def toafft(toas, freqs, days=0):
if days:
toas = (toas - toas[0]) * 86400.0
else:
toas = toas - toas[0]
twid = zeros(len(freqs), 'D')
twid.imag = -2.0 * pi * freqs
return spectralpower(add.reduce(exp(\
multiply.outer(toas, twid)))) / len(toas)
print "Computing harmonic", harmnum
ldr = dr * harmnum
ldz = dz * harmnum
lor = startr * harmnum
loz = 0.0 - (numzs-1)/2 * ldz
rs = N.arange(numrs) * ldr + lor
zs = N.arange(numzs) * ldz + loz
if harmnum==1:
rs0, zs0 = rs[:], zs[:]
lo_file_r = int(rs.min()) - 1000
hi_file_r = int(rs.max()) + 1000
# Read and normalize the raw spectrum
infile.seek(lo_file_r * 8, 0)
fftamps = fread(infile, hi_file_r-lo_file_r+1, 'F')
fftpows = spectralpower(fftamps)
pownorm = 1.0 / (1.442695 * N.median(fftpows))
fftamps *= sqrt(pownorm)
ffd = ffdot_plane(fftamps, lor-lo_file_r, ldr, numrs, loz, ldz, numzs)
ffd_pows = (ffd * ffd.conj()).real
ffdps.append(ffd_pows)
if (harmnum==1):
sumpows = N.zeros_like(ffd_pows)
sumpows += ffd_pows
argmax = ffd_pows.argmax()
maxvals.append(ffd_pows.max())
maxargs.append((argmax / numrs, argmax % numrs))
print " Maximum power for harmonic %d = %.2f"%(harmnum, maxvals[-1])
a = presto.gen_cvect(1024 * 16384)
del a
print "success"
print "Testing psrparams and orbitparams stuff...",
psr = presto.psrepoch("J0737-3039A", 56000.0, verbose=False)
assert(round(psr.dm-48.92, 7)==0)
# This needs to change when we start using the actual psrcat.db file
print "\nTODO: fix the precision of the values in the catalog!!"
assert(round(psr.orb.p-8838.72, 7)==0)
#assert(round(psr.orb.p-8834.534998272, 7)==0)
print "success"
print "Testing spectralpower and spectralphase...",
a = np.arange(5.0) + complex(0.0, 1.0)
assert(np.allclose(presto.spectralpower(a),
np.arange(5.0)**2.0 + 1))
assert(np.allclose(presto.spectralphase(a),
np.array([90., 45., 26.56505203, 18.43494797, 14.03624344])))
print "success"
print "Testing vector shifting / rotation...",
a = np.arange(4, dtype=np.float32)
presto.frotate(a, 1)
assert(np.allclose(a, np.array([1, 2, 3, 0])))
a = np.arange(4, dtype=np.float64)
presto.drotate(a, 1)
assert(np.allclose(a, np.array([1, 2, 3, 0])))
print "success"
print "Testing orbit integration stuff...",
print ' Orbit z =', \
presto.TWOPI*psr.orb.x/psr.p
print ''
# Create the data set
cand = presto.orbitparams()
m = 0
comb = presto.gen_bin_response(0.0, 1, psr.p, T, psr.orb ,
presto.LOWACC, m)
ind = len(comb)
# The follwoing is performed automatically in gen_bin_resp() now
# m = (ind / 2 + 10) * numbetween
data = Numeric.zeros(3 * ind, 'F')
data[ind:2*ind] = comb
if showplots and not parallel:
Pgplot.plotxy(presto.spectralpower(data), color='red',
title='Data', labx='Fourier Frequency',
laby='Relative Power')
a = raw_input("Press enter to continue...")
Pgplot.nextplotpage(1)
# Perform the loops over the Keplarian parameters
for job in range(numjobs):
if parallel:
myjob = work[myid]
else:
myjob = work[job]
if myjob=='p':
Dd = Dp
psrref = psr.orb.p
if myjob=='x':
print ' Orbit z =', \
presto.TWOPI*psr.orb.x/psr.p
print ''
# Create the data set
cand = presto.orbitparams()
m = 0
comb = presto.gen_bin_response(0.0, 1, psr.p, T, psr.orb ,
presto.LOWACC, m)
ind = len(comb)
# The follwoing is performed automatically in gen_bin_resp() now
# m = (ind / 2 + 10) * numbetween
data = Numeric.zeros(3 * ind, 'F')
data[ind:2*ind] = comb
if showplots and not parallel:
Pgplot.plotxy(presto.spectralpower(data), color='red',
title='Data', labx='Fourier Frequency',
laby='Relative Power')
a = raw_input("Press enter to continue...")
Pgplot.nextplotpage(1)
# Perform the loops over the Keplerian parameters
for job in range(numjobs):
if parallel:
myjob = work[myid]
else:
myjob = work[job]
if myjob=='p':
Dd = Dp
psrref = psr.orb.p
if myjob=='x':
a = presto.gen_cvect(1024 * 16384)
del a
print "success"
print "Testing psrparams and orbitparams stuff...",
psr = presto.psrepoch("J0737-3039A", 56000.0, verbose=False)
assert (round(psr.dm - 48.92, 7) == 0)
# This needs to change when we start using the actual psrcat.db file
print "\nTODO: fix the precision of the values in the catalog!!"
assert (round(psr.orb.p - 8838.72, 7) == 0)
#assert(round(psr.orb.p-8834.534998272, 7)==0)
print "success"
print "Testing spectralpower and spectralphase...",
a = np.arange(5.0) + complex(0.0, 1.0)
assert (np.allclose(presto.spectralpower(a), np.arange(5.0)**2.0 + 1))
assert (np.allclose(
presto.spectralphase(a),
np.array([90., 45., 26.56505203, 18.43494797, 14.03624344])))
print "success"
print "Testing vector shifting / rotation...",
a = np.arange(4, dtype=np.float32)
presto.frotate(a, 1)
assert (np.allclose(a, np.array([1, 2, 3, 0])))
a = np.arange(4, dtype=np.float64)
presto.drotate(a, 1)
assert (np.allclose(a, np.array([1, 2, 3, 0])))
print "success"
print "Testing orbit integration stuff...",
dr = 1.0 / 32.0
dz = 0.18
np = 512 # number of pixels across for f-fdot image
z = 0.0 # average fourier f-dot
w = 0.0 # fourier freq double deriv
noise = 0.0
#noise = 4*num.random.standard_normal(N)
us = num.arange(N, dtype=num.float64) / N # normalized time coordinate
r0 = r - 0.5 * z + w / 12.0 # Make symmetric for all z and w
z0 = z - 0.5 * w
phss = 2.0 * num.pi * (us * (us * (us * w / 6.0 + z0 / 2.0) + r0))
ft = presto.rfft(num.cos(phss) + noise)
ffdot = presto.ffdot_plane(ft, rint - np / 2 * dr, dr, np, 0.0 - np / 2 * dz,
dz, np)
pffdot = presto.spectralpower(ffdot.flat)
theo_max_pow = N**2.0 / 4.0
frp = max(pffdot) / theo_max_pow # Fraction of recovered power
print("Fraction of recovered signal power = %f" % frp)
# print "Raw power should be ~%.2e" % theo_max_pow
pffdot = pffdot / theo_max_pow
pffdot.shape = (np, np)
rs = num.arange(np) * dr - np / 2 * dr
zs = num.arange(np) * dz - np / 2 * dz
rgx = num.asarray([rs[0], rs[np - 1]])
rgy = num.asarray([zs[0], zs[np - 1]])
freqcut = pffdot[np / 2, :]
fdotcut = pffdot[:, np / 2]
image = 'antirainbow'
device = 'ffdot_combined.eps/VCPS'
print(' Orbit Fourier Freq =', T / psr.orb.p)
print(' Orbit z =', \
presto.TWOPI*psr.orb.x/psr.p)
print('')
# Create the data set
cand = presto.orbitparams()
m = 0
comb = presto.gen_bin_response(0.0, 1, psr.p, T, psr.orb, presto.LOWACC, m)
ind = len(comb)
# The follwoing is performed automatically in gen_bin_resp() now
# m = (ind / 2 + 10) * numbetween
data = Numeric.zeros(3 * ind, 'F')
data[ind:2 * ind] = comb
if showplots and not parallel:
Pgplot.plotxy(presto.spectralpower(data),
color='red',
title='Data',
labx='Fourier Frequency',
laby='Relative Power')
a = input("Press enter to continue...")
Pgplot.nextplotpage(1)
# Perform the loops over the Keplerian parameters
for job in range(numjobs):
if parallel:
myjob = work[myid]
else:
myjob = work[job]
if myjob == 'p':
Dd = Dp
us = num.arange(N, dtype=num.float64) / N # normalized time coordinate
r0 = r - 0.5 * z + w / 12.0 # Make symmetric for all z and w
z0 = z - 0.5 * w
phss = 2.0 * num.pi * (us * (us * (us * w / 6.0 + z0 / 2.0) + r0))
ft = presto.rfft(num.cos(phss) + noise)
a = time.clock()
vol = presto.fdotdot_vol(ft, rint - np / 2 * dr, dr, np, 0.0 - np / 2 * dz, dz,
np, 0.0 - np / 2 * dw, dw, np)
print "First jerk vol took %.3f s" % (time.clock() - a)
a = time.clock()
vol = presto.fdotdot_vol(ft, rint - np / 2 * dr, dr, np, 0.0 - np / 2 * dz, dz,
np, 0.0 - np / 2 * dw, dw, np)
print "Second jerk vol took %.3f s" % (time.clock() - a)
pvol = presto.spectralpower(vol.flat)
theo_max_pow = N**2.0 / 4.0
frp = max(pvol) / theo_max_pow # Fraction of recovered power
print "Fraction of recovered signal power = %f" % frp
[maxpow, rmax, zmax,
rd] = presto.maximize_rz(ft,
r + num.random.standard_normal(1)[0] / 5.0,
z + num.random.standard_normal(1)[0],
norm=1.0)
print r, rmax, z, zmax, theo_max_pow, maxpow
# print "Raw power should be ~%.2e" % theo_max_pow
pvol = pvol / theo_max_pow
pvol.shape = (np, np, np)
rs = num.arange(np) * dr - np / 2 * dr
zs = num.arange(np) * dz - np / 2 * dz
ws = num.arange(np) * dw - np / 2 * dw
rint = num.floor(r)
dr = 1.0/32.0
dz = 0.18
np = 512 # number of pixels across for f-fdot image
z = 10.0 # average fourier f-dot
w = -40.0 # fourier freq double deriv
noise = 0.0
noise = 1.0*norm(N)
us = num.arange(N, dtype=num.float64) / N # normalized time coordinate
r0 = r - 0.5 * z + w / 12.0 # Make symmetric for all z and w
z0 = z - 0.5 * w
phss = 2.0 * num.pi * (us * (us * (us * w/6.0 + z0/2.0) + r0))
ft = presto.rfft(num.cos(phss)+noise)
ffdot = presto.ffdot_plane(ft, rint-np/2*dr, dr, np, 0.0-np/2*dz, dz, np)
pffdot = presto.spectralpower(ffdot.flat)
theo_max_pow = N**2.0/4.0
frp = max(pffdot) / theo_max_pow # Fraction of recovered power
print "Fraction of recovered signal power = %f" % frp
a = time.clock()
[maxpow, rmax, zmax, rd] = presto.maximize_rz(ft, r+norm(1)[0]/5.0,
z+norm(1)[0], norm=1.0)
print "Time for rz:", time.clock()-a
print r, rmax, z, zmax, theo_max_pow, maxpow
a = time.clock()
[maxpow, rmax, zmax, wmax, rd] = presto.maximize_rzw(ft, r+norm(1)[0]/5.0,
z+norm(1)[0],
w+norm(1)[0]*5.0,
norm=1.0)
print "Time for rzw:", time.clock()-a
print r, rmax, z, zmax, w, wmax, theo_max_pow, maxpow
print "Computing harmonic", harmnum
ldr = dr * harmnum
ldz = dz * harmnum
lor = startr * harmnum
loz = 0.0 - (numzs - 1) / 2 * ldz
rs = N.arange(numrs) * ldr + lor
zs = N.arange(numzs) * ldz + loz
if harmnum == 1:
rs0, zs0 = rs[:], zs[:]
lo_file_r = int(rs.min()) - 1000
hi_file_r = int(rs.max()) + 1000
# Read and normalize the raw spectrum
infile.seek(lo_file_r * 8, 0)
fftamps = N.fromfile(infile, 'F', hi_file_r - lo_file_r + 1)
fftpows = spectralpower(fftamps)
pownorm = 1.0 / (1.442695 * N.median(fftpows))
fftamps *= sqrt(pownorm)
ffd = ffdot_plane(fftamps, lor - lo_file_r, ldr, numrs, loz, ldz, numzs)
ffd_pows = (ffd * ffd.conj()).real
ffdps.append(ffd_pows)
if (harmnum == 1):
sumpows = N.zeros_like(ffd_pows)
sumpows += ffd_pows
argmax = ffd_pows.argmax()
maxvals.append(ffd_pows.max())
maxargs.append((argmax / numrs, argmax % numrs))
print " Maximum power for harmonic %d = %.2f" % (harmnum, maxvals[-1])
r0 = r - 0.5 * z + w / 12.0 # Make symmetric for all z and w
z0 = z - 0.5 * w
phss = 2.0 * num.pi * (us * (us * (us * w/6.0 + z0/2.0) + r0))
ft = presto.rfft(num.cos(phss)+noise)
a = time.clock()
vol = presto.fdotdot_vol(ft, rint-np/2*dr, dr, np,
0.0-np/2*dz, dz, np,
0.0-np/2*dw, dw, np)
print "First jerk vol took %.3f s" % (time.clock()-a)
a = time.clock()
vol = presto.fdotdot_vol(ft, rint-np/2*dr, dr, np,
0.0-np/2*dz, dz, np,
0.0-np/2*dw, dw, np)
print "Second jerk vol took %.3f s" % (time.clock()-a)
pvol = presto.spectralpower(vol.flat)
theo_max_pow = N**2.0/4.0
frp = max(pvol) / theo_max_pow # Fraction of recovered power
print "Fraction of recovered signal power = %f" % frp
[maxpow, rmax, zmax, rd] = presto.maximize_rz(ft, r+num.random.standard_normal(1)[0]/5.0,
z+num.random.standard_normal(1)[0], norm=1.0)
print r, rmax, z, zmax, theo_max_pow, maxpow
# print "Raw power should be ~%.2e" % theo_max_pow
pvol = pvol / theo_max_pow
pvol.shape = (np, np, np)
rs = num.arange(np) * dr - np/2*dr
zs = num.arange(np) * dz - np/2*dz
ws = num.arange(np) * dw - np/2*dw
rgx = num.asarray([rs[0], rs[np-1]])
rgy = num.asarray([zs[0], zs[np-1]])
from presto import spectralpower
from periodogram import *
from time import clock
file = 'rosat_crab_3k.toa'
toas = ravel(readColumns(file, '#'))
toas = (toas - toas[0]) * 86400.0
T = toas[-1] - toas[0]
df = 1.0 / (10.0 * T)
p0 = 0.033468239225/2
numf = 100000
lof = 1.0 / p0 - df * numf / 2.0
freqs = arange(numf) * df + lof
beg = clock()
mypows = spectralpower(toafft(toas, len(toas), lof, df, numf))
end = clock()
print ' TOAFFT took ', end-beg, ' sec. (%d freqs/sec)' % (numf/(end-beg))
beg = clock()
pows = periodogram(ones(len(toas), 'd'), toas, len(toas), lof, df, numf)
end = clock()
print 'periodogram took ', end-beg, ' sec. (%d freqs/sec)' % (numf/(end-beg))
def toafft(toas, freqs, days=0):
if days:
toas = (toas - toas[0]) * 86400.0
else:
toas = toas - toas[0]
twid = zeros(len(freqs), 'D')
twid.imag = -2.0 * pi * freqs
return spectralpower(add.reduce(exp(\
