def create_acquisition_operator_REC(pointing, parameters):
s = QubicScene(nside=parameters['nside'], kind='IQU')
## number of sub frequencies to build the TOD
Nf = int(parameters['nf_sub_build'])
band = parameters['band']
relative_bandwidth = parameters['relative_bandwidth']
Nbfreq_in, nus_edge_in, nus_in, deltas_in, Delta_in, Nbbands_in = compute_freq(
band, relative_bandwidth, Nf)
# Polychromatic instrument model
q = QubicMultibandInstrument(
filter_nus=nus_in * 1e9,
filter_relative_bandwidths=deltas_in / nus_in,
#TD = parameters['TD'],
ripples=parameters['ripples']
) # The peaks of the synthesized beam are modeled with "ripples"
### Operators for Maps Reconstruction ################################################
Nsb = parameters['nf_sub_rec']
Nbfreq, nus_edge, nus, deltas, Delta, Nbbands = compute_freq(
band, relative_bandwidth, Nsb)
arec = QubicMultibandAcquisition(
q,
pointing,
s,
nus_edge,
effective_duration=parameters['effective_duration'])
######################################################################################
return arec
def create_acquisition_operator_REC(pointing,
d,
nf_sub_rec,
verbose=False,
instrument=None):
# scene
s = qubic.QubicScene(d)
if d['nf_sub'] == 1:
if verbose:
print('Making a QubicInstrument.')
q = qubic.QubicInstrument(d)
# one subfreq for recons
_, nus_edge, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth'])
arec = qubic.QubicAcquisition(q, pointing, s, d)
return arec
else:
if instrument is None:
if verbose:
print('Making a QubicMultibandInstrument.')
q = qubic.QubicMultibandInstrument(d)
else:
q = instrument
# number of sub frequencies for reconstruction
_, nus_edge, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth'])
# Operator for Maps Reconstruction
arec = qubic.QubicMultibandAcquisition(q, pointing, s, d, nus_edge)
return arec
def foreground_signal(dictionaries, sky_configuration, sky = 'T',
seed = None, verbose = False):
"""
Averaging manually the maps into a band if nf_sub != nfrecon, otherwise, foreground are computed
in nf_recon sub-bands
Assumes . dictionaries[:]['nf_sub'] == dictionaries[:]['nf_recon']
. all regions and frequencies uses same sky configuration.
Parameters:
dictionaries:
array of dictionaries. #dicts = #regions + #bands_needed
sky_configuration:
dictionary with PySM format to build foregrounds
sky:
'T' or 'P' for temperature or polarization study
seed:
fix seed for simulations
"""
# Generate foregrounds
##### QubicSkySim instanciation
seed = seed
QubicSkyObject = []
foreground_maps = np.zeros((len(dictionaries), dictionaries[0]['nf_recon'], 12 * dictionaries[0]['nside'] ** 2, 3))
for ic, idict in enumerate(dictionaries):
QubicSkyObject.append(qss.Qubic_sky(sky_configuration, idict))
if idict['nf_sub'] != idict['nf_recon']:
_, nus_edge_in, nus_in, _, _, _ = qubic.compute_freq(idict['filter_nu'] / 1e9,
idict['nf_sub'],
idict['filter_relative_bandwidth'])
_, nus_edge_out, nus_out, _, _, _ = qubic.compute_freq(idict['filter_nu'] / 1e9,
idict['nf_recon'],
idict['filter_relative_bandwidth'])
if verbose: print('Computing maps averaging')
# Generate convolved sky of dust without noise
dust_map_in = QubicSkyObject[ic].get_fullsky_convolved_maps(FWHMdeg = None, verbose = False)
if verbose: print('=== Done {} map ===='.format(idict['filter_nu'] / 1e9, regions[ic//len(regions)][0]))
for i in range(idict['nf_recon']):
inband = (nus_in > nus_edge_out[i]) & (nus_in < nus_edge_out[i + 1])
foreground_maps[ic, ...] = np.mean(dust_map_in[inband, ...], axis=0)
elif idict['nf_sub'] == idict['nf_recon']:
# Now averaging maps into reconstruction sub-bands maps
foreground_maps[ic] = QubicSkyObject[ic].get_fullsky_convolved_maps(FWHMdeg = None, verbose = False)
return foreground_maps
def create_input_sky(d, skypars):
Nf = int(d['nf_sub'])
band = d['filter_nu'] / 1e9
filter_relative_bandwidth = d['filter_relative_bandwidth']
_, _, nus_in, _, _, Nbbands_in = qubic.compute_freq(
band, filter_relative_bandwidth, Nf)
# seed
if d['seed']:
np.random.seed(d['seed'])
# Generate the input CMB map
sp = qubic.read_spectra(skypars['r'])
cmb = np.array(
hp.synfast(sp, d['nside'], new=True, pixwin=True, verbose=False)).T
# Generate the dust map
coef = skypars['dust_coeff']
ell = np.arange(1, 3 * d['nside'])
fact = (ell * (ell + 1)) / (2 * np.pi)
spectra_dust = [
np.zeros(len(ell)), coef * (ell / 80.)**(-0.42) / (fact * 0.52),
coef * (ell / 80.)**(-0.42) / fact,
np.zeros(len(ell))
]
dust = np.array(
hp.synfast(spectra_dust,
d['nside'],
new=True,
pixwin=True,
verbose=False)).T
# Combine CMB and dust. As output we have N 3-component maps of sky.
x0 = cmb_plus_dust(cmb, dust, Nbbands_in, nus_in, d['kind'])
return x0
def __init__(self, skyconfig, d):
Nf = d['nf_sub']
band = d['filter_nu'] / 1e9
filter_relative_bandwidth = d['filter_relative_bandwidth']
_, _, central_nus, _, _, _ = qubic.compute_freq(
band, Nf, filter_relative_bandwidth)
names = [np.str(np.round(cn, 2)) for cn in central_nus]
names = [n.replace('.', 'p') for n in names]
instrument = pysm.Instrument({
'nside': d['nside'],
'frequencies': central_nus, # GHz
'use_smoothing': False,
'beams': np.ones_like(central_nus), # arcmin
'add_noise': False,
'noise_seed': 0,
'sens_I': np.ones_like(central_nus),
'sens_P': np.ones_like(central_nus),
'use_bandpass': False,
'channel_names': names,
'channels': np.ones_like(central_nus),
'output_units': 'uK_RJ',
'output_directory': "./",
'output_prefix': "qubic",
'pixel_indices': None
})
sky.__init__(self, skyconfig, d, instrument)
def __init__(self, skyconfig, d, output_directory="./", output_prefix="qubic_sky"):
self.Nfin = int(d['nf_sub'])
self.Nfout = int(d['nf_recon'])
self.filter_relative_bandwidth = d['filter_relative_bandwidth']
self.filter_nu = int(d['filter_nu'] / 1e9)
_, nus_edge_in, central_nus, deltas, _, _ = qubic.compute_freq(self.filter_nu,
self.Nfin,
self.filter_relative_bandwidth)
self.qubic_central_nus = central_nus
# THESE LINES HAVE TO BE CONFIRMED/IMPROVED in future since fwhm = lambda / (P Delta_x)
# is an approximation for the resolution
if d['config'] == 'FI':
self.fi2td = 1
elif d['config'] == 'TD':
P_FI = 22 # horns in the largest baseline in the FI
P_TD = 8 # horns in the largest baseline in the TD
self.fi2td = (P_FI - 1) / (P_TD - 1)
#
self.qubic_resolution_nus = d['synthbeam_peak150_fwhm'] * 150 / self.qubic_central_nus * self.fi2td
self.qubic_channels_names = ["{:.3s}".format(str(i)) + "_GHz" for i in self.qubic_central_nus]
instrument = {'nside': d['nside'], 'frequencies': central_nus, # GHz
'use_smoothing': False, 'beams': np.ones_like(central_nus), # arcmin
'add_noise': False, # If True `sens_I` and `sens_Q` are required
'noise_seed': 0., # Not used if `add_noise` is False
'sens_I': np.ones_like(central_nus), # Not used if `add_noise` is False
'sens_P': np.ones_like(central_nus), # Not used if `add_noise` is False
'use_bandpass': False, # If True pass banpasses with the key `channels`
'channel_names': self.qubic_channels_names, # np.ones_like(central_nus),
'channels': np.ones_like(central_nus), 'output_units': 'uK_RJ',
'output_directory': output_directory, 'output_prefix': output_prefix,
'pixel_indices': None}
sky.__init__(self, skyconfig, d, instrument, output_directory, output_prefix)
def create_acquisition_operator_REC(pointing, d, nf_sub_rec):
# Polychromatic instrument model
q = qubic.QubicMultibandInstrument(d)
# scene
s = qubic.QubicScene(d)
# number of sub frequencies for reconstruction
_, nus_edge, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth'])
# Operator for Maps Reconstruction
arec = qubic.QubicMultibandAcquisition(q, pointing, s, d, nus_edge)
return arec
def reconstruct_maps(TOD, d, pointing, nf_sub_rec, x0=None):
_, nus_edge, nus, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth'])
arec = create_acquisition_operator_REC(pointing, d, nf_sub_rec)
cov = arec.get_coverage()
maps_recon = arec.tod2map(TOD, cov=cov, tol=d['tol'], maxiter=1500)
if x0 is None:
return maps_recon, cov, nus, nus_edge
else:
_, maps_convolved = arec.get_observation(x0)
maps_convolved = np.array(maps_convolved)
return maps_recon, cov, nus, nus_edge, maps_convolved
def get_simple_sky_map(self):
"""
Create as many skies as the number of input frequencies. Instrumental
effects are not considered. For this use the `get_sky_map` method.
Return a vector of shape (number_of_input_subfrequencies, npix, 3)
"""
sky_signal = self.sky.signal()
Nf = int(self.dictionary['nf_sub'])
band = self.dictionary['filter_nu'] / 1e9
filter_relative_bandwidth = self.dictionary['filter_relative_bandwidth']
_, _, nus_in, _, _, Nbbands_in = qubic.compute_freq(band, Nf, filter_relative_bandwidth)
return np.rollaxis(sky_signal(nu=nus_in), 2, 1)
def create_acquisition_operator_TOD(pointing, d):
# Polychromatic instrument model
q = qubic.QubicMultibandInstrument(d)
# scene
s = qubic.QubicScene(d)
# number of sub frequencies to build the TOD
_, nus_edge_in, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, d['filter_relative_bandwidth'],
d['nf_sub']) # Multiband instrument model
# Multi-band acquisition model for TOD fabrication
atod = qubic.QubicMultibandAcquisition(q, pointing, s, d, nus_edge_in)
return atod
def get_simple_sky_map(self):
"""
Create as many skies as the number of input frequencies.
Instrumental effects are not considered.
Return a vector of shape (number_of_input_subfrequencies, npix, 3)
"""
_, nus_edge, nus_in, _, _, Nbbands_in = qubic.compute_freq(self.filter_nu, self.Nfin,
self.filter_relative_bandwidth)
sky = np.zeros((self.Nfin, self.npix, 3))
##### This is the old code by JCH - It has been replaced by what Edgar Jaber has proposed
##### see his presentation on Git: qubic/scripts/ComponentSeparation/InternshipJaber/teleconf_03122020.pdf
# for i in range(Nf):
# # ###################### This is puzzling part here: ############################
# # # See Issue on PySM Git: https://github.com/healpy/pysm/issues/49
# # ###############################################################################
# # # #### THIS IS WHAT WOULD MAKE SENSE BUT DOES NOT WORK ~ 5% on maps w.r.t. input
# # # nfreqinteg = 5
# # # nus = np.linspace(nus_edge[i], nus_edge[i + 1], nfreqinteg)
# # # freqs = utils.check_freq_input(nus)
# # # convert_to_uK_RJ = (np.ones(len(freqs), dtype=np.double) * u.uK_CMB).to_value(
# # # u.uK_RJ, equivalencies=u.cmb_equivalencies(freqs))
# # # #print('Convert_to_uK_RJ :',convert_to_uK_RJ)
# # # weights = np.ones(nfreqinteg) * convert_to_uK_RJ
# # ###############################################################################
# # ###### Works OK but not clear why...
# # ###############################################################################
# # nfreqinteg = 5
# # nus = np.linspace(nus_edge[i], nus_edge[i + 1], nfreqinteg)
# # filter_uK_CMB = np.ones(len(nus), dtype=np.double)
# # filter_uK_CMB_normalized = utils.normalize_weights(nus, filter_uK_CMB)
# # weights = 1. / filter_uK_CMB_normalized
# # ###############################################################################
# # ### Integrate through band using filter shape defined in weights
# # themaps_iqu = self.sky.get_emission(nus * u.GHz, weights=weights)
# # sky[i, :, :] = np.array(themaps_iqu.to(u.uK_CMB, equivalencies=u.cmb_equivalencies(nus_in[i] * u.GHz))).T
# # ratio = np.mean(self.input_cmb_maps[0,:]/sky[i,:,0])
# # print('Ratio to initial: ',ratio)
# #### Here is the new code from Edgar Jaber
for i in range(self.Nfin):
nfreqinteg = 5
freqs = np.linspace(nus_edge[i], nus_edge[i + 1], nfreqinteg)
weights = np.ones(nfreqinteg)
sky[i, :, :] = (
self.sky.get_emission(freqs * u.GHz, weights) * utils.bandpass_unit_conversion(freqs * u.GHz,
weights,
u.uK_CMB)).T
return sky
def get_corrections(nf_sub, nf_recon, band=150, relative_bandwidth=0.25):
"""
The reconstructed subbands have different widths.
Here, we compute the corrections you can applied to
the variances and covariances to take this into account.
Parameters
----------
nf_sub : int
Number of input subbands
nf_recon : int
Number of reconstructed subbands
band : int
QUBIC frequency band, in GHz. 150 by default
Typical values: 150, 220.
relative_bandwidth : float
Ratio of the difference between the edges of the
frequency band over the average frequency of the band
Typical value: 0.25
Returns
----------
corrections : list
Correction coefficients for each subband.
correction_mat : array of shape (3xnf_recon, 3xnf_recon)
Matrix containing the corrections.
It can be multiplied term by term to a covariance matrix.
"""
nb = nf_sub // nf_recon # Number of input subbands in each reconstructed subband
_, nus_edge, nus, deltas, Delta, _ = qubic.compute_freq(band, nf_sub, relative_bandwidth)
corrections = []
for isub in range(nf_recon):
# Compute wide of the sub-band
sum_delta_i = deltas[isub * nb: isub * nb + nb].sum()
corrections.append(Delta / sum_delta_i)
correction_mat = np.empty((3 * nf_recon, 3 * nf_recon))
for i in range(3 * nf_recon):
for j in range(3 * nf_recon):
freq_i = i // nf_recon
freq_j = j // nf_recon
sum_delta_i = deltas[freq_i * nb: freq_i * nb + nb].sum()
sum_delta_j = deltas[freq_j * nb: freq_j * nb + nb].sum()
correction_mat[i, j] = Delta / np.sqrt(sum_delta_i * sum_delta_j)
return corrections, correction_mat
def get_simple_sky_map(self):
"""
Create as many skies as the number of the qubic sub-frequencies.
Instrumental effects are not considered. For this purpose use the
`get_sky_map` method.
Return a vector of shape (number_of_input_subfrequencies, npix, 3)
"""
sky_signal = self.sky.signal()
Nf = self.dictionary['nf_sub']
band = self.dictionary['filter_nu'] / 1e9
filter_relative_bandwidth = self.dictionary[
'filter_relative_bandwidth']
_, _, central_nus, _, _, _ = qubic.compute_freq(
band, filter_relative_bandwidth, Nf)
return np.rollaxis(sky_signal(nu=central_nus), 2, 1)
def reconstruct_maps(TOD, parameters, pointing, x0=None):
band = parameters['band']
relative_bandwidth = parameters['relative_bandwidth']
Nsb = int(parameters['nf_sub_rec'])
Nbfreq, nus_edge, nus, deltas, Delta, Nbbands = compute_freq(
band, relative_bandwidth, Nsb)
arec = create_acquisition_operator_REC(pointing, parameters)
maps_recon = arec.tod2map(TOD, tol=parameters['tol'], maxiter=100000)
cov = arec.get_coverage()
if x0 is None:
return maps_recon, cov, nus, nus_edge
else:
TOD_useless, maps_convolved = arec.get_observation(x0)
TOD_useless = 0
maps_convolved = np.array(maps_convolved)
return maps_recon, cov, nus, nus_edge, maps_convolved
def reconstruct_maps(TOD, d, pointing, nf_sub_rec, x0=None):
_, nus_edge, nus, _, _, _ = qubic.compute_freq(d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth'])
arec = create_acquisition_operator_REC(pointing, d, nf_sub_rec)
cov = arec.get_coverage()
maps_recon, nit, error = arec.tod2map(TOD, d, cov=cov)
if not d['verbose']:
print('niterations = {}, error = {}'.format(nit, error))
if x0 is None:
return maps_recon, cov, nus, nus_edge
else:
if d['nf_sub'] == 1:
_, maps_convolved = arec.get_observation(x0[0], noiseless = d['noiseless'])
else:
_, maps_convolved = arec.get_observation(x0, noiseless = d['noiseless'])
maps_convolved = np.array(maps_convolved)
return maps_recon, cov, nus, nus_edge, maps_convolved
def get_sub_freqs_and_resolutions(dico_fast_simulator):
"""
Give the frequency sub-bands and corresponding angular resolutions around f = 150 or 220 GHz.
:param dico_fast_simulator: instrument dictionary containing frequency band and nbr of sub-bands wanted
:return: Tuple (freqs, fwhms) containing the list of the central frequencies
and the list of resolutions (in degrees).
"""
band = dico_fast_simulator['filter_nu'] / 1e9
n = int(dico_fast_simulator['nf_recon'])
filter_relative_bandwidth = dico_fast_simulator[
'filter_relative_bandwidth']
_, _, nus_in, _, _, _ = qubic.compute_freq(
band, Nfreq=n, relative_bandwidth=filter_relative_bandwidth)
# nus_in are in GHz so we use inverse scaling of resolution with frequency
# we know the fwhm at 150 GHz so the factor is 150 / (target frequency)
return nus_in, dico_fast_simulator['synthbeam_peak150_fwhm'] * 150 / nus_in
def get_tod(d, p, x0):
# Polychromatic instrument model
q = qubic.QubicMultibandInstrument(d)
# Scene
s = qubic.QubicScene(d)
# Number of sub frequencies to build the TOD
_, nus_edge_in, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, d['filter_relative_bandwidth'], d['nf_sub'])
# Multi-band acquisition operator
a = qubic.QubicMultibandAcquisition(q, p, s, d, nus_edge_in)
tod, _ = a.get_observation(x0, noiseless=True)
return q, tod
def make_covTD(d): """ Usually coverage map is provided in a separate file. But if not the case, this method can compute a coverage map Parameters: d: Qubic dictionary Return: cov: coverage map in a.QubicMultibandAcquisition shape (nfreq, npix). """ pointing = qubic.get_pointing(d) q= qubic.QubicMultibandInstrument(d) s= qubic.QubicScene(d) nf_sub_rec = d['nf_recon'] _, nus_edge, nus, _, _, _ = qubic.compute_freq(d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth']) arec = qubic.QubicMultibandAcquisition(q, pointing, s, d, nus_edge) cov = arec.get_coverage() return cov
def create_input_sky(d, skypars):
"""
Parameters
----------
d : file .dict
skypars : dictionary
Contains the dust coeff and r
Returns
-------
x0 : a sky with 3 components I, Q, U
"""
Nf = int(d['nf_sub'])
band = d['filter_nu'] / 1e9
filter_relative_bandwidth = d['filter_relative_bandwidth']
_, _, nus_in, _, _, Nbbands_in = qubic.compute_freq(
band, Nf, filter_relative_bandwidth)
# seed
if d['seed']:
np.random.seed(d['seed'])
# Generate the input CMB map
sp = qubic.read_spectra(skypars['r'])
cmb = np.array(
hp.synfast(sp, d['nside'], new=True, pixwin=True, verbose=False)).T
# Generate the dust map
ell = np.arange(1, 3 * d['nside'])
spectra_dust = dust_spectra(ell, skypars)
# coef = skypars['dust_coeff']
# fact = (ell * (ell + 1)) / (2 * np.pi)
# spectra_dust = [np.zeros(len(ell)),
# coef * (ell / 80.) ** (-0.42) / (fact * 0.52),
# coef * (ell / 80.) ** (-0.42) / fact,
# np.zeros(len(ell))]
dust = np.array(
hp.synfast(spectra_dust,
d['nside'],
new=True,
pixwin=True,
verbose=False)).T
# Combine CMB and dust. As output we have N 3-component maps of sky.
x0 = cmb_plus_dust(cmb, dust, Nbbands_in, nus_in, d['kind'])
return x0
def create_acquisition_operator_TOD(pointing, d, verbose=False):
# scene
s = qubic.QubicScene(d)
if d['nf_sub'] == 1:
if verbose:
print('Making a QubicInstrument.')
q = qubic.QubicInstrument(d)
return qubic.QubicAcquisition(q, pointing, s, d)
else:
# Polychromatic instrument model
if verbose:
print('Making a QubicMultibandInstrument.')
q = qubic.QubicMultibandInstrument(d)
# number of sub frequencies to build the TOD
_, nus_edge_in, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9,
d['nf_sub'], # Multiband instrument model
d['filter_relative_bandwidth'])
# Multi-band acquisition model for TOD fabrication
return qubic.QubicMultibandAcquisition(q, pointing, s, d, nus_edge_in)
def __init__(self, skyconfig, d, output_directory="./", output_prefix="qubic_sky"):
_, nus_edge_in, central_nus, deltas, _, _ = qubic.compute_freq(d['filter_nu'] / 1e9, d['nf_sub'],
# Multiband instrument model
d['filter_relative_bandwidth'])
self.qubic_central_nus = central_nus
self.qubic_resolution_nus = 61.347409 / self.qubic_central_nus
self.qubic_channels_names = ["{:.3s}".format(str(i)) + "_GHz" for i in self.qubic_central_nus]
instrument = pysm.Instrument({'nside': d['nside'], 'frequencies': central_nus, # GHz
'use_smoothing': False, 'beams': np.ones_like(central_nus), # arcmin
'add_noise': False, # If True `sens_I` and `sens_Q` are required
'noise_seed': 0., # Not used if `add_noise` is False
'sens_I': np.ones_like(central_nus), # Not used if `add_noise` is False
'sens_P': np.ones_like(central_nus), # Not used if `add_noise` is False
'use_bandpass': False, # If True pass banpasses with the key `channels`
'channel_names': self.qubic_channels_names, # np.ones_like(central_nus),
'channels': np.ones_like(central_nus), 'output_units': 'uK_RJ',
'output_directory': output_directory, 'output_prefix': output_prefix,
'pixel_indices': None})
sky.__init__(self, skyconfig, d, instrument, output_directory, output_prefix)
def get_tod(d, p, x0, closed_horns=None):
"""
Parameters
----------
d : dictionnary
p : pointing
x0 : sky
closed_horns : array
index of closed horns
Returns
-------
Returns an instrument with closed horns and TOD
"""
# Polychromatic instrument model
q = qubic.QubicMultibandInstrument(d)
# q = qubic.QubicInstrument(d)
if closed_horns is not None:
for i in range(d['nf_sub']):
for h in closed_horns:
q[i].horn.open[h] = False
# Scene
s = qubic.QubicScene(d)
# Number of sub frequencies to build the TOD
_, nus_edge_in, _, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, d['nf_sub'], d['filter_relative_bandwidth'])
# Multi-band acquisition operator
a = qubic.QubicMultibandAcquisition(q, p, s, d, nus_edge_in)
# a = qubic.QubicPolyAcquisition(q, p, s, d)
tod = a.get_observation(x0, convolution=False, noiseless=True)
return q, tod
def create_input_sky(parameters):
Nf = int(parameters['nf_sub_build'])
band = parameters['band']
relative_bandwidth = parameters['relative_bandwidth']
Nbfreq_in, nus_edge_in, nus_in, deltas_in, Delta_in, Nbbands_in = compute_freq(
band, relative_bandwidth, Nf)
# seed
if parameters['seed']:
np.random.seed(parameters['seed'])
# Generate the input CMB map
sp = read_spectra(0)
cmb = np.array(
hp.synfast(sp,
parameters['nside'],
new=True,
pixwin=True,
verbose=False)).T
# Generate the dust map
coef = parameters['dust_coeff']
ell = np.arange(1, 3 * parameters['nside'])
fact = (ell * (ell + 1)) / (2 * np.pi)
spectra_dust = [
np.zeros(len(ell)), coef * (ell / 80.)**(-0.42) / (fact * 0.52),
coef * (ell / 80.)**(-0.42) / fact,
np.zeros(len(ell))
]
dust = np.array(
hp.synfast(spectra_dust,
parameters['nside'],
new=True,
pixwin=True,
verbose=False)).T
# Combine CMB and dust. As output we have N 3-component maps of sky.
x0 = cmb_plus_dust(cmb, dust, Nbbands_in, nus_in)
return x0
def reconstruct_maps(TOD,
d,
pointing,
nf_sub_rec,
x0=None,
verbose=False,
instrument=None,
forced_tes_sigma=None):
_, nus_edge, nus, _, _, _ = qubic.compute_freq(
d['filter_nu'] / 1e9, nf_sub_rec, d['filter_relative_bandwidth'])
arec = create_acquisition_operator_REC(pointing,
d,
nf_sub_rec,
verbose=verbose,
instrument=instrument)
print('len(arec) = {}'.format(len(arec)))
if forced_tes_sigma is not None:
for i in range(len(arec)):
arec[i].forced_sigma = forced_tes_sigma
print('In SpectroImLib:reconstruct_maps: arec.forced_sigma{} = {}'.
format(i, arec[i].forced_sigma))
cov = arec.get_coverage()
maps_recon, nit, error = arec.tod2map(TOD, d, cov=cov)
if not d['verbose']:
print('niterations = {}, error = {}'.format(nit, error))
if x0 is None:
return maps_recon, cov, nus, nus_edge
else:
if d['nf_sub'] == 1:
_, maps_convolved = arec.get_observation(x0[0],
noiseless=d['noiseless'])
else:
_, maps_convolved = arec.get_observation(x0,
noiseless=d['noiseless'])
maps_convolved = np.array(maps_convolved)
return maps_recon, cov, nus, nus_edge, maps_convolved
nside = 256
# Observe a patch at the galactic north pole
center_gal = 0, 90
center = gal2equ(center_gal[0], center_gal[1])
band = 150
tol = 1e-4
# Compute frequencies at which we sample the TOD.
# As input we set 150 [GHz] - the central frequency of the band and
# the relative bandwidth -- 0.25.
# The bandwidth is assumed to be uniform.
# The number of frequencies is set by an optional parameter Nfreq,
# which is, by default, 15 for 150 GHz band
# and 20 for 220 GHz band.
Nbfreq, nus_edge, nus, deltas, Delta, Nbbands = compute_freq(band, 0.25)
# Use random pointings for the test
p = create_random_pointings(center, 1000, 10)
# Polychromatic instrument model
q = QubicMultibandInstrument(filter_nus=nus * 1e9,
filter_relative_bandwidths=nus / deltas,
ripples=True) # The peaks of the synthesized beam are modeled with "ripples"
s = QubicScene(nside=nside, kind='IQU')
# Polychromatic acquisition model
a = QubicPolyAcquisition(q, p, s, effective_duration=2)
sp = read_spectra(0)
hp.gnomview(maps_ud[2,-1,:,0], reso = 15,#hold = True,
notext = False, title = 'G patch ', sub = (121),
max = 0.4*np.max(maps_ud[2,-1,:,0]),
unit = r'$\mu$K',
rot = centers[2])
hp.projscatter(hp.pix2ang(nside_new, pixG_ud), marker = '*', color = 'r', s = 200)
hp.gnomview(maps_ud[1,-1,:,0], reso = 15, title = 'Q patch ',
unit = r'$\mu$K', sub = (122),
rot = centerQ)
hp.projscatter(hp.pix2ang(nside_new, pixQ_ud), marker = '*', color = 'r', s = 200)
hp.graticule(dpar = 10, dmer = 20, alpha = 0.6, verbose = False)
plt.show()
print("# Preparing for run MCMC ")
_, nus150, nus_out150, _, _, _ = qubic.compute_freq(dictionaries[0]['filter_nu'] / 1e9,
dictionaries[0]['nf_recon'],
dictionaries[0]['filter_relative_bandwidth'])
_, nus220, nus_out220, _, _, _ = qubic.compute_freq(dictionaries[1]['filter_nu'] / 1e9,
dictionaries[1]['nf_recon'],
dictionaries[1]['filter_relative_bandwidth'])
nus_out = [nus_out150, nus_out220, nus_out150, nus_out220]
pixs_ud = [pixQ_ud, pixQ_ud, pixG_ud, pixG_ud]
pixs_red = [pixQ_red, pixQ_red, pixG_red, pixG_red]
nus_edge = [nus150, nus220, nus150, nus220]
study = "dust+synch"
if study == "dust":
FuncModel = fsed.ThermDust_Planck353
p0 = np.array([1e3,3])
elif study == "synch":
FuncModel = fsed.Synchrotron_storja
nside = 256
# Observe a patch at the galactic north pole
center_gal = 0, 90
center = gal2equ(center_gal[0], center_gal[1])
band = 150
tol = 1e-4
# Compute frequencies at which we sample the TOD.
# As input we set 150 [GHz] - the central frequency of the band and
# the relative bandwidth -- 0.25.
# The bandwidth is assumed to be uniform.
# The number of frequencies is set by an optional parameter Nfreq,
# which is, by default, 15 for 150 GHz band
# and 20 for 220 GHz band.
Nbfreq, nus_edge, nus, deltas, Delta, Nbbands = compute_freq(band, 0.25)
# Use random pointings for the test
p = create_random_pointings(center, 1000, 10)
# Polychromatic instrument model
q = QubicMultibandInstrument(filter_nus=nus * 1e9,
filter_relative_bandwidths=nus / deltas,
ripples=True) # The peaks of the synthesized beam are modeled with "ripples"
s = QubicScene(nside=nside, kind='IQU')
# Polychromatic acquisition model
a = QubicPolyAcquisition(q, p, s, effective_duration=2)
sp = read_spectra(0)
subq = q.detector_subset(dets)
# Reading a sky map
m0=hp.fitsfunc.read_map('CMB_test.fits', field=(0,1,2))
x0=np.zeros((d['nf_sub'],len(m0[0]),len(m0)))
for j in range(len(m0)):
for i in range(d['nf_sub']):
x0[i,:,j]=m0[j]
# field center in galactic coordinates
center_gal = qubic.equ2gal(d['RA_center'], d['DEC_center'])
# Choosing the subfrequencies for map acquisition
Nbfreq_in, nus_edge_in, nus_in, deltas_in, Delta_in, Nbbands_in =\
qubic.compute_freq(d['filter_nu']/1e9, d['filter_relative_bandwidth'],
d['nf_sub']) # Multiband instrument model
# Map acquisition for the full and reduced instruments
a = qubic.QubicMultibandAcquisition(q, p, s, d, nus_edge_in)
suba = qubic.QubicMultibandAcquisition(subq, p, s, d, nus_edge_in)
t = time()
# Time lines construction
TOD, maps_convolved= a.get_observation(x0, noiseless=True)
subTOD= suba.get_observation(np.array(maps_convolved), convolution=False,
noiseless=True)
print 'TOD time =', time()-t
# Choosing the subfrequencies for map reconstruction
nf_sub_rec = 2
center = gal2equ(center_gal[0], center_gal[1])
band = 150
tol = 1e-4
# Compute frequencies at which we sample the TOD.
# As input we set 150 [GHz] - the central frequency of the band and
# the relative bandwidth -- 0.25.
# The bandwidth is assumed to be uniform.
# The number of frequencies is set by an optional parameter Nfreq,
# which is, by default, 15 for 150 GHz band
# and 20 for 220 GHz band.
# Here we use only Nf=5 frequencies
Nf = 5
relative_bandwidth = 0.25
Nbfreq, nus_edge, nus, deltas, Delta, Nbbands = compute_freq(band, relative_bandwidth, 5)
# Use random pointings
p = create_random_pointings(center, 1000, 10)
# Polychromatic instrument model
q = QubicMultibandInstrument(filter_nus=nus * 1e9,
filter_relative_bandwidths=nus / deltas,
ripples=True) # The peaks of the synthesized beam are modeled with "ripples"
s = QubicScene(nside=nside, kind='IQU')
# Multi-band acquisition model
# Nsb=2 sub-bands to reconstruct the CMB
Nsb = 2
Nbfreq, nus_edge, nus_, deltas_, Delta_, Nbbands_ = compute_freq(band, relative_bandwidth, Nsb)
for freq in xrange(nbands):
for i in xrange(2):
for pitch in xrange(7):
std[pitch, freq, i] = np.std(residus[pitch][:,freq,:,i+1])
std_meanQU = np.mean(std, axis=2) / np.sqrt(nbands)
plt.plot(pitch_std, std_meanQU[:,freq], 'o', label='subband ' + str(freq+1) + '/' + str(nbands))
# plt.plot(pitch_mean, std[:,i], '.', label=stokes[i+1])
plt.xlim(-0.5, 31)
plt.xlabel('pitch std')
plt.ylabel('std_Residus / sqrt(nbands)')
plt.legend(numpoints=1, loc=4)
plt.title('Q an U std residus averaged and corrected by sqrt(nbands)')
#Calcul de la correction
Nfreq = 12
_, nus_edge, nus, deltas, Delta, _ = qubic.compute_freq(band=150, relative_bandwidth=0.25, Nfreq=Nfreq)
print(Delta)
print(deltas)
plot(nus, deltas, 'o')
#si on les import tous
plt.figure('pitch_test_I=0_std_residus_corrected2')
for nbands in [1,2,3,4]:
plt.subplot(2,2,nbands)
std = np.empty((7, nbands, 2))
for freq in xrange(nbands):
for i in xrange(2):
for pitch in xrange(7):
res = pitch*4+nbands-1
#print(res)
std[pitch, freq, i] = np.std(residus[res][:,freq,:,i+1])
source = m0 * 0
source[id] = 1
arcToRad = np.pi / (180 * 60.)
source = hp.sphtfunc.smoothing(source, fwhm=30 * arcToRad)
x0[:, :, component] = source
hp.mollview(x0[0, :, component])
plt.show()
if p.fix_az:
center = (fix_azimuth['az'], fix_azimuth['el'])
else:
center = qubic.equ2gal(d['RA_center'], d['DEC_center'])
# Make TOD
Nbfreq_in, nus_edge_in, nus_in, deltas_in, Delta_in, Nbbands_in = qubic.compute_freq(d['filter_nu'] / 1e9,
d['nf_sub'],
d['filter_relative_bandwidth'])
a = qubic.QubicMultibandAcquisition(q, p, s, d, nus_edge_in)
TOD = a.get_observation(x0, noiseless=True, convolution=False)
plt.plot(TOD[0, :])
plt.xlabel('pointing index')
plt.ylabel('TOD')
plt.show()
# Map making
if alaImager:
nf_sub_rec = 1
d['synthbeam_kmax'] = 0
if oneComponent: