0].endswith("fits"):
raise ValueError("The first file must be a psrFits file! ")
basename = args[0][:-5]
filetype = "psrfits"
inffile = options.infile
topo, bary = bary_and_topo.bary_to_topo(inffile)
time_shift = bary - topo
inf = infodata.infodata(inffile)
RA = inf.RA
dec = inf.DEC
MJD = inf.epoch
mjd = Popen(["mjd2cal", "%f" % MJD], stdout=PIPE, stderr=PIPE)
date, err = mjd.communicate()
date = date.split()[2:5]
telescope = inf.telescope
N = inf.N
Total_observed_time = inf.dt * N
print_debug('getting file..')
rawdatafile = psrfits.PsrfitsFile(args[0])
print "rawdatafile", memory.resident() / (1024.0**3)
bin_shift = np.round(time_shift / rawdatafile.tsamp).astype('int')
for group in [6, 5, 4, 3, 2]:
rank = group + 1
if files[group] != "Number of rank %i groups: 0 " % rank:
print_debug(files[group])
values = split_parameters(rank, options.txtfile)
lis = np.where(files == '\tRank: %i.000000' % rank)[0]
for ii in range(len(values)):
#### Array for Plotting DM vs SNR
print "DM, S/N", memory.resident() / (1024.0**3)
print_debug("Making arrays for DM vs Signal to Noise...")
temp_list = files[lis[ii] - 6].split()
npulses = int(temp_list[2])
temp_lines = files[(lis[ii] + 3):(lis[ii] + npulses + 1)]
arr = np.split(temp_lines, len(temp_lines))
dm_list = []
time_list = []
for i in range(len(arr)):
dm_val = float(arr[i][0].split()[0])
time_val = float(arr[i][0].split()[2])
dm_list.append(dm_val)
time_list.append(time_val)
arr_2 = np.array([arr[i][0].split() for i in range(len(arr))],
dtype=np.float32)
dm_arr = np.array([arr_2[i][0] for i in range(len(arr))],
dtype=np.float32)
sigma_arr = np.array([arr_2[i][1] for i in range(len(arr))],
dtype=np.float32)
print "After DM, S/N", memory.resident() / (1024.0**3)
#### Array for Plotting DM vs Time is in show_spplots.plot(...)
#### Setting variables up for the waterfall arrays.
j = ii + 1
subdm = dm = sweep_dm = values[ii][0]
integrate_dm = None
sigma = values[ii][1]
sweep_posn = 0.0
topo_start_time = values[ii][2] - topo_timeshift(
values[ii][2], time_shift, topo)[0]
sample_number = values[ii][3]
width_bins = values[ii][4]
binratio = 50
scaleindep = False
zerodm = None
downsamp = np.round((values[ii][2] / sample_number /
6.54761904761905e-05)).astype('int')
duration = binratio * width_bins * rawdatafile.tsamp * downsamp
start = topo_start_time - (0.25 * duration)
if (start < 0.0):
start = 0.0
pulse_width = width_bins * downsamp * 6.54761904761905e-05
if sigma <= 10:
nsub = 32
elif sigma >= 10 and sigma < 15:
nsub = 64
else:
nsub = 96
nbins = np.round(duration / rawdatafile.tsamp).astype('int')
start_bin = np.round(start / rawdatafile.tsamp).astype('int')
dmfac = 4.15e3 * np.abs(1. / rawdatafile.frequencies[0]**2 -
1. / rawdatafile.frequencies[-1]**2)
nbinsextra = np.round(
(duration + dmfac * dm) / rawdatafile.tsamp).astype('int')
if (start_bin + nbinsextra) > N - 1:
nbinsextra = N - 1 - start_bin
data = rawdatafile.get_spectra(start_bin, nbinsextra)
print "After rawdata", memory.resident() / (1024.0**3)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
#make an array to store header information for the .npz files
temp_filename = basename + "_DM%.1f_%.1fs_rank_%i" % (
subdm, topo_start_time, rank)
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
print_debug("Running waterfaller with Zero-DM OFF...")
data, Data_dedisp_nozerodm = waterfall_array(
start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm,
integrate_dm, downsamp, scaleindep, width_bins,
rawdatafile, binratio, data)
print "waterfall", memory.resident() / (1024.0**3)
# Add additional information to the header information array
text_array = np.array([
args[0], 'Arecibo', RA, dec, MJD, rank, nsub, nbins, subdm,
sigma, sample_number, duration, width_bins, pulse_width,
rawdatafile.tsamp, Total_observed_time, topo_start_time,
data.starttime, data.dt, data.numspectra,
data.freqs.min(),
data.freqs.max()
])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
zerodm = True
data, Data_dedisp_zerodm = waterfall_array(
start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm,
integrate_dm, downsamp, scaleindep, width_bins,
rawdatafile, binratio, data)
print "waterfall", memory.resident() / (1024.0**3)
####Sweeped without zerodm
print_debug("Running waterfaller for sweeped arrays.")
start = start + (0.25 * duration)
start_bin = np.round(start / rawdatafile.tsamp).astype('int')
sweep_duration = 4.15e3 * np.abs(
1. / rawdatafile.frequencies[0]**2 -
1. / rawdatafile.frequencies[-1]**2) * sweep_dm
nbins = np.round(sweep_duration /
(rawdatafile.tsamp)).astype('int')
if ((nbins + start_bin) > (N - 1)):
nbins = N - 1 - start_bin
data = rawdatafile.get_spectra(start_bin, nbins)
data = maskdata(data, start_bin, nbins, options.maskfile)
zerodm = None
dm = None
data, Data_nozerodm = waterfall_array(
start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm,
integrate_dm, downsamp, scaleindep, width_bins,
rawdatafile, binratio, data)
print "waterfall", memory.resident() / (1024.0**3)
text_array = np.append(text_array, sweep_duration)
text_array = np.append(text_array, data.starttime)
# Array to Construct the sweep
if sweep_dm is not None:
ddm = sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
downsamp_temp = 1
data, Data_zerodm = waterfall_array(start_bin, dmfac, duration,
nbins, zerodm, nsub, subdm,
dm, integrate_dm,
downsamp_temp, scaleindep,
width_bins, rawdatafile,
binratio, data)
print "waterfall", memory.resident() / (1024.0**3)
# Saving the arrays into the .spd file.
with open(temp_filename + ".spd", 'wb') as f:
np.savez_compressed(
f,
Data_dedisp_nozerodm=Data_dedisp_nozerodm.astype(
np.float16),
Data_dedisp_zerodm=Data_dedisp_zerodm.astype(
np.float16),
Data_nozerodm=Data_nozerodm.astype(np.float16),
delays_nozerodm=delays_nozerodm,
freqs_nozerodm=freqs_nozerodm,
Data_zerodm=Data_zerodm.astype(np.float16),
dm_arr=map(np.float16, dm_arr),
sigma_arr=map(np.float16, sigma_arr),
dm_list=map(np.float16, dm_list),
time_list=map(np.float16, time_list),
text_array=text_array)
print_debug("Now plotting...")
print "Before plot..", memory.resident() / (1024.0**3)
show_spplots.plot(temp_filename + ".spd",
args[1:],
xwin=False,
outfile=basename,
tar=None)
print "After plot..", memory.resident() / (1024.0**3)
print_debug("Finished plot %i " % j +
strftime("%Y-%m-%d %H:%M:%S"))
print_debug("Finished group %i... " % rank +
strftime("%Y-%m-%d %H:%M:%S"))
print_debug("Finished running waterfaller... " +
strftime("%Y-%m-%d %H:%M:%S"))
def main():
fn = args[0]
if fn.endswith(".fil"):
# Filterbank file
filetype = "filterbank"
rawdatafile = filterbank.filterbank(fn)
elif fn.endswith(".fits"):
# PSRFITS file
filetype = "psrfits"
rawdatafile = psrfits.PsrfitsFile(fn)
else:
raise ValueError("Cannot recognize data file type from "
"extension. (Only '.fits' and '.fil' "
"are supported.)")
# Read data
start_bin = np.round(options.start/rawdatafile.tsamp).astype('int')
#dmfac = 4.15e3 * np.abs(1./rawdatafile.fch1**2 - 1./(rawdatafile.frequencies[-1])**2)
dmfac = 4.15e3 * np.abs(1./rawdatafile.frequencies[0]**2 - 1./rawdatafile.frequencies[-1]**2)
if options.nbins is None:
nbins = np.round(options.duration/rawdatafile.tsamp).astype('int')
else:
nbins = options.nbins
binratio = 50
if options.dm:
nbinsextra = np.round((options.duration + dmfac * options.dm)/rawdatafile.tsamp).astype('int')
else:
nbinsextra = nbins
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskfile(data, start_bin, nbinsextra)
data, bins = waterfall(start_bin, dmfac, options.duration, nbins, options.zerodm, options.nsub, options.subdm, options.dm, options.integrate_dm, options.downsamp, options.scaleindep, options.width_bins, rawdatafile, binratio, data)
# Ploting it up
fig = plt.figure()
fig.canvas.set_window_title("Frequency vs. Time")
ax = plt.axes((0.15, 0.15, 0.8, 0.60))
ragfac = float(nbins)/bins
dmrange, trange = data.data.shape
nbinlim = np.int(trange * ragfac)
print data.dt, rawdatafile.tsamp
#np.save('data',data.data[..., :nbinlim])
plt.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[options.cmap], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
if options.show_cb:
cb = plt.colorbar()
cb.set_label("Scaled signal intensity (arbitrary units)")
#plt.axis('tight')
# Sweeping it up
for ii, sweep_dm in enumerate(options.sweep_dms):
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if options.sweep_posns is None:
sweep_posn = 0.0
elif len(options.sweep_posns) == 1:
sweep_posn = options.sweep_posns[0]
else:
sweep_posn = options.sweep_posns[ii]
sweepstart = data.dt*data.numspectra*sweep_posn+data.starttime
sty = SWEEP_STYLES[ii%len(SWEEP_STYLES)]
plt.plot(delays+sweepstart, data.freqs, sty, lw=4, alpha=0.5)
# Dressing it up
plt.xlabel("Time")
plt.ylabel("Observing frequency (MHz)")
plt.suptitle("Frequency vs. Time")
# Plot Time series
if options.integrate_dm is not None:
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data.numspectra)*data.dt + options.start)[..., :nbinlim]
ax = plt.axes((0.15, 0.75, 0.8, 0.2))
plt.plot(times, Dedisp_ts)
plt.setp(ax.get_xticklabels(), visible = False)
plt.setp(ax.get_yticklabels(), visible = False)
fig.canvas.mpl_connect('key_press_event', \
lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
plt.show()
if counterpart == False:
print "Didn't find counterpart frequency for %f" % f0
sub.set_weight(i,0.0)
continue
# else:
# print counterpart,f1
# print f0, f1
# sys.exit()
# print f0,f1
p = sub.get_folding_period()
smear = (psr_utils.dm_smear(dm,chbw,f0)
+ psr_utils.dm_smear(dm,chbw,f1)) / p
delay = (psr_utils.delay_from_DM(dm,f0)
- psr_utils.delay_from_DM(dm,f1)) / p
delay -= int(delay)
if delay<-0.5: delay += 1.0
if delay>0.5: delay -= 1.0
#print i, smear, delay
for pol in range(2):
if pol == 0:
correction = pol0correction/2.0
else:
correction = pol1correction/2.0
# correction = correction * 16.0
def main():
parser = optparse.OptionParser(prog="sp_pipeline..py", \
version=" Chitrang Patel (May. 12, 2015)", \
usage="%prog INFILE(PsrFits FILE, SINGLEPULSE FILES)", \
description="Create single pulse plots to show the " \
"frequency sweeps of a single pulse, " \
"DM vs time, and SNR vs DM,"\
"in psrFits data.")
parser.add_option('--infile', dest='infile', type='string', \
help="Give a .inf file to read the appropriate header information.")
parser.add_option('--groupsfile', dest='txtfile', type='string', \
help="Give the groups.txt file to read in the groups information.")
parser.add_option('--mask', dest='maskfile', type='string', \
help="Mask file produced by rfifind. (Default: No Mask).", \
default=None)
parser.add_option('-n', dest='maxnumcands', type='int', \
help="Maximum number of candidates to plot. (Default: 100).", \
default=100)
options, args = parser.parse_args()
if not hasattr(options, 'infile'):
raise ValueError("A .inf file must be given on the command line! ")
if not hasattr(options, 'txtfile'):
raise ValueError(
"The groups.txt file must be given on the command line! ")
files = get_textfile(options.txtfile)
print_debug("Begining waterfaller... " + strftime("%Y-%m-%d %H:%M:%S"))
if not args[0].endswith("fits"):
raise ValueError("The first file must be a psrFits file! ")
print_debug('Maximum number of candidates to plot: %i' %
options.maxnumcands)
basename = args[0][:-5]
filetype = "psrfits"
inffile = options.infile
topo, bary = bary_and_topo.bary_to_topo(inffile)
time_shift = bary - topo
inf = infodata.infodata(inffile)
RA = inf.RA
dec = inf.DEC
MJD = inf.epoch
mjd = Popen(["mjd2cal", "%f" % MJD], stdout=PIPE, stderr=PIPE)
date, err = mjd.communicate()
date = date.split()[2:5]
telescope = inf.telescope
N = inf.N
numcands = 0
Total_observed_time = inf.dt * N
print_debug('getting file..')
values = split_parameters(options.txtfile)
if len(values) > options.maxnumcands:
values = sorted(values, key=itemgetter(
5, 1)) #sorting candidates based on ranks and snr
values = values[-options.maxnumcands:]
print "More than", options.maxnumcands, "candidates, making plots for", options.maxnumcands, "candidates"
values = sorted(values, key=itemgetter(0))
for ii in range(len(values)):
#### Array for Plotting DM vs SNR
print_debug("Making arrays for DM vs Signal to Noise...")
temp_list = files[values[ii][6] - 6].split()
npulses = int(temp_list[2])
temp_lines = files[(values[ii][6] + 3):(values[ii][6] + npulses + 1)]
arr = np.split(temp_lines, len(temp_lines))
dm_list = []
time_list = []
for i in range(len(arr)):
dm_val = float(arr[i][0].split()[0])
time_val = float(arr[i][0].split()[2])
dm_list.append(dm_val)
time_list.append(time_val)
arr_2 = np.array([arr[i][0].split() for i in range(len(arr))],
dtype=np.float32)
dm_arr = np.array([arr_2[i][0] for i in range(len(arr))],
dtype=np.float32)
sigma_arr = np.array([arr_2[i][1] for i in range(len(arr))],
dtype=np.float32)
#### Array for Plotting DM vs Time is in show_spplots.plot(...)
#### Setting variables up for the waterfall arrays.
j = ii + 1
subdm = dm = sweep_dm = values[ii][0]
sample_number = values[ii][3]
rank = values[ii][5]
width_bins = values[ii][4]
#print "dm", dm
#print "width_bins", width_bins
downsamp = np.round(
(values[ii][2] / sample_number / inf.dt)).astype('int')
#print "downsamp", downsamp
pulse_width = width_bins * downsamp * inf.dt
#print "pulse_width", pulse_width
if ii == 0:
mask_subband = rfifind.rfifind("%s_rfifind.mask" % (basename))
mask_subband.set_zap_chans(power=1000, plot=False)
mask_subband.set_weights_and_offsets()
mask_subband.write_weights(filename="%s_weights.txt" % (basename))
cmd = "psrfits_subband -dm %.2f -nsub 128 -o %s_subband_%.2f -weights %s_weights.txt %s" % (
dm, basename, dm, basename, args[0])
call(cmd, shell=True)
#subband args[0] at dm and then generate a file that will be set equal to rawdatafile
subband_file = "%s_subband_%.2f_0001.fits" % (basename, dm)
dm_prev = dm
subband_prev = subband_file
else:
dm_diff = dm - dm_prev
t_smear = 8.3e3 * dm_diff * (350**-3) * (
np.abs(rawdatafile.frequencies[0] -
rawdatafile.frequencies[-1]) / 128.)
if (5 * t_smear) > pulse_width:
cmd = "psrfits_subband -dm %.2f -nsub 128 -o %s_subband_%.2f -weights %s_weights.txt %s" % (
dm, basename, dm, basename, args[0])
call(cmd, shell=True)
#subband args[0] at dm and then generate a file that will be set equal to rawdatafile
subband_file = "%s_subband_%.2f_0001.fits" % (basename, dm)
dm_prev = dm
subband_prev = subband_file
rawdatafile = psrfits.PsrfitsFile(subband_file)
bin_shift = np.round(time_shift / rawdatafile.tsamp).astype('int')
integrate_dm = None
sigma = values[ii][1]
sweep_posn = 0.0
bary_start_time = values[ii][2]
topo_start_time = bary_start_time - topo_timeshift(
bary_start_time, time_shift, topo)[0]
binratio = 50
scaleindep = False
zerodm = None
duration = binratio * width_bins * rawdatafile.tsamp * downsamp
start = topo_start_time - (0.25 * duration)
if (start < 0.0):
start = 0.0
if sigma <= 7:
nsub = 32
elif sigma >= 7 and sigma < 10:
nsub = 64
else:
nsub = 128
nbins = np.round(duration / rawdatafile.tsamp).astype('int')
start_bin = np.round(start / rawdatafile.tsamp).astype('int')
dmfac = 4.15e3 * np.abs(1. / rawdatafile.frequencies[0]**2 -
1. / rawdatafile.frequencies[-1]**2)
nbinsextra = np.round(
(duration + dmfac * dm) / rawdatafile.tsamp).astype('int')
if (start_bin + nbinsextra) > N - 1:
nbinsextra = N - 1 - start_bin
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
#make an array to store header information for the .npz files
temp_filename = basename + "_DM%.1f_%.1fs_rank_%i" % (
subdm, topo_start_time, rank)
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
print_debug("Running waterfaller with Zero-DM OFF...")
data, Data_dedisp_nozerodm = waterfall_array(
start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm,
integrate_dm, downsamp, scaleindep, width_bins, rawdatafile,
binratio, data)
#Add additional information to the header information array
text_array = np.array([
subband_file, 'GBT', RA, dec, MJD, rank, nsub, nbins, subdm, sigma,
sample_number, duration, width_bins, pulse_width,
rawdatafile.tsamp, Total_observed_time, topo_start_time,
data.starttime, data.dt, data.numspectra,
data.freqs.min(),
data.freqs.max()
])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
#print "before get_spectra",memory.resident()/(1024.0**3)
data = rawdatafile.get_spectra(start_bin, nbinsextra)
#print "after get_spectra",memory.resident()/(1024.0**3)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
zerodm = True
data, Data_dedisp_zerodm = waterfall_array(start_bin, dmfac, duration,
nbins, zerodm, nsub, subdm,
dm, integrate_dm, downsamp,
scaleindep, width_bins,
rawdatafile, binratio, data)
#print "waterfall",memory.resident()/(1024.0**3)
####Sweeped without zerodm
start = start + (0.25 * duration)
start_bin = np.round(start / rawdatafile.tsamp).astype('int')
sweep_duration = 4.15e3 * np.abs(
1. / rawdatafile.frequencies[0]**2 -
1. / rawdatafile.frequencies[-1]**2) * sweep_dm
nbins = np.round(sweep_duration / (rawdatafile.tsamp)).astype('int')
if ((nbins + start_bin) > (N - 1)):
nbins = N - 1 - start_bin
#print "before get_spectra",memory.resident()/(1024.0**3)
data = rawdatafile.get_spectra(start_bin, nbins)
#print "after get_spectra",memory.resident()/(1024.0**3)
data = maskdata(data, start_bin, nbins, options.maskfile)
zerodm = None
dm = None
data, Data_nozerodm = waterfall_array(start_bin, dmfac, duration,
nbins, zerodm, nsub, subdm, dm,
integrate_dm, downsamp,
scaleindep, width_bins,
rawdatafile, binratio, data)
#print "waterfall",memory.resident()/(1024.0**3)
text_array = np.append(text_array, sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, bary_start_time)
# Array to Construct the sweep
if sweep_dm is not None:
ddm = sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
downsamp_temp = 1
data, Data_zerodm = waterfall_array(start_bin, dmfac, duration, nbins,
zerodm, nsub, subdm, dm,
integrate_dm, downsamp_temp,
scaleindep, width_bins,
rawdatafile, binratio, data)
#print "waterfall",memory.resident()/(1024.0**3)
# Saving the arrays into the .spd file.
with open(temp_filename + ".spd", 'wb') as f:
np.savez_compressed(
f,
Data_dedisp_nozerodm=Data_dedisp_nozerodm.astype(np.float16),
Data_dedisp_zerodm=Data_dedisp_zerodm.astype(np.float16),
Data_nozerodm=Data_nozerodm.astype(np.float16),
delays_nozerodm=delays_nozerodm,
freqs_nozerodm=freqs_nozerodm,
Data_zerodm=Data_zerodm.astype(np.float16),
dm_arr=map(np.float16, dm_arr),
sigma_arr=map(np.float16, sigma_arr),
dm_list=map(np.float16, dm_list),
time_list=map(np.float16, time_list),
text_array=text_array)
print_debug("Now plotting...")
#print "Before plot..",memory.resident()/(1024.0**3)
show_spplots.plot(temp_filename + ".spd",
args[1:],
xwin=False,
outfile=basename,
tar=None)
print_debug("Finished plot %i " % j + strftime("%Y-%m-%d %H:%M:%S"))
#print "After plot..",memory.resident()/(1024.0**3)
numcands += 1
print_debug('Finished sp_candidate : %i' % numcands)
print_debug("Finished running waterfaller... " +
strftime("%Y-%m-%d %H:%M:%S"))
def get_delaybins(self, dm):
subdelays = psr_utils.delay_from_DM(dm, self.subfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays-hifreqdelay
delaybins = subdelays*self.binspersec
return np.floor(delaybins+0.5)
def get_delaybins(self, dm):
subdelays = psr_utils.delay_from_DM(dm, self.subfreqs)
hifreqdelay = subdelays[-1]
subdelays = subdelays - hifreqdelay
delaybins = subdelays * self.binspersec
return np.floor(delaybins + 0.5)
if counterpart == False:
print "Didn't find counterpart frequency for %f" % f0
sub.set_weight(i, 0.0)
continue
# else:
# print counterpart,f1
# print f0, f1
# sys.exit()
# print f0,f1
p = sub.get_folding_period()
smear = (psr_utils.dm_smear(dm, chbw, f0) +
psr_utils.dm_smear(dm, chbw, f1)) / p
delay = (psr_utils.delay_from_DM(dm, f0) -
psr_utils.delay_from_DM(dm, f1)) / p
delay -= int(delay)
if delay < -0.5: delay += 1.0
if delay > 0.5: delay -= 1.0
#print i, smear, delay
for pol in range(2):
if pol == 0:
correction = pol0correction / 2.0
else:
correction = pol1correction / 2.0
# correction = correction * 16.0
# Combine the profiles as required
profs = fold_pfd.combine_profs(numtoas, numsubbands)
# PRESTO de-disperses at the high frequency channel so determine a
# correction to the middle of the band
if not events:
subpersumsub = fold_pfd.nsub / numsubbands
# Calculate the center of the summed subband freqs and delays
sumsubfreqs = (Num.arange(numsubbands)+0.5)*subpersumsub*fold_pfd.subdeltafreq + \
(fold_pfd.lofreq-0.5*fold_pfd.chan_wid)
# Note: In the following, we cannot use fold_pfd.hifreqdelay since that
# is based on the _barycentric_ high frequency (if the barycentric
# conversion was available). For TOAs, we need a topocentric
# delay, which is based on the topocentric frequency fold_pfd.hifreq
sumsubdelays = (
psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs) -
psr_utils.delay_from_DM(fold_pfd.bestdm, fold_pfd.hifreq))
sumsubdelays_phs = Num.fmod(sumsubdelays / p_dedisp, 1.0)
# Save the "higest channel within a subband" freqs/delays for use in
# later DM/timing correction. PBD 2011/11/03
sumsubfreqs_hi = sumsubfreqs + \
fold_pfd.subdeltafreq/2.0 - fold_pfd.chan_wid/2.0
subdelays2 = psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs) - \
psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs_hi)
else:
fold_pfd.subfreqs = Num.asarray([0.0])
sumsubfreqs = Num.asarray([0.0])
sumsubdelays = Num.asarray([0.0])
subdelays2 = Num.asarray([0.0])
sumsubdelays_phs = Num.asarray([0.0])
profs = fold_pfd.combine_profs(numtoas, numsubbands)
# PRESTO de-disperses at the high frequency channel so determine a
# correction to the middle of the band
if not events:
subpersumsub = fold_pfd.nsub / numsubbands
# Calculate the center of the summed subband freqs and delays
sumsubfreqs = (Num.arange(numsubbands) + 0.5) * subpersumsub * fold_pfd.subdeltafreq + (
fold_pfd.lofreq - 0.5 * fold_pfd.chan_wid
)
# Note: In the following, we cannot use fold_pfd.hifreqdelay since that
# is based on the _barycentric_ high frequency (if the barycentric
# conversion was available). For TOAs, we need a topocentric
# delay, which is based on the topocentric frequency fold_pfd.hifreq
sumsubdelays = (
psr_utils.delay_from_DM(fold_pfd.bestdm, sumsubfreqs)
- psr_utils.delay_from_DM(fold_pfd.bestdm, fold_pfd.hifreq)
) / SECPERDAY
else:
fold_pfd.subfreqs = Num.asarray([0.0])
sumsubfreqs = Num.asarray([0.0])
sumsubdelays = Num.asarray([0.0])
# Read the template profile
if templatefilenm is not None:
template = psr_utils.read_profile(templatefilenm, normalize=1)
else:
if gaussfitfile:
template = psr_utils.read_gaussfitfile(gaussfitfile, fold_pfd.proflen)
else:
template = psr_utils.gaussian_profile(fold_pfd.proflen, 0.0, gaussianwidth)
def plot_waterfall(data, start, duration,
integrate_ts=False, integrate_spec=False, show_cb=False,
cmap_str="gist_yarg", sweep_dms=[], sweep_posns=[],
ax_im=None, ax_ts=None, ax_spec=None, interactive=True):
""" I want a docstring too!
"""
# Set up axes
if interactive:
fig = plt.figure()
fig.canvas.set_window_title("Frequency vs. Time")
im_width = 0.6 if integrate_spec else 0.8
im_height = 0.6 if integrate_ts else 0.8
if not ax_im:
ax_im = plt.axes((0.15, 0.15, im_width, im_height))
if integrate_ts and not ax_ts:
ax_ts = plt.axes((0.15, 0.75, im_width, 0.2),sharex=ax_im)
if integrate_spec and not ax_spec:
ax_spec = plt.axes((0.75, 0.15, 0.2, im_height),sharey=ax_im)
# Ploting it up
nbinlim = np.int(duration/data.dt)
img = ax_im.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
if show_cb:
cb = ax_im.get_figure().colorbar(img)
cb.set_label("Scaled signal intensity (arbitrary units)")
#plt.axis('tight')
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt*data.numspectra*sweep_posn+data.starttime
sty = SWEEP_STYLES[ii%len(SWEEP_STYLES)]
ax_im.plot(delays+sweepstart, data.freqs, sty, lw=4, alpha=0.5)
# Dressing it up
ax_im.xaxis.get_major_formatter().set_useOffset(False)
ax_im.set_xlabel("Time")
ax_im.set_ylabel("Observing frequency (MHz)")
# Plot Time series
if integrate_ts:
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data.numspectra)*data.dt + start)[..., :nbinlim]
ax_ts.plot(times, Dedisp_ts,"k")
ax_ts.set_xlim([times.min(),times.max()])
plt.setp(ax_ts.get_xticklabels(), visible = False)
plt.setp(ax_ts.get_yticklabels(), visible = False)
# Plot Spectrum
if integrate_spec:
spectrum_window = 0.05*duration
window_width = int(spectrum_window/data.dt) # bins
burst_bin = nbinlim/2
on_spec = np.array(data.data[..., burst_bin-window_width:burst_bin+window_width])
Dedisp_spec = on_spec.sum(axis=1)[::-1]
freqs = np.linspace(data.freqs.min(), data.freqs.max(), len(Dedisp_spec))
ax_spec.plot(Dedisp_spec,freqs,"k")
plt.setp(ax_spec.get_xticklabels(), visible = False)
plt.setp(ax_spec.get_yticklabels(), visible = False)
ax_spec.set_ylim([data.freqs.min(),data.freqs.max()])
if integrate_ts:
ax_ts.axvline(times[burst_bin]-spectrum_window,ls="--",c="grey")
ax_ts.axvline(times[burst_bin]+spectrum_window,ls="--",c="grey")
if interactive:
fig.suptitle("Frequency vs. Time")
fig.canvas.mpl_connect('key_press_event', \
lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
plt.show()
def make_spd_from_man_params(spdcand, rawdatafile, \
txtfile, maskfile, \
plot, just_waterfall, \
subdm, dm, sweep_dm, \
sigma, \
start_time, duration, \
width_bins, nbins, downsamp, \
nsub, \
scaleindep, \
spec_width, loc_pulse, \
integrate_ts, integrate_spec, disp_pulse, \
basename, \
mask, bandpass_corr, barytime, man_params):
"""
Makes spd files from output files of rratrap.
Inputs:
spdcand: spcand parameters instance (read in spcand.params)
rawdatafile: psrfits file instance
txtfile: rratrap output file (groups.txt file)
maskfile: rfifind mask file. need this file if you want to remove the bandpass
or use rfifind mask information.
plot: do you want to produce the plots as well?
just_waterfall: Do you just want to make the waterfall plots.
subdm: DM to use when subbanding.
dm: DM to use when dedispersing data for plot.
sweep_dm: Show the frequency sweep using this DM.
sigma: signal-to-noise of the pulse
start_time: start time of the data to be read in for waterfalling.
duration: duration of data to be waterfalled.
width_bins: Smooth each channel/subband with a boxcar width_bins wide.
nbins: Number of time bins to plot. This option overrides
the duration argument.
downsamp: Factor to downsample in time by. Default: Don't downsample.
nsub: Number of subbands to use. Must be a factor of number of channels.
scaleindep:Do you want to scale each subband independently?(Type: Boolean)
spec_width: Twice this number times the pulse_width around the pulse to consider for the spectrum
loc_pulse: Fraction of the window length where the pulse is located.(eg. 0.25 = 1/4th of the way in.
0.5 = middle of the plot)
integrate_ts: Do you want to display the dedispersed time series in the plot?
integrate_spec: Do you want to display the pulse spectrum in the plot?
disp_pulse: Do you want to see the inset dispersed pulse in the plot?
basename: output basename of the file. Appended with _DM_TIME(s)_RANK.spd
mask: Do you want to mask out rfi contaminated channels?
bandpass_corr: Do you want to remove the bandpass?
barytime: Is the given time(s) barycentric?
man_params: Do you want to specify the parameters for waterfalling
manually? If yes, I suggest using the function make_spd_from_man_params().
(I suggest giving it the rratrap output file)
Outputs:
Binary npz file containing the necessary arrays and header information to generate the spd plots.
"""
rank = None
if not nsub:
nsub = rawdatafile.nchan
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
spdcand.manual_params(subdm, dm, sweep_dm, sigma, start_time, \
width_bins, downsamp, duration, nbins, nsub, rawdatafile.tsamp, \
rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], rawdatafile, \
loc_pulse=loc_pulse, dedisp=True, scaleindep=False, zerodm=False, \
mask=mask, barytime=barytime, bandpass_corr=bandpass_corr)
#make an array to store header information for the spd files
temp_filename = basename + "_DM%.1f_%.1fs" % (spdcand.subdm,
spdcand.topo_start_time)
print_debug("Running waterfaller with Zero-DM OFF...")
data, Data_dedisp_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
# Add additional information to the header information array
text_array = np.array([args[0], rawdatafile.specinfo.telescope, \
rawdatafile.specinfo.ra_str, rawdatafile.specinfo.dec_str, \
rawdatafile.specinfo.start_MJD[0], rank, \
spdcand.nsub, spdcand.nbins, \
spdcand.subdm, spdcand.sigma, spdcand.sample_number, \
spdcand.duration, spdcand.width_bins, spdcand.pulse_width, \
rawdatafile.tsamp, rawdatafile.specinfo.T, spdcand.topo_start_time, \
data.starttime, data.dt,data.numspectra, data.freqs.min(), \
data.freqs.max()])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
zerodm = True
data, Data_dedisp_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
####Sweeped without zerodm
spdcand.manual_params(subdm, dm, sweep_dm, sigma, start_time, \
width_bins, downsamp, duration, nbins, nsub, rawdatafile.tsamp, \
rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], rawdatafile, \
loc_pulse=loc_pulse, dedisp=None, scaleindep=None, zerodm=None, mask=mask, \
barytime=barytime, bandpass_corr=bandpass_corr)
data, Data_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
text_array = np.append(text_array, spdcand.sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, spdcand.bary_start_time)
text_array = np.append(text_array, man_params)
# Array to Construct the sweep
if spdcand.sweep_dm is not None:
ddm = spdcand.sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
#downsamp_temp = 1
data, Data_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
with open(temp_filename + ".spd", 'wb') as f:
np.savez_compressed(f, \
Data_dedisp_nozerodm = Data_dedisp_nozerodm.astype(np.float16),\
Data_dedisp_zerodm = Data_dedisp_zerodm.astype(np.float16),\
Data_nozerodm = Data_nozerodm.astype(np.float16),\
delays_nozerodm = delays_nozerodm, \
freqs_nozerodm = freqs_nozerodm,\
Data_zerodm = Data_zerodm.astype(np.float16), \
text_array = text_array)
#### Arrays for Plotting DM vs Time is in plot_spd.plot(...)
if plot:
print_debug("Now plotting...")
plot_spd.plot(temp_filename+".spd", args[1:], \
spec_width=spec_width, loc_pulse=loc_pulse, xwin=False, \
outfile = basename, just_waterfall=just_waterfall, \
integrate_spec=integrate_spec, integrate_ts=integrate_ts, \
disp_pulse=disp_pulse, tar = None)
def plot_waterfall(data,data_noscale,start,duration,centre_MJD,dm,sigma,width,tsamp,\
fres,tavg=1,favg=1,cmap_str="gist_yarg",integrate_spec=False,sweep_dms=[], sweep_posns=[],save_plot=False,interactive=True):
# Set up axes
if interactive:
fig = plt.figure(figsize=[12, 7])
fig.text(0.1, 0.9, "DM = %s pc/cc" % dm)
fig.text(0.1, 0.85, "Centre MJD = %s" % centre_MJD)
fig.text(0.1, 0.8, "Significance = %s sigma" % sigma)
fig.text(0.1, 0.75, "Boxcar width = %s seconds" % (tsamp * width))
fig.text(0.1, 0.25, "Plotting resolution")
fig.text(0.1, 0.2,
"Time resolution %s milliseconds" % (tsamp * tavg * 1e3))
fig.text(0.1, 0.15, "Frequency resolution %s MHz" % (fres * favg))
im_width = 0.3 if integrate_spec else 0.4
im_height = 0.8
ax_im = plt.axes((0.45, 0.15, im_width, im_height - 0.2))
ax_ts = plt.axes((0.45, 0.75, im_width, 0.2), sharex=ax_im)
if integrate_spec:
ax_spec = plt.axes((0.75, 0.15, 0.2, im_height), sharey=ax_im)
# Ploting it up
nbinlim = np.int(duration / data.dt)
#downsample in frequency
if favg != None and favg > 1:
nchan_tot = data.data.shape[0]
favg = float(favg)
if (nchan_tot / favg) - int(nchan_tot / favg) != 0:
print(
"The total number of channels is %s, please choose an fscrunch val\
ue that divides the total number of channels." % nchan_tot)
sys.exit()
else:
newnchan = nchan_tot / favg
data.data = np.array(
np.row_stack([
np.mean(subint, axis=0)
for subint in np.vsplit(data.data, newnchan)
]))
img = ax_im.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm - data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt * data.numspectra * sweep_posn + data.starttime
#sty = SWEEP_STYLES[ii%len(SWEEP_STYLES)]
ax_im.plot(delays + sweepstart, data.freqs, lw=4, alpha=0.5)
# Dressing it up
ax_im.xaxis.get_major_formatter().set_useOffset(False)
ax_im.set_xlabel("Time")
ax_im.set_ylabel("Frequency (MHz)")
ax_im.set_ylim((data.freqs.min(), data.freqs.max()))
axsec = ax_im.twinx()
axsec.set_yticks(
np.round(np.linspace(0, data.data[..., :nbinlim].shape[0], 10)) * favg)
axsec.set_ylabel('Bins')
# Plot Time series
Data = np.array(data_noscale.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data_noscale.numspectra) * data_noscale.dt +
start)[..., :nbinlim]
ax_ts.plot(times, Dedisp_ts, "k")
ax_ts.set_xlim([times.min(), times.max()])
plt.setp(ax_ts.get_xticklabels(), visible=False)
plt.setp(ax_ts.get_yticklabels(), visible=False)
# Plot Spectrum
if integrate_spec:
spectrum_window = 0.05 * duration
window_width = int(spectrum_window / data.dt) # bins
burst_bin = nbinlim / 2
on_spec = np.array(data.data[..., burst_bin - window_width:burst_bin +
window_width])
Dedisp_spec = on_spec.sum(axis=1)[::-1]
freqs = np.linspace(data.freqs.min(), data.freqs.max(),
len(Dedisp_spec))
ax_spec.plot(Dedisp_spec, freqs, "k")
plt.setp(ax_spec.get_xticklabels(), visible=False)
plt.setp(ax_spec.get_yticklabels(), visible=False)
ax_spec.set_ylim([data.freqs.min(), data.freqs.max()])
ax_ts.axvline(times[burst_bin] - spectrum_window, ls="--", c="grey")
ax_ts.axvline(times[burst_bin] + spectrum_window, ls="--", c="grey")
if interactive:
fig.canvas.mpl_connect('key_press_event', \
lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
if save_plot == True:
fig.savefig('waterfall_%sMJD_DM%s_sigma%s.png' %
(centre_MJD, dm, sigma),
dpi=300,
facecolor='w',
edgecolor='w',
format='png')
plt.close()
else:
plt.show()
def make_spd_from_file(spdcand, rawdatafile, \
txtfile, maskfile, \
min_rank, group_rank, \
plot, just_waterfall, \
integrate_ts, integrate_spec, disp_pulse, \
loc_pulse, nsub, \
maxnumcands, \
basename, \
mask=False, bandpass_corr=True, barytime=True, \
man_params=None):
"""
Makes spd files from output files of rratrap.
Inputs:
spdcand: spcand parameters instance (read in spcand.params)
rawdatafile: psrfits file instance
txtfile: rratrap output file (groups.txt file)
maskfile: rfifind mask file. need this file if you want to remove the bandpass
or use rfifind mask information.
min_rank: plot all groups with rank more than this. min 1, max 6
group_rank: plot groups ranked whatever you specify
plot: do you want to produce the plots as well?
just_waterfall: Do you just want to make the waterfall plots.
integrate_ts: Do you want to display the dedispersed time series in the plot?
integrate_spec: Do you want to display the pulse spectrum in the plot?
disp_pulse: Do you want to see the inset dispersed pulse in the plot?
loc_pulse: Fraction of the window length where the pulse is located.(eg. 0.25 = 1/4th of the way in.
0.5 = middle of the plot)
maxnumcands: What is the maximum number of candidates you would like to generate?
basename: output basename of the file. Appended with _DM_TIME(s)_RANK.spd
Optional arguments:
mask: Do you want to mask out rfi contaminated channels?
bandpass_corr: Do you want to remove the bandpass?
barytime: Is the given time(s) barycentric?
man_params: Do you want to specify the parameters for waterfalling
manually? If yes, I suggest using the function make_spd_from_man_params().
(I suggest giving it the rratrap output file)
Outputs:
Binary npz file containing the necessary arrays and header information to generate the spd plots.
"""
numcands=0 # counter for max number of candidates
loop_must_break = False # dont break the loop unless num of cands >100.
files = spio.get_textfile(options.txtfile)
if group_rank:
groups=[group_rank-1]
else:
groups = [i for i in range(6) if(i>=min_rank)][::-1]
for group in groups:
rank = group+1
if files[group] != "Number of rank %i groups: 0 "%rank:
values = spio.split_parameters(rank, txtfile)
lis = np.where(files == '\tRank: %i.000000'%rank)[0]
for ii in range(len(values)):
#### Arrays for Plotting DM vs SNR
dm_list, time_list, dm_arr, sigma_arr, width_arr = spio.read_RRATrap_info(txtfile, lis[ii], rank)
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
spdcand.read_from_file(values[ii], rawdatafile.tsamp, rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], \
rawdatafile, loc_pulse=loc_pulse, dedisp = True, \
scaleindep = None, zerodm = None, mask = mask, \
barytime=barytime, \
nsub = nsub, bandpass_corr = bandpass_corr)
#make an array to store header information for the spd files
temp_filename = basename+"_DM%.1f_%.1fs_rank_%i"%(spdcand.subdm, \
spdcand.topo_start_time, rank)
print_debug("Running waterfaller with Zero-DM OFF...")
# Add additional information to the header information array
data, Data_dedisp_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
text_array = np.array([args[0], rawdatafile.specinfo.telescope, \
rawdatafile.specinfo.ra_str, rawdatafile.specinfo.dec_str, \
rawdatafile.specinfo.start_MJD[0], \
rank, spdcand.nsub, spdcand.nbins, spdcand.subdm, \
spdcand.sigma, spdcand.sample_number, spdcand.duration, \
spdcand.width_bins, spdcand.pulse_width, rawdatafile.tsamp,\
rawdatafile.specinfo.T, spdcand.topo_start_time, data.starttime, \
data.dt,data.numspectra, data.freqs.min(), data.freqs.max()])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
zerodm=True
data, Data_dedisp_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
####Sweeped without zerodm
spdcand.read_from_file(values[ii], rawdatafile.tsamp, rawdatafile.specinfo.N, \
rawdatafile.frequencies[0], rawdatafile.frequencies[-1], \
rawdatafile, loc_pulse=loc_pulse, dedisp = None, \
scaleindep = None, zerodm = None, mask = mask, \
barytime=barytime, \
nsub = nsub, bandpass_corr = bandpass_corr)
data, Data_nozerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, spdcand.zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
text_array = np.append(text_array, spdcand.sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, spdcand.bary_start_time)
text_array = np.append(text_array, man_params)
# Array to Construct the sweep
if spdcand.sweep_dm is not None:
ddm = spdcand.sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
#downsamp_temp = 1
data, Data_zerodm = waterfall_array(rawdatafile, spdcand.start, \
spdcand.duration, spdcand.dm, spdcand.nbins, spdcand.nsub, \
spdcand.subdm, zerodm, spdcand.downsamp, \
spdcand.scaleindep, spdcand.width_bins, \
spdcand.mask, maskfile, spdcand.bandpass_corr)
# Saving the arrays into the .spd file.
with open(temp_filename+".spd", 'wb') as f:
np.savez_compressed(f, \
Data_dedisp_nozerodm = Data_dedisp_nozerodm.astype(np.float16),\
Data_dedisp_zerodm = Data_dedisp_zerodm.astype(np.float16),\
Data_nozerodm = Data_nozerodm.astype(np.float16),\
delays_nozerodm = delays_nozerodm, \
freqs_nozerodm = freqs_nozerodm,\
Data_zerodm = Data_zerodm.astype(np.float16), \
dm_arr= list(map(np.float16, dm_arr)),\
sigma_arr = list(map(np.float16, sigma_arr)), \
width_arr =list(map(np.uint8, width_arr)),\
dm_list= list(map(np.float16, dm_list)), \
time_list = list(map(np.float16, time_list)), \
text_array = text_array)
#### Arrays for Plotting DM vs Time is in plot_spd.plot(...)
if plot:
print_debug("Now plotting...")
plot_spd.plot(temp_filename+".spd", args[1:], \
spec_width=1.5, loc_pulse=loc_pulse, \
xwin=False, outfile=basename, \
just_waterfall=just_waterfall, \
integrate_spec=integrate_spec, \
integrate_ts=integrate_ts, \
disp_pulse=disp_pulse, tar = None)
print_debug("Finished plot %i " %ii+strftime("%Y-%m-%d %H:%M:%S"))
numcands+= 1
print_debug('Finished sp_candidate : %i'%numcands)
if numcands >= maxnumcands: # Max number of candidates to plot 100.
loop_must_break = True
break
if loop_must_break:
break
print_debug("Finished group %i... "%rank+strftime("%Y-%m-%d %H:%M:%S"))
print_debug("Finished running waterfaller... "+strftime("%Y-%m-%d %H:%M:%S"))
def inject(infile, outfn, prof, period, dm, nbitsout=None,
block_size=BLOCKSIZE, pulsar_only=False, inplace=False):
if isinstance(infile, filterbank.FilterbankFile):
fil = infile
elif inplace:
fil = filterbank.FilterbankFile(infile, 'readwrite')
else:
fil = filterbank.FilterbankFile(infile, 'read')
print("Injecting pulsar signal into: %s" % fil.filename)
if False:
delays = psr_utils.delay_from_DM(dm, fil.frequencies)
delays -= delays[np.argmax(fil.frequencies)]
get_phases = lambda times: (times-delays)/period % 1
else:
get_phases = lambda times: times/period % 1
# Create the output filterbank file
if nbitsout is None:
nbitsout = fil.nbits
if inplace:
warnings.warn("Injecting pulsar signal *in-place*")
outfil = fil
else:
# Start an output file
print("Creating out file: %s" % outfn)
outfil = filterbank.create_filterbank_file(outfn, fil.header, \
nbits=nbitsout, mode='append')
if outfil.nbits == 8:
raise NotImplementedError("This code is out of date. 'delays' is not " \
"done in this way anymore..")
# Read the first second of data to get the global scaling to use
onesec = fil.get_timeslice(0, 1).copy()
onesec_nspec = onesec.shape[0]
times = np.atleast_2d(np.arange(onesec_nspec)*fil.tsamp).T+delays
phases = times/period % 1
onesec += prof(phases)
minimum = np.min(onesec)
median = np.median(onesec)
# Set median to 1/3 of dynamic range
global_scale = (256.0/3.0) / median
del onesec
else:
# No scaling to be performed
# These values will cause scaling to keep data unchanged
minimum = 0
global_scale = 1
sys.stdout.write(" %3.0f %%\r" % 0)
sys.stdout.flush()
oldprogress = -1
# Loop over data
lobin = 0
spectra = fil.get_spectra(0, block_size)
numread = spectra.shape[0]
while numread:
if pulsar_only:
# Do not write out data from input file
# zero it out
spectra *= 0
hibin = lobin+numread
# Sample at middle of time bin
times = (np.arange(lobin, hibin, 1.0/NINTEG_PER_BIN)+0.5/NINTEG_PER_BIN)*fil.dt
#times = (np.arange(lobin, hibin)+0.5)*fil.dt
phases = get_phases(times)
profvals = prof(phases)
shape = list(profvals.shape)
shape[1:1] = [NINTEG_PER_BIN]
shape[0] /= NINTEG_PER_BIN
profvals.shape = shape
toinject = profvals.mean(axis=1)
#toinject = profvals
if np.ndim(toinject) > 1:
injected = spectra+toinject
else:
injected = spectra+toinject[:,np.newaxis]
scaled = (injected-minimum)*global_scale
if inplace:
outfil.write_spectra(scaled, lobin)
else:
outfil.append_spectra(scaled)
# Print progress to screen
progress = int(100.0*hibin/fil.nspec)
if progress > oldprogress:
sys.stdout.write(" %3.0f %%\r" % progress)
sys.stdout.flush()
oldprogress = progress
# Prepare for next iteration
lobin = hibin
spectra = fil.get_spectra(lobin, lobin+block_size)
numread = spectra.shape[0]
sys.stdout.write("Done \n")
sys.stdout.flush()
def main():
parser = optparse.OptionParser(prog="sp_pipeline..py", \
version=" Chitrang Patel (May. 12, 2015)", \
usage="%prog INFILE(PsrFits FILE, SINGLEPULSE FILES)", \
description="Create single pulse plots to show the " \
"frequency sweeps of a single pulse, " \
"DM vs time, and SNR vs DM,"\
"in psrFits data.")
parser.add_option('--infile', dest='infile', type='string', \
help="Give a .inf file to read the appropriate header information.")
parser.add_option('--groupsfile', dest='txtfile', type='string', \
help="Give the groups.txt file to read in the groups information.")
parser.add_option('--mask', dest='maskfile', type='string', \
help="Mask file produced by rfifind. (Default: No Mask).", \
default=None)
parser.add_option('-n', dest='maxnumcands', type='int', \
help="Maximum number of candidates to plot. (Default: 100).", \
default=100)
options, args = parser.parse_args()
if not hasattr(options, 'infile'):
raise ValueError("A .inf file must be given on the command line! ")
if not hasattr(options, 'txtfile'):
raise ValueError("The groups.txt file must be given on the command line! ")
files = get_textfile(options.txtfile)
print_debug("Begining waterfaller... "+strftime("%Y-%m-%d %H:%M:%S"))
if not args[0].endswith("fits"):
raise ValueError("The first file must be a psrFits file! ")
print_debug('Maximum number of candidates to plot: %i'%options.maxnumcands)
basename = args[0][:-5]
filetype = "psrfits"
inffile = options.infile
topo, bary = bary_and_topo.bary_to_topo(inffile)
time_shift = bary-topo
inf = infodata.infodata(inffile)
RA = inf.RA
dec = inf.DEC
MJD = inf.epoch
mjd = Popen(["mjd2cal", "%f"%MJD], stdout=PIPE, stderr=PIPE)
date, err = mjd.communicate()
date = date.split()[2:5]
telescope = inf.telescope
N = inf.N
numcands=0
Total_observed_time = inf.dt *N
print_debug('getting file..')
values = split_parameters(options.txtfile)
if len(values)> options.maxnumcands:
values=sorted(values, key=itemgetter(5,1)) #sorting candidates based on ranks and snr
values=values[-options.maxnumcands:]
print "More than", options.maxnumcands, "candidates, making plots for", options.maxnumcands, "candidates"
values = sorted(values, key=itemgetter(0))
for ii in range(len(values)):
#### Array for Plotting DM vs SNR
print_debug("Making arrays for DM vs Signal to Noise...")
temp_list = files[values[ii][6]-6].split()
npulses = int(temp_list[2])
temp_lines = files[(values[ii][6]+3):(values[ii][6]+npulses+1)]
arr = np.split(temp_lines, len(temp_lines))
dm_list = []
time_list = []
for i in range(len(arr)):
dm_val= float(arr[i][0].split()[0])
time_val = float(arr[i][0].split()[2])
dm_list.append(dm_val)
time_list.append(time_val)
arr_2 = np.array([arr[i][0].split() for i in range(len(arr))], dtype = np.float32)
dm_arr = np.array([arr_2[i][0] for i in range(len(arr))], dtype = np.float32)
sigma_arr = np.array([arr_2[i][1] for i in range(len(arr))], dtype = np.float32)
#### Array for Plotting DM vs Time is in show_spplots.plot(...)
#### Setting variables up for the waterfall arrays.
j = ii+1
subdm = dm = sweep_dm= values[ii][0]
sample_number = values[ii][3]
rank=values[ii][5]
width_bins = values[ii][4]
#print "dm", dm
#print "width_bins", width_bins
downsamp = np.round((values[ii][2]/sample_number/inf.dt)).astype('int')
#print "downsamp", downsamp
pulse_width = width_bins*downsamp*inf.dt
#print "pulse_width", pulse_width
if ii == 0:
mask_subband=rfifind.rfifind("%s_rfifind.mask"%(basename))
mask_subband.set_zap_chans(power=1000,plot=False)
mask_subband.set_weights_and_offsets()
mask_subband.write_weights(filename="%s_weights.txt"%(basename))
cmd="psrfits_subband -dm %.2f -nsub 128 -o %s_subband_%.2f -weights %s_weights.txt %s"%(dm,basename,dm,basename,args[0])
call(cmd, shell=True)
#subband args[0] at dm and then generate a file that will be set equal to rawdatafile
subband_file="%s_subband_%.2f_0001.fits" %(basename,dm)
dm_prev=dm
subband_prev= subband_file
else:
dm_diff=dm-dm_prev
t_smear=8.3e3*dm_diff*(350**-3)*(np.abs(rawdatafile.frequencies[0]-rawdatafile.frequencies[-1])/128.)
if (5*t_smear) > pulse_width:
cmd="psrfits_subband -dm %.2f -nsub 128 -o %s_subband_%.2f -weights %s_weights.txt %s"%(dm,basename,dm,basename,args[0])
call(cmd, shell=True)
#subband args[0] at dm and then generate a file that will be set equal to rawdatafile
subband_file="%s_subband_%.2f_0001.fits" %(basename,dm)
dm_prev=dm
subband_prev=subband_file
rawdatafile = psrfits.PsrfitsFile(subband_file)
bin_shift = np.round(time_shift/rawdatafile.tsamp).astype('int')
integrate_dm = None
sigma = values[ii][1]
sweep_posn = 0.0
bary_start_time = values[ii][2]
topo_start_time = bary_start_time - topo_timeshift(bary_start_time, time_shift, topo)[0]
binratio = 50
scaleindep = False
zerodm = None
duration = binratio * width_bins * rawdatafile.tsamp * downsamp
start = topo_start_time - (0.25 * duration)
if (start<0.0):
start = 0.0
if sigma <= 7:
nsub = 32
elif sigma >= 7 and sigma < 10:
nsub = 64
else:
nsub = 128
nbins = np.round(duration/rawdatafile.tsamp).astype('int')
start_bin = np.round(start/rawdatafile.tsamp).astype('int')
dmfac = 4.15e3 * np.abs(1./rawdatafile.frequencies[0]**2 - 1./rawdatafile.frequencies[-1]**2)
nbinsextra = np.round((duration + dmfac * dm)/rawdatafile.tsamp).astype('int')
if (start_bin+nbinsextra) > N-1:
nbinsextra = N-1-start_bin
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
#make an array to store header information for the .npz files
temp_filename = basename+"_DM%.1f_%.1fs_rank_%i"%(subdm, topo_start_time, rank)
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
print_debug("Running waterfaller with Zero-DM OFF...")
data, Data_dedisp_nozerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp, scaleindep, width_bins, rawdatafile, binratio, data)
#Add additional information to the header information array
text_array = np.array([subband_file, 'GBT', RA, dec, MJD, rank, nsub, nbins, subdm, sigma, sample_number, duration, width_bins, pulse_width, rawdatafile.tsamp, Total_observed_time, topo_start_time, data.starttime, data.dt, data.numspectra, data.freqs.min(), data.freqs.max()])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
#print "before get_spectra",memory.resident()/(1024.0**3)
data = rawdatafile.get_spectra(start_bin, nbinsextra)
#print "after get_spectra",memory.resident()/(1024.0**3)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
zerodm = True
data, Data_dedisp_zerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp, scaleindep, width_bins, rawdatafile, binratio, data)
#print "waterfall",memory.resident()/(1024.0**3)
####Sweeped without zerodm
start = start + (0.25*duration)
start_bin = np.round(start/rawdatafile.tsamp).astype('int')
sweep_duration = 4.15e3 * np.abs(1./rawdatafile.frequencies[0]**2-1./rawdatafile.frequencies[-1]**2)*sweep_dm
nbins = np.round(sweep_duration/(rawdatafile.tsamp)).astype('int')
if ((nbins+start_bin)> (N-1)):
nbins = N-1-start_bin
#print "before get_spectra",memory.resident()/(1024.0**3)
data = rawdatafile.get_spectra(start_bin, nbins)
#print "after get_spectra",memory.resident()/(1024.0**3)
data = maskdata(data, start_bin, nbins, options.maskfile)
zerodm = None
dm = None
data, Data_nozerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp, scaleindep, width_bins, rawdatafile, binratio, data)
#print "waterfall",memory.resident()/(1024.0**3)
text_array = np.append(text_array, sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, bary_start_time)
# Array to Construct the sweep
if sweep_dm is not None:
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
downsamp_temp = 1
data, Data_zerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp_temp, scaleindep, width_bins, rawdatafile, binratio, data)
#print "waterfall",memory.resident()/(1024.0**3)
# Saving the arrays into the .spd file.
with open(temp_filename+".spd", 'wb') as f:
np.savez_compressed(f, Data_dedisp_nozerodm = Data_dedisp_nozerodm.astype(np.float16), Data_dedisp_zerodm = Data_dedisp_zerodm.astype(np.float16), Data_nozerodm = Data_nozerodm.astype(np.float16), delays_nozerodm = delays_nozerodm, freqs_nozerodm = freqs_nozerodm, Data_zerodm = Data_zerodm.astype(np.float16), dm_arr= map(np.float16, dm_arr), sigma_arr = map(np.float16, sigma_arr), dm_list= map(np.float16, dm_list), time_list = map(np.float16, time_list), text_array = text_array)
print_debug("Now plotting...")
#print "Before plot..",memory.resident()/(1024.0**3)
show_spplots.plot(temp_filename+".spd", args[1:], xwin=False, outfile = basename, tar = None)
print_debug("Finished plot %i " %j+strftime("%Y-%m-%d %H:%M:%S"))
#print "After plot..",memory.resident()/(1024.0**3)
numcands+=1
print_debug('Finished sp_candidate : %i'%numcands)
print_debug("Finished running waterfaller... "+strftime("%Y-%m-%d %H:%M:%S"))
def main():
parser = optparse.OptionParser(prog="sp_pipeline..py", \
version=" Chitrang Patel (May. 12, 2015)", \
usage="%prog INFILE(PsrFits FILE, SINGLEPULSE FILES)", \
description="Create single pulse plots to show the " \
"frequency sweeps of a single pulse, " \
"DM vs time, and SNR vs DM,"\
"in psrFits data.")
parser.add_option('--infile', dest='infile', type='string', \
help="Give a .inf file to read the appropriate header information.")
parser.add_option('--groupsfile', dest='txtfile', type='string', \
help="Give the groups.txt file to read in the groups information.")
parser.add_option('--mask', dest='maskfile', type='string', \
help="Mask file produced by rfifind. (Default: No Mask).", \
default=None)
parser.add_option('-n', dest='maxnumcands', type='int', \
help="Maximum number of candidates to plot. (Default: 100).", \
default=100)
options, args = parser.parse_args()
if not hasattr(options, 'infile'):
raise ValueError("A .inf file must be given on the command line! ")
if not hasattr(options, 'txtfile'):
raise ValueError("The groups.txt file must be given on the command line! ")
files = sp_utils.spio.get_textfile(options.txtfile)
print_debug("Begining waterfaller... "+strftime("%Y-%m-%d %H:%M:%S"))
if not args[0].endswith("fits"):
raise ValueError("The first file must be a psrFits file! ")
print_debug('Maximum number of candidates to plot: %i'%options.maxnumcands)
basename = args[0][:-5]
filetype = "psrfits"
inffile = options.infile
topo, bary = bary_and_topo.bary_to_topo(inffile)
time_shift = bary-topo
inf = infodata.infodata(inffile)
RA = inf.RA
dec = inf.DEC
MJD = inf.epoch
mjd = Popen(["mjd2cal", "%f"%MJD], stdout=PIPE, stderr=PIPE)
date, err = mjd.communicate()
date = date.split()[2:5]
telescope = inf.telescope
N = inf.N
Total_observed_time = inf.dt *N
print_debug('getting file..')
rawdatafile = psrfits.PsrfitsFile(args[0])
bin_shift = np.round(time_shift/rawdatafile.tsamp).astype('int')
numcands = 0 # candidate counter. Use this to decide the maximum bumber of candidates to plot.
loop_must_break = False # dont break the loop unless num of cands >100.
for group in [6, 5, 4, 3, 2]:
rank = group+1
if files[group] != "Number of rank %i groups: 0 "%rank:
print_debug(files[group])
values = sp_utils.spio.split_parameters(rank, options.txtfile)
lis = np.where(files == '\tRank: %i.000000'%rank)[0]
for ii in range(len(values)):
#### Array for Plotting DM vs SNR
print_debug("Making arrays for DM vs Signal to Noise...")
temp_list = files[lis[ii]-6].split()
npulses = int(temp_list[2])
temp_lines = files[(lis[ii]+3):(lis[ii]+npulses+1)]
arr = np.split(temp_lines, len(temp_lines))
dm_list = []
time_list = []
for i in range(len(arr)):
dm_val= float(arr[i][0].split()[0])
time_val = float(arr[i][0].split()[2])
dm_list.append(dm_val)
time_list.append(time_val)
arr_2 = np.array([arr[i][0].split() for i in range(len(arr))], dtype = np.float32)
dm_arr = np.array([arr_2[i][0] for i in range(len(arr))], dtype = np.float32)
sigma_arr = np.array([arr_2[i][1] for i in range(len(arr))], dtype = np.float32)
#### Array for Plotting DM vs Time is in show_spplots.plot(...)
#### Setting variables up for the waterfall arrays.
j = ii+1
subdm = dm = sweep_dm= values[ii][0]
integrate_dm = None
sigma = values[ii][1]
sweep_posn = 0.0
bary_start_time = values[ii][2]
topo_start_time = bary_start_time - topo_timeshift(bary_start_time, time_shift, topo)[0]
sample_number = values[ii][3]
width_bins = values[ii][4]
binratio = 50
scaleindep = False
zerodm = None
downsamp = np.round((values[ii][2]/sample_number/rawdatafile.tsamp)).astype('int')
duration = binratio * width_bins * rawdatafile.tsamp * downsamp
start = topo_start_time - (0.25 * duration)
if (start<0.0):
start = 0.0
pulse_width = width_bins*downsamp*rawdatafile.tsamp
if sigma < 10:
nsub = 32
elif sigma >= 10 and sigma < 15:
nsub = 64
else:
nsub = 96
if nsub > inf.numchan:
nsub = inf.numchan
nbins = np.round(duration/rawdatafile.tsamp).astype('int')
start_bin = np.round(start/rawdatafile.tsamp).astype('int')
dmfac = 4.15e3 * np.abs(1./rawdatafile.frequencies[0]**2 - 1./rawdatafile.frequencies[-1]**2)
nbinsextra = np.round((duration + dmfac * dm)/rawdatafile.tsamp).astype('int')
if (start_bin+nbinsextra) > N-1:
nbinsextra = N-1-start_bin
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
#make an array to store header information for the .npz files
temp_filename = basename+"_DM%.1f_%.1fs_rank_%i"%(subdm, topo_start_time, rank)
# Array for Plotting Dedispersed waterfall plot - zerodm - OFF
print_debug("Running waterfaller with Zero-DM OFF...")
data, Data_dedisp_nozerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp, scaleindep, width_bins, rawdatafile, binratio, data)
# Add additional information to the header information array
text_array = np.array([args[0], 'Arecibo', RA, dec, MJD, rank, nsub, nbins, subdm, sigma, sample_number, duration, width_bins, pulse_width, rawdatafile.tsamp, Total_observed_time, topo_start_time, data.starttime, data.dt, data.numspectra, data.freqs.min(), data.freqs.max()])
#### Array for plotting Dedispersed waterfall plot zerodm - ON
print_debug("Running Waterfaller with Zero-DM ON...")
data = rawdatafile.get_spectra(start_bin, nbinsextra)
data = maskdata(data, start_bin, nbinsextra, options.maskfile)
zerodm = True
data, Data_dedisp_zerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp, scaleindep, width_bins, rawdatafile, binratio, data)
####Sweeped without zerodm
start = start + (0.25*duration)
start_bin = np.round(start/rawdatafile.tsamp).astype('int')
sweep_duration = 4.15e3 * np.abs(1./rawdatafile.frequencies[0]**2-1./rawdatafile.frequencies[-1]**2)*sweep_dm
nbins = np.round(sweep_duration/(rawdatafile.tsamp)).astype('int')
if ((nbins+start_bin)> (N-1)):
nbins = N-1-start_bin
data = rawdatafile.get_spectra(start_bin, nbins)
data = maskdata(data, start_bin, nbins, options.maskfile)
zerodm = None
dm = None
data, Data_nozerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp, scaleindep, width_bins, rawdatafile, binratio, data)
text_array = np.append(text_array, sweep_duration)
text_array = np.append(text_array, data.starttime)
text_array = np.append(text_array, bary_start_time)
# Array to Construct the sweep
if sweep_dm is not None:
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
delays_nozerodm = delays
freqs_nozerodm = data.freqs
# Sweeped with zerodm-on
zerodm = True
downsamp_temp = 1
data, Data_zerodm = waterfall_array(start_bin, dmfac, duration, nbins, zerodm, nsub, subdm, dm, integrate_dm, downsamp_temp, scaleindep, width_bins, rawdatafile, binratio, data)
# Saving the arrays into the .spd file.
with open(temp_filename+".spd", 'wb') as f:
np.savez_compressed(f, Data_dedisp_nozerodm = Data_dedisp_nozerodm.astype(np.float16), Data_dedisp_zerodm = Data_dedisp_zerodm.astype(np.float16), Data_nozerodm = Data_nozerodm.astype(np.float16), delays_nozerodm = delays_nozerodm, freqs_nozerodm = freqs_nozerodm, Data_zerodm = Data_zerodm.astype(np.float16), dm_arr= map(np.float16, dm_arr), sigma_arr = map(np.float16, sigma_arr), dm_list= map(np.float16, dm_list), time_list = map(np.float16, time_list), text_array = text_array)
print_debug("Now plotting...")
show_spplots.plot(temp_filename+".spd", args[1:], xwin=False, outfile = basename, tar = None)
print_debug("Finished plot %i " %j+strftime("%Y-%m-%d %H:%M:%S"))
numcands+= 1
print_debug('Finished sp_candidate : %i'%numcands)
if numcands >= options.maxnumcands: # Max number of candidates to plot 100.
loop_must_break = True
break
if loop_must_break:
break
print_debug("Finished group %i... "%rank+strftime("%Y-%m-%d %H:%M:%S"))
print_debug("Finished running waterfaller... "+strftime("%Y-%m-%d %H:%M:%S"))
def plot_waterfall(data, start, source_name, duration, dm,ofile,
integrate_ts=False, integrate_spec=False, show_cb=False,
cmap_str="gist_yarg", sweep_dms=[], sweep_posns=[],
ax_im=None, ax_ts=None, ax_spec=None, interactive=True, downsamp=1,nsub=None,subdm=None,width=None, snr=None):
""" I want a docstring too!
"""
if source_name is None:
source_name="Unknown"
#Output file
if ofile is "unknown_cand":
title = "%s_" + ofile + "_%.3f_%s" % (source_name,start,str(dm))
else: title=source_name + "_" + ofile
# Set up axes
fig = plt.figure(figsize=(10,14))
#fig.canvas.set_window_title("Frequency vs. Time")
'''
im_width = 0.6 if integrate_spec else 0.8
im_height = 0.6 if integrate_ts else 0.8
if not ax_im:
ax_im = plt.axes((0.15, 0.15, im_width, im_height))
if integrate_ts and not ax_ts:
ax_ts = plt.axes((0.15, 0.75, im_width, 0.2),sharex=ax_im)
if integrate_spec and not ax_spec:
ax_spec = plt.axes((0.75, 0.15, 0.2, im_height),sharey=ax_im)
'''
ax_ts = plt.axes((0.15, 0.835, 0.8, 0.145))
ax_im = plt.axes((0.15, 0.59, 0.8, 0.24), sharex=ax_ts)
ax_dmvstm = plt.axes((0.15, 0.345, 0.8, 0.24), sharex=ax_ts)
ax_orig = plt.axes((0.15, 0.1,0.8, 0.21))
data.downsample(downsamp)
nbinlim = np.int(duration/data.dt)
# DM-vs-time plot
dmvstm_array = []
lodm = int(dm-(dm*0.15))
if lodm < 0: lodm = 0
hidm = int(dm+(dm*0.15))
dmstep = (hidm-lodm)/50.0
datacopy = copy.deepcopy(data)
#print lodm,hidm
for ii in np.arange(lodm,hidm,dmstep):
#for ii in range(400,600,10):
#Without this, dispersion delay with smaller DM step does not produce delay close to bin width
data.dedisperse(0,padval='rotate')
data.dedisperse(ii,padval='rotate')
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
dmvstm_array.append(Dedisp_ts)
dmvstm_array=np.array(dmvstm_array)
#print np.shape(dmvstm_array)
#np.save('dmvstm_1step.npz',dmvstm_array)
ax_dmvstm.set_xlabel("Time (sec) ")
ax_dmvstm.set_ylabel("DM")
#ax_dmvstm.imshow(dmvstm_array, aspect='auto', cmap=matplotlib.cm.cmap_d[cmap_str], origin='lower',extent=(data.starttime, data.starttime+ nbinlim*data.dt, lodm, hidm))
ax_dmvstm.imshow(dmvstm_array, aspect='auto', origin='lower',extent=(data.starttime, data.starttime+ nbinlim*data.dt, lodm, hidm))
#cmap=matplotlib.cm.cmap_d[cmap_str])
#interpolation='nearest', origin='upper')
plt.setp(ax_im.get_xticklabels(), visible = False)
plt.setp(ax_ts.get_xticklabels(), visible = False)
#extent=(data.starttime, data.starttime+ nbinlim*data.dt, 500, 700)
#plt.show()
#fig2 = plt.figure(2)
#plt.imshow(dmvstm_array,aspect='auto')
#Plot Freq-vs-time
data = copy.deepcopy(datacopy)
#data.downsample(downsamp)
data.dedisperse(dm,padval='rotate')
nbinlim = np.int(duration/data.dt)
img = ax_im.imshow(data.data[..., :nbinlim], aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime+ nbinlim*data.dt, \
data.freqs.min(), data.freqs.max()))
if show_cb:
cb = ax_im.get_figure().colorbar(img)
cb.set_label("Scaled signal intensity (arbitrary units)")
# Dressing it up
ax_im.xaxis.get_major_formatter().set_useOffset(False)
#ax_im.set_xlabel("Time")
ax_im.set_ylabel("Frequency (MHz)")
# Plot Time series
#Data = np.array(data.data[..., :nbinlim])
Data = np.array(data.data[..., :nbinlim])
Dedisp_ts = Data.sum(axis=0)
times = (np.arange(data.numspectra)*data.dt + start)[..., :nbinlim]
ax_ts.plot(times, Dedisp_ts,"k")
ax_ts.set_xlim([times.min(),times.max()])
text1 = "DM: " + "%.2f" % float(data.dm)
plt.text(0.1,0.9,text1,fontsize=12,ha='center', va='center', transform=ax_ts.transAxes)
text2 = "Width: " + "%.2f" % float(width)
plt.text(0.1,0.8,text2,fontsize=12,ha='center', va='center', transform=ax_ts.transAxes)
text3 = "SNR: " + "%.2f" % float(snr)
plt.text(0.1,0.7,text3,fontsize=12,ha='center', va='center', transform=ax_ts.transAxes)
ax_ts.set_title(title,fontsize=12)
plt.setp(ax_ts.get_xticklabels(), visible = False)
plt.setp(ax_ts.get_yticklabels(), visible = False)
#Plot original data
data.dedisperse(0,padval='rotate')
ax_im.set_ylabel("Frequency (MHz)")
ax_orig.set_ylabel("Frequency (MHz)")
ax_orig.set_xlabel("Time (sec)")
# Sweeping it up
for ii, sweep_dm in enumerate(sweep_dms):
ddm = sweep_dm-data.dm
delays = psr_utils.delay_from_DM(ddm, data.freqs)
delays -= delays.min()
if sweep_posns is None:
sweep_posn = 0.0
elif len(sweep_posns) == 1:
sweep_posn = sweep_posns[0]
else:
sweep_posn = sweep_posns[ii]
sweepstart = data.dt*data.numspectra*sweep_posn+data.starttime
#sty = SWEEP_STYLES[ii%len(SWEEP_STYLES)]
sty="b-"
ax_orig.plot(delays+sweepstart, data.freqs, "b-", lw=2, alpha=0.7)
ax_orig.plot(delays+sweepstart+duration, data.freqs, "b-", lw=2, alpha=0.7)
ax_orig.imshow(data.data, aspect='auto', \
cmap=matplotlib.cm.cmap_d[cmap_str], \
interpolation='nearest', origin='upper', \
extent=(data.starttime, data.starttime + len(data.data[0])*data.dt, \
data.freqs.min(), data.freqs.max()))
#if interactive:
# fig.suptitle("Frequency vs. Time")
# fig.canvas.mpl_connect('key_press_event', \
# lambda ev: (ev.key in ('q','Q') and plt.close(fig)))
#oname = "%.3f_%s.png" % (start,str(dm))
if ofile is "unknown_cand":
plt.savefig(ofile)
ofile = ofile + "_%.3f_%s.png" % (start,str(dm))
else: plt.savefig(ofile)
