def _FiveDelta2g_1(xyzs, fft='pyfftw', Ngrid=360):
''' calculate first part of
(2 ell + 1) * delta_2 (Scoccimarro 2015 Eq. 20)
More specific this function calculates
delta_2 = 15/2 (kx^2 Qxx + ky^2 Qyy + kz^2 Qzz)
'''
# Qxx, Qyy, Qzz (Scoccimarro 2015 Eq. 19)
ifft_Qii = []
for i in range(3):
_delta = np.zeros([2 * Ngrid, Ngrid, Ngrid],
dtype=np.float32,
order='F')
# order is reversed. check this carefully
fEstimate.assign_quad(xyzs, _delta, kf_ks, i + 1, i + 1, 0, 0, N,
Ngrid)
ifft_delta = _FFT(_delta, fft=fft, Ngrid=Ngrid) # run FFT
fEstimate.fcomb(ifft_delta, N, Ngrid) # combine
ifft_Qii.append(ifft_delta[:Ngrid // 2 + 1, :, :])
fEstimate.FiveDelta2g_1(ifft_Qii[0], ifft_Qii[1], ifft_Qii[2], Ngrid)
return ifft_Qii[0]
def _FiveDelta2g_2(xyzs, dcg, dcgxx, fft='pyfftw', Ngrid=360):
''' calculate second part of
(2 ell + 1) x delta_2 (Scoccimarro 2015 Eq. 20)
= 5 x delta_2
'''
# Qxx, Qyy, Qzz (Scoccimarro 2015 Eq. 19)
ifft_Qij = []
for i, j in zip([1, 2, 3], [2, 3, 1]):
_delta = np.zeros([2 * Ngrid, Ngrid, Ngrid],
dtype=np.float32,
order='F')
# order is reversed. check this carefully
fEstimate.assign_quad(xyzs, _delta, kf_ks, i, j, 0, 0, N, Ngrid)
ifft_delta = _FFT(_delta, fft=fft, Ngrid=Ngrid) # run FFT
fEstimate.fcomb(ifft_delta, N, Ngrid) # combine
ifft_Qij.append(ifft_delta[:Ngrid // 2 + 1, :, :])
fEstimate.FiveDelta2g_2(dcg, dcgxx, ifft_Qii[0], ifft_Qii[1], ifft_Qii[2],
Ngrid)
return dcgxx
def FFTperiodic(xyz, w=None, Lbox=2600., Ngrid=360, fft='pyfftw', silent=True):
''' Place galaxies/halos/particles in a periodic box onto a grid to
estimate the density field and FFT it. This function wraps some of the
functions in estimator.f and does the same thing as roman's
zmapFFTil4_aniso_gen.f
:param xyz:
3 x N dimensional array
:param Lbox: (default: 2600.)
Box size
:param Ngrid: (default: 360)
grid size
:param fft: (default: 'pyfftw')
determines which fftw version to use. Options are 'pyfftw'
and 'fortran'.
:param silent: (default: True)
if not silent then it'll output stuff
'''
kf_ks = np.float32(float(Ngrid) / Lbox)
N = np.int32(xyz.shape[1]) # number of objects
if w is None:
w = np.ones(N)
# position of galaxies (checked with fortran)
xyzs = np.zeros([3, N], dtype=np.float32, order='F')
xyzs[0, :] = np.clip(xyz[0, :], 0., Lbox * (1. - 1e-6))
xyzs[1, :] = np.clip(xyz[1, :], 0., Lbox * (1. - 1e-6))
xyzs[2, :] = np.clip(xyz[2, :], 0., Lbox * (1. - 1e-6))
if not silent: print('%i positions, Ntot=%.f' % (N, np.sum(w)))
ws = np.zeros(N, dtype=np.float32, order='F')
ws = w
# assign galaxies to grid (checked with fortran)
_delta = np.zeros([2 * Ngrid, Ngrid, Ngrid], dtype=np.float32,
order='F') # even indices (real) odd (complex)
# the order is reversed. Don't touch it!!!
fEstimate.assign_quad(xyzs, ws, _delta, kf_ks, 0, 0, 0, 0, N, Ngrid)
print(_delta[:5, :5, :5])
ifft_delta = _FFT(_delta, fft=fft, Ngrid=Ngrid, silent=silent)
if not silent: print('position grid FFTed')
# combine fields
fEstimate.fcomb_periodic(ifft_delta, np.sum(w), Ngrid)
if not silent: print('fcomb complete')
return ifft_delta[:Ngrid // 2 + 1, :, :]
def FFT_survey(radecz,
w=None,
Lbox=2600.,
Ngrid=360,
cosmo=None,
fft='pyfftw',
silent=True):
''' Put galaxies from a survey onto a grid and FFT it. This function wraps
some of the functions in estimator.f and does the same thing as roman's
zmapFFTil4_aniso_gen.f
:param radecz:
3 x N dimensional array that specify the [ra, dec, z]
:parapm w: (default: None)
N dimensional array that specifies the weight.
:param Lbox: (default: 2600.)
Box size
:param Ngrid: (default: 360)
grid size
:param cosmo: (default: None)
astropy.cosmology objec that specifies the cosmology for converting RA,
Dec, z to cartesian coordinates.
:param fft: (default: 'pyfftw')
determines which fftw version to use. Options are 'pyfftw'
and 'fortran'.
:param silent: (default: True)
if not silent then it'll output stuff
notes
-----
'''
kf_ks = np.float32(float(Ngrid) / Lbox)
N = np.int32(xyz.shape[1]) # number of objects
# default cosmology
if cosmo is None:
cosmo = FlatLambdaCDM(H0=67.6, Om0=0.31)
if w is None:
w = np.ones(N)
# convert ra, dec, z to cartesian coordinates
xyz = UT.radecz_to_cartesian(radecz, cosmo=cosmo)
if not silent:
print([
'%.1f < %s < %.1f\n' % (mi, _axis, ma)
for _axis, mi, ma in zip(['x', 'y', 'z'], np.min(xyz, axis=1),
np.max(xyz, axis=1))
])
# position of galaxies (checked with fortran)
xyzs = np.zeros([3, N], dtype=np.float32, order='F')
xyzs[0, :] = np.clip(xyz[0, :], 0., Lbox * (1. - 1e-6))
xyzs[1, :] = np.clip(xyz[1, :], 0., Lbox * (1. - 1e-6))
xyzs[2, :] = np.clip(xyz[2, :], 0., Lbox * (1. - 1e-6))
if not silent: print('%i positions' % N)
# calculate I10,I12d,I22,I13d,I23,I33
_delta = np.zeros([2 * Ngrid, Ngrid, Ngrid], dtype=np.float32, order='F')
fEstimate.assign_quad(xyzs, w, _delta, kf_ks, 0, 0, 0, 0, N,
Ngrid) # assign to grid
ifft_delta = _FFT(_delta, fft=fft, Ngrid=Ngrid, silent=silent) # run FFT
fEstimate.fcomb(ifft_delta, N, Ngrid) # combine
delta0 = ifft_delta[:Ngrid // 2 + 1, :, :]
if not silent: print('delta_0(k) complete')
# calculate delta2
five_delta2 = _FiveDelta2g_1(xyzs, fft=fft, Ngrid=Ngrid)
five_delta2 = _FiveDelta2g_1(xyzs,
delta0,
five_delta2,
fft=fft,
Ngrid=Ngrid)
# calculat reweighted fields
w = w**2
_delta = np.zeros([2 * Ngrid, Ngrid, Ngrid], dtype=np.float32, order='F')
fEstimate.assign_quad(xyzs, w, _delta, kf_ks, 0, 0, 0, 0, N,
Ngrid) # assign to grid
ifft_delta = _FFT(_delta, fft=fft, Ngrid=Ngrid, silent=silent) # run FFT
fEstimate.fcomb(ifft_delta, N, Ngrid) # combine
delta_w = ifft_delta[:Ngrid // 2 + 1, :, :]
return delta0, five_delta2, delta_w