def qe_shear(px,mlmax,Talm=None,fTalm=None):
"""
px is a pixelization object, initialized like this:
px = pixelization(shape=shape,wcs=wcs) # for CAR
px = pixelization(nside=nside) # for healpix
output: curved sky shear estimator
"""
ells = np.arange(mlmax)
#prepare temperature map
rmapT=px.alm2map(np.stack((Talm,Talm)),spin=0,ncomp=1,mlmax=mlmax)[0]
#find tbarf
t_alm=cs.almxfl(fTalm,np.sqrt((ells-1.)*ells*(ells+1.)*(ells+2.)))
alms=np.stack((t_alm,t_alm))
rmap=px.alm2map_spin(alms,0,2,ncomp=2,mlmax=mlmax) #same as 2 2
#multiply the two fields together
prodmap=rmap*rmapT
if not(px.hpix): prodmap=enmap.enmap(prodmap,px.wcs)
realsp2=prodmap[0] #spin +2 real space real space field
realsm2=prodmap[1] #spin -2 real space real space field
if not(px.hpix):
realsp2 = enmap.enmap(realsp2,px.wcs)
realsm2=enmap.enmap(realsm2,px.wcs)
#convert the above spin2 fields to spin pm 2 alms
res1 = px.map2alm_spin(realsp2,mlmax,2,2) #will return pm2
res2= px.map2alm_spin(realsm2,mlmax,-2,2) #will return pm2
#spin 2 ylm
ttalmsp2=rot2dalm(res1,2)[0] #pick up the spin 2 alm of the first one
ttalmsm2=rot2dalm(res1,2)[1] #pick up the spin -2 alm of the second one
shear_alm=ttalmsp2+ttalmsm2
return shear_alm
def high_res_plot_img(array,
filename=None,
down=None,
verbose=True,
overwrite=True,
crange=None,
cmap="planck"):
if not (overwrite):
if os.path.isfile(filename): return
try:
from pixell import enmap, enplot
except:
traceback.print_exc()
cprint(
"Could not produce plot " + filename +
". High resolution plotting requires enlib, which couldn't be imported. Continuing without plotting.",
color='fail')
return
if (down is not None) and (down != 1):
downmap = enmap.downgrade(enmap.enmap(array)[None], down)
else:
downmap = enmap.enmap(array)[None]
img = enplot.draw_map_field(downmap,
enplot.parse_args("-c " + cmap + " -vvvg moo"),
crange=crange)
#img = enplot.draw_map_field(downmap,enplot.parse_args("--grid 1"),crange=crange)
if filename is None:
img.show()
else:
img.save(filename)
if verbose:
print(bcolors.OKGREEN + "Saved high-res plot to",
filename + bcolors.ENDC)
def sim_build(region, version, overwrite):
save_scratch = True
savedir = tutils.get_save_path(version, region)
if save_scratch:
scratch = tutils.get_scratch_path(version, region)
covscratch = scratch
else:
covscratch = None
if not (overwrite):
assert not(os.path.exists(savedir)), \
"This version already exists on disk. Please use a different version identifier."
try:
os.makedirs(savedir)
except:
if overwrite: pass
else: raise
if save_scratch:
try:
os.makedirs(scratch)
except:
pass
#enmap.write_map(scratch+"/temp1.hdf",enmap.enmap(np.zeros((100,100))))
#enmap.write_map(savedir+"/temp2.hdf",enmap.enmap(np.zeros((100,100))))
np.save(scratch + "/temp1.npy", enmap.enmap(np.zeros((100, 100))))
np.save(savedir + "/temp2.npy", enmap.enmap(np.zeros((100, 100))))
shutil.rmtree(scratch)
def process(kouts, name="default", ellmax=None, y=False, y_ellmin=400):
ellmax = lmax if ellmax is None else ellmax
ksilc = enmap.zeros((Ny, Nx), wcs, dtype=np.complex128).reshape(-1)
ksilc[modlmap.reshape(-1) < lmax] = np.nan_to_num(kouts.copy())
ksilc = enmap.enmap(ksilc.reshape((Ny, Nx)), wcs)
ksilc[modlmap > ellmax] = 0
if y: ksilc[modlmap < y_ellmin] = 0
msilc = np.nan_to_num(
fft.ifft(ksilc, axes=[-2, -1], normalize=True).real * bmask)
enmap.write_map(proot + "outmap_%s.fits" % name, enmap.enmap(msilc, wcs))
p2d = fc.f2power(ksilc, ksilc)
bin_edges = np.arange(100, 3000, 40)
binner = stats.bin2D(modlmap, bin_edges)
cents, p1d = binner.bin(p2d)
try:
# io.plot_img(np.log10(np.fft.fftshift(p2d)),proot+"ksilc_%s.png" % name,aspect='auto')
# io.plot_img(msilc,proot+"msilc_%s.png" % name)
# io.plot_img(msilc,proot+"lmsilc_%s.png" % name,lim=300)
tmask = maps.mask_kspace(shape,
wcs,
lmin=300,
lmax=5000 if not (y) else 1500)
fmap = maps.filter_map(msilc, tmask) * bmask
io.plot_img(fmap, proot + "hmsilc_%s.png" % name, high_res=True)
except:
pass
return cents, p1d
def get_shear(self, do_m=True, do_c=True):
rms = self.cat.data['ishape_hsm_regauss_derived_rms_e']
m = self.cat.data['ishape_hsm_regauss_derived_bias_m']
e1 = self.cat.data['ishape_hsm_regauss_e1']
e2 = self.cat.data['ishape_hsm_regauss_e2']
c1 = self.cat.data['ishape_hsm_regauss_derived_bias_c1']
c2 = self.cat.data['ishape_hsm_regauss_derived_bias_c2']
hsc_wts = self.hsc_wts
wts = self.wts
hsc_resp = 1. - np.nan_to_num(
self.get_map(weights=(wts * (rms**2.))) / hsc_wts)
hsc_m = np.nan_to_num(self.get_map(weights=(wts * (m))) /
hsc_wts) if do_m else hsc_wts * 0.
hsc_e1 = self.get_map(weights=e1 * wts)
hsc_e2 = self.get_map(weights=e2 * wts)
hsc_c1 = np.nan_to_num(self.get_map(weights=c1 * wts) /
hsc_wts) if do_c else hsc_wts * 0.
hsc_c2 = np.nan_to_num(self.get_map(weights=c2 * wts) /
hsc_wts) if do_c else hsc_wts * 0.
g1map = np.nan_to_num(hsc_e1 / 2. / hsc_resp / (1. + hsc_m) /
hsc_wts) - np.nan_to_num(hsc_c1 / (1. + hsc_m))
g2map = np.nan_to_num(hsc_e2 / 2. / hsc_resp / (1. + hsc_m) /
hsc_wts) - np.nan_to_num(hsc_c2 / (1. + hsc_m))
if not self.curved:
g1map = enmap.enmap(g1map, self.wcs)
g2map = enmap.enmap(g2map, self.wcs)
return g1map, g2map
def qe_m4(px,mlmax,Talm=None,fTalm=None):
"""
px is a pixelization object, initialized like this:
px = pixelization(shape=shape,wcs=wcs) # for CAR
px = pixelization(nside=nside) # for healpix
output: curved sky multipole=4 estimator
"""
ells = np.arange(mlmax)
#prepare temperature map
rmapT=px.alm2map(np.stack((Talm,Talm)),spin=0,ncomp=1,mlmax=mlmax)[0]
#find tbarf
t_alm=cs.almxfl(fTalm,np.sqrt((ells-3.)*(ells-2.)*(ells-1.)*ells*(ells+1.)*(ells+2.)*(ells+3.)*(ells+4.)))
alms=np.stack((t_alm,t_alm))
rmap=px.alm2map_spin(alms,0,4,ncomp=2,mlmax=mlmax)
#multiply the two fields together
rmap=np.nan_to_num(rmap)
prodmap=rmap*rmapT
prodmap=np.nan_to_num(prodmap)
if not(px.hpix): prodmap=enmap.enmap(prodmap,px.wcs)
realsp2=prodmap[0] #spin +4 real space real space field
if not(px.hpix): realsp2 = enmap.enmap(realsp2,px.wcs)
#convert the above spin4 fields to spin pm 4 alms
res1 = px.map2alm_spin(realsp2,mlmax,4,4) #will return pm4
#spin 4 ylm
ttalmsp2=rot2dalm(res1,4)[0] #pick up the spin 4 alm of the first one
ttalmsm2=rot2dalm(res1,4)[1] #pick up the spin -4 alm of the second one
m4_alm=ttalmsp2+ttalmsm2
return m4_alm
def get_delta(self):
delta = (self.counts/self.nmean-1.)
if not self.curved:
parea = maps.psizemap(delta.shape, self.wcs)*((180.*60./np.pi)**2.)
delta = ((delta+1.)*self.nmean/self.ngal_per_arcminsq/parea)-1.
delta = enmap.enmap(delta,self.wcs)
return delta
def get_maps(self, seed=None):
# SKY
fgs = []
for i, comp in enumerate(self.components):
fgs.append(self.fgens[comp].get_map(seed=(1, i, seed)))
arrays = []
for k, (beam, inhom,
nsplit) in enumerate(zip(self.beams, self.inhoms,
self.nsplits)):
# SKY
sky = 0.
for i, comp in enumerate(self.components):
sky += (fgs[i] * self.rdict[comp][i])
kbeam = maps.gauss_beam(self.modlmap, beam)
kbeam[self.modlmap < self.ellmin] = 0
sky_convolved = maps.filter_map(sky, kbeam)
# NOISE
nmaps = []
for j in range(nsplit):
nmap = self.ngens[k].get_map(seed=(2, j, seed)) * nsplit
nmaps.append(nmap.copy())
nmaps = np.stack(nmaps)
observed = enmap.enmap(sky_convolved + nmaps, self.wcs)
arrays.append(observed.copy())
return arrays
def process_splits(splits,
wins,
mask,
skip_splits=False,
do_fft_splits=False,
pixwin=False):
assert wins.ndim > 2
with np.errstate(divide='ignore', invalid='ignore'):
coadd = (splits * wins).sum(axis=0) / wins.sum(axis=0)
coadd[~np.isfinite(coadd)] = 0
Ny, Nx = splits.shape[-2:]
assert coadd.shape == (Ny, Nx)
kcoadd = enmap.enmap(enmap.fft(coadd * mask, normalize='phys'), wins.wcs)
if pixwin: pwin = tutils.get_pixwin(coadd.shape[-2:])
else: pwin = 1
kcoadd = kcoadd / pwin
if not (skip_splits):
#data = (splits-coadd)*mask # !!!! wins removed, was (splits-coadd)*wins*mask earlier
data = (splits - coadd) * mask * wins / wins.sum(
axis=0) # !!!! wins removed, was (splits-coadd)*wins*mask earlier
data[~np.isfinite(data)] = 0
kdiffs = enmap.fft(data, normalize='phys')
kdiffs = kdiffs / pwin
else:
kdiffs = None
if do_fft_splits:
ksplits = enmap.fft(splits * wins * mask, normalize='phys')
ksplits = ksplits / pwin
return kdiffs, kcoadd, ksplits
else:
return kdiffs, kcoadd
def map2alm_spin(self,imap,lmax,spin_alm,spin_transform):
dmap = -irot2d(np.stack((imap,imap.conj())),spin=spin_alm).real
if self.hpix:
res = hp.map2alm_spin(dmap,lmax=lmax,spin=spin_transform)
return res
else:
return cs.map2alm(enmap.enmap(dmap,imap.wcs),spin=spin_transform,lmax=lmax)
def get_sim(self,season,patch,array,sim_num, save_alm=True, save_map=False, set_idx=0,mask_patch=None,fgflux="15mjy"):
shape,wcs = self.noise_gen.load_covsqrt(season,patch,array,coadd=True,mask_patch=mask_patch,get_geometry=True)
# (nfreqs,nsplits,npol,Ny,Nx)
noises,ivars = self.get_noise(season=season,patch=patch,array=array, sim_num=sim_num,mask_patch=mask_patch,set_idx=set_idx,apply_ivar=False)
#noises,ivars = self.get_noise(season=season,patch=patch,array=array, sim_num=0,mask_patch=mask_patch,set_idx=set_idx,apply_ivar=False)
afreqs = self.noise_gen.dm.array_freqs[array]
#afreqs = ['pa1_f090', 'pa1_f150']
signals = []
for afreq in afreqs:
# This could be improved
if self.model=='act_mr3': pfreq = afreq.split('_')[1]
elif self.model=='planck_hybrid':
pfreq = afreq
assert season is None
season = "planck"
patch = "planck"
array = "planck"
imap = self.get_signal(season, patch, array, pfreq, sim_num, save_alm=save_alm, save_map=save_map, set_idx=set_idx,oshape=shape,owcs=wcs,fgflux=fgflux)
signals.append(imap)
owcs = imap.wcs
# (nfreqs,npol,Ny,Nx)
signals = enmap.enmap(np.stack(signals),owcs)[:,None,...]
del imap
assert wcsutils.equal(wcs,noises.wcs)
assert wcsutils.equal(owcs,noises.wcs)
return self._footprint(noise.apply_ivar_window(signals + noises,ivars))
def pcov_from_ivar(n,dec,ra,ivar,cmb_theory_fn,beam_fn,iau=False):
"""
Get a pixel covariance matrix for a stamp around a given location
from the white noise inverse variance map and theory and beam
functions.
"""
assert ivar.ndim==2
py,px = ivar.sky2pix((dec,ra))
py = int(py)
px = int(px)
sy = py - n//2
sx = px - n//2
ey = sy + n
ex = sx + n
sliced = 1./ivar[sy:ey,sx:ex]
sliced[~np.isfinite(sliced)] = 1./ivar[ivar>0].max() # this is wrong! but needed to prevent singular matrices?!
ncov = np.diag(sliced.reshape(-1))
ncov_IQU = np.zeros((3,3,n*n,n*n))
ncov_IQU[0,0] = ncov.copy()
ncov_IQU[1,1] = ncov.copy() * 2.
ncov_IQU[2,2] = ncov.copy() * 2.
modlmap = sliced.modlmap()
cmb2d_TEB = np.zeros((3,3,n,n))
theory = cmb_theory_fn
cmb2d_TEB[0,0] = theory('TT',modlmap)
cmb2d_TEB[1,1] = theory('EE',modlmap)
cmb2d_TEB[2,2] = theory('BB',modlmap)
cmb2d_TEB[0,1] = theory('TE',modlmap)
cmb2d_TEB[1,0] = theory('TE',modlmap)
beam2d = beam_fn(modlmap)
tcov = stamp_pixcov_from_theory(n,enmap.enmap(cmb2d_TEB,sliced.wcs),n2d_IQU=0.,beam2d=beam2d,iau=iau,return_pow=False)
return tcov + ncov_IQU
def update_mask(self, mask_threshold):
mask = np.zeros(self.shape)
mask[self.mean_wt > mask_threshold] = 1
self.mask = mask
if not self.curved:
self.mask = enmap.enmap(self.mask, self.wcs)
self._counts()
def signal_average(cov,bin_edges=None,bin_width=40,kind=3,lmin=None,dlspace=True,return_bins=False,**kwargs):
"""
dcov = cov * ellfact
bin dcov in annuli
interpolate back on to ell
cov = dcov / ellfact
where ellfact = ell**2 if dlspace else 1
"""
modlmap = cov.modlmap()
assert np.all(np.isfinite(cov))
dcov = cov*modlmap**2. if dlspace else cov.copy()
if lmin is None:
minell = maps.minimum_ell(dcov.shape,dcov.wcs)
else:
minell = modlmap[modlmap<=lmin].max()
if bin_edges is None: bin_edges = np.append([2],np.arange(minell,modlmap.max(),bin_width))
binner = stats.bin2D(modlmap,bin_edges)
cents,c1d = binner.bin(dcov)
outcov = enmap.enmap(maps.interp(cents,c1d,kind=kind,fill_value=c1d[-1],**kwargs)(modlmap),dcov.wcs)
with np.errstate(invalid='ignore'): outcov = outcov / modlmap**2. if dlspace else outcov
outcov[modlmap<2] = 0
assert np.all(np.isfinite(outcov))
if return_bins: return cents,c1d,outcov
else: return outcov
def load_covsqrt(self,
season=None,
patch=None,
array=None,
coadd=True,
mask_patch=None,
get_geometry=False):
pout, cout, sout = get_save_paths(self._model,
self._version,
coadd=coadd,
season=season,
patch=patch,
array=array,
overwrite=False,
mask_patch=mask_patch)
fpath = "%s_covsqrt.fits" % (cout)
if get_geometry: return enmap.read_map_geometry(fpath)
ikey = '_'.join([str(x) for x in [season, patch]])
try:
covsqrt = self._ccache[fpath]
ivars = self._icache[ikey]
if self.verbose: print("Loaded cached covsqrt and ivars.")
except:
if self.verbose:
print(
"Couldn't find covsqrt and ivars in cache. Reading from disk..."
)
ivars = enmap.enmap([self.dm.get_ivars(q) for q in self._qid])
covsqrt = enmap.read_map(fpath)
print(fpath, covsqrt.shape)
if len(self._ccache.keys()) < self.ncache:
self._ccache[fpath] = covsqrt
self._icache[ikey] = ivars
return covsqrt, ivars
def get_splits_ivar(qid, extracter, ivar_unhit=1e-7, ivar_tol=20):
dmodel = sints.arrays(qid, 'data_model')
season = sints.arrays(qid, 'season')
region = sints.arrays(qid, 'region')
array = sints.arrays(qid, 'array')
freq = sints.arrays(qid, 'freq')
dm = sints.models[dmodel]()
ivars = []
for i in range(dm.get_nsplits(season=season, patch=region, array=array)):
omap = extracter(
dm.get_split_ivar_fname(season=season,
patch=region,
array=array + "_" +
freq if not (is_planck(qid)) else freq,
splitnum=i))
if omap.ndim > 2: omap = omap[0]
if not (np.any(omap > 0)):
print(
"Skipping %s as it seems to have an all zero ivar in this tile"
% qid)
return None
omap[~np.isfinite(omap)] = 0
omap[omap < ivar_unhit] = 0
ref_div = robust_ref(omap)
omap = np.minimum(omap, ref_div * ivar_tol)
omap = filter_div(omap)
eshape, ewcs = omap.shape, omap.wcs
ivars.append(omap.copy())
return enmap.enmap(np.stack(ivars), ewcs)
def generate_noise_sim(covsqrt, ivars, seed=None, dtype=None):
"""
Supports only two cases
1) nfreqs>=1,npol=3
2) nfreqs=1,npol=1
"""
if isinstance(seed, int): seed = (seed, )
assert np.all(np.isfinite(covsqrt))
shape, wcs = covsqrt.shape, covsqrt.wcs
Ny, Nx = shape[-2:]
ncomps = covsqrt.shape[0]
assert ncomps == covsqrt.shape[1]
assert ((ncomps % 3) == 0) or (ncomps == 1)
nfreqs = 1 if ncomps == 1 else ncomps // 3
if ncomps == 1: npol = 1
else: npol = 3
wmaps = enmap.extract(ivars, shape[-2:], wcs)
nsplits = wmaps.shape[1]
if dtype is np.float32: ctype = np.complex64
elif dtype is np.float64: ctype = np.complex128
# Old way with loop
kmap = []
for i in range(nsplits):
if seed is None:
np.random.seed(None)
else:
np.random.seed(seed + (i, ))
rmap = enmap.rand_gauss_harm((ncomps, Ny, Nx),
covsqrt.wcs).astype(ctype)
kmap.append(enmap.map_mul(covsqrt, rmap))
del covsqrt, rmap
kmap = enmap.enmap(np.stack(kmap), wcs)
outmaps = enmap.ifft(kmap, normalize="phys").real
del kmap
# Need to test this more ; it's only marginally faster and has different seed behaviour
# covsqrt = icovsqrt
# np.random.seed(seed)
# rmap = enmap.rand_gauss_harm((nsplits,ncomps,Ny, Nx),covsqrt.wcs)
# kmap = enmap.samewcs(np.einsum("abyx,cbyx->cayx", covsqrt, rmap),rmap)
# outmaps = enmap.ifft(kmap, normalize="phys").real
# isivars = 1/np.sqrt(wmaps)
with np.errstate(divide='ignore', invalid='ignore'):
isivars = ((1. / wmaps) - (1. / wmaps.sum(axis=1)[:, None, ...]))**0.5
isivars[~np.isfinite(isivars)] = 0
assert np.all(np.isfinite(outmaps))
# Divide by hits
for ifreq in range(nfreqs):
outmaps[:, ifreq * npol:(ifreq + 1) * npol,
...] = outmaps[:, ifreq * npol:(ifreq + 1) * npol,
...] * isivars[ifreq, ...] * np.sqrt(nsplits)
retmaps = outmaps.reshape((nsplits, nfreqs, npol, Ny, Nx)).swapaxes(0, 1)
assert np.all(np.isfinite(retmaps))
return retmaps, wmaps
def get_offset_result(res=1.,dtype=np.float64,seed=1):
shape,wcs = enmap.fullsky_geometry(res=np.deg2rad(res))
shape = (3,) + shape
obs_pos = enmap.posmap(shape, wcs)
np.random.seed(seed)
grad = enmap.enmap(np.random.random(shape),wcs)*1e-3
raw_pos = enmap.samewcs(lensing.offset_by_grad(obs_pos, grad, pol=shape[-3]>1, geodesic=True), obs_pos)
return obs_pos,grad,raw_pos
def get_covsqrt(ps, method="arrayops"):
if method == "multipow":
covsq = enmap.multi_pow(ps.copy(), 0.5)
elif method == "arrayops":
from enlib import array_ops
covsq = array_ops.eigpow(ps.copy(), 0.5, axes=[0, 1])
covsq[:, :, ps.modlmap() < 2] = 0
assert np.all(np.isfinite(covsq))
return enmap.enmap(covsq, ps.wcs)
def mask_smoothing(inmap, N, f=0.5):
import scipy
smoothed = scipy.ndimage.filters.gaussian_filter(inmap, N)
new = np.zeros(smoothed.shape)
new[smoothed > f] = 1.
smoothedagain = scipy.ndimage.filters.gaussian_filter(new, N)
new = enmap.enmap(smoothedagain, inmap.wcs)
assert np.all((inmap - new) >= 0)
return new
def __init__(self,
ras_deg,
decs_deg,
shape=None,
wcs=None,
nside=None,
verbose=True,
hp_coords="equatorial",
mask=None):
self.verbose = verbose
if nside is not None:
eq_coords = ['fk5', 'j2000', 'equatorial']
gal_coords = ['galactic']
if verbose: print("Calculating pixels...")
if hp_coords in gal_coords:
if verbose: print("Transforming coords...")
from astropy.coordinates import SkyCoord
import astropy.units as u
gc = SkyCoord(ra=ras_deg * u.degree,
dec=decs_deg * u.degree,
frame='fk5')
gc = gc.transform_to('galactic')
phOut = gc.l.deg * np.pi / 180.
thOut = gc.b.deg * np.pi / 180.
thOut = np.pi / 2. - thOut #polar angle is 0 at north pole
self.pixs = hp.ang2pix(nside, thOut, phOut)
elif hp_coords in eq_coords:
ras_out = ras_deg
decs_out = decs_deg
self.pixs = hp.ang2pix(nside, ras_out, decs_out, lonlat=True)
else:
raise ValueError
if verbose: print("Done with pixels...")
self.nside = nside
self.shape = hp.nside2npix(nside)
self.curved = True
else:
coords = np.vstack((decs_deg, ras_deg)) * np.pi / 180.
self.shape = shape
self.wcs = wcs
if verbose: print("Calculating pixels...")
self.pixs = enmap.sky2pix(shape, wcs, coords,
corner=True) # should corner=True?!
if verbose: print("Done with pixels...")
self.curved = False
self.counts = self.get_map()
if not self.curved:
self.counts = enmap.enmap(self.counts, self.wcs)
self.mask = np.ones(shape) if mask is None else mask
self._counts()
def get_splits(qid, extracter):
nsplits = 2
splits = []
for i in range(nsplits):
fname = os.environ['WORK'] + '/sim_tiling/%s_split_%d.fits' % (qid, i)
omap = extracter(fname)
assert np.all(np.isfinite(omap))
eshape, ewcs = omap.shape, omap.wcs
splits.append(omap.copy())
return enmap.enmap(np.stack(splits), ewcs)
def test_fft(self):
# Tests that ifft(ifft(imap))==imap, i.e. default normalizations are consistent
shape, wcs = enmap.geometry(pos=(0, 0), shape=(3, 100, 100), res=0.01)
imap = enmap.enmap(np.random.random(shape), wcs)
assert np.all(
np.isclose(
imap,
enmap.ifft(enmap.fft(imap, normalize='phy'),
normalize='phy').real))
assert np.all(np.isclose(imap, enmap.ifft(enmap.fft(imap)).real))
def tqu2teb(tmap, qmap, umap, lmax):
atol = np.min(np.array(tmap.pixshape() / eutils.arcmin))
tqu = np.zeros((3, ) + tmap.shape)
tqu[0], tqu[1], tqu[2] = (tmap, qmap, umap)
tqu = enmap.enmap(tqu, tmap.wcs)
alm = curvedsky.map2alm(tqu, lmax=lmax, atol=atol)
teb = curvedsky.alm2map(alm[:, None], tqu.copy()[:, None], spin=0)[:, 0]
del tqu
return (teb[0], teb[1], teb[2]) # tmap, emap, bmap
def get_anisotropic_noise_template(shape,wcs,template_file=None,tmin=0,tmax=100):
"""
This function reads in a 2D PS unredenned template and returns a full 2D noise PS.
It doesn't use the template in the most sensible way though.
"""
if template_file is None: template_file = "data/anisotropy_template.fits"
template = np.nan_to_num(enmap.read_map(template_file))
template[template<tmin] = tmin
template[template>tmax] = tmax
ops = enmap.enmap(enmap.resample(template,shape),wcs) # interpolate to new geometry
return ops
def coadd_real_data(qid, mask, dg=2):
# Compute coadded map by simply summing up each split with the inverse variance weight
assert mask.ndim == 2
# First, read survey parameters from qid
model, season, array, patch, freq = local.qid_info(qid[0])
# Day time data
if model == 'dr5':
dm = interfaces.models['dr5'](region=mask)
datas = enmap.enmap([dm.get_splits(q, calibrated=True) for q in qid])
ivars = enmap.enmap([dm.get_ivars(q, calibrated=True) for q in qid])
# Night time data
if model == 'act_mr3':
dm = interfaces.models['act_mr3'](region=mask, calibrated=True)
datas = dm.get_splits(season=season,
patch=patch,
arrays=dm.array_freqs[array],
srcfree=True)
ivars = dm.get_splits_ivar(season=season,
patch=patch,
arrays=dm.array_freqs[array])
# coadded map
civars = np.average(ivars, axis=1)
civars[civars == 0] = np.inf
map_c = mask[None, None, :, :] * np.average(datas * ivars,
axis=1) / civars / local.Tcmb
# downgrade
map_c = enmap.downgrade(map_c, dg)
# check
assert map_c.ndim == 4
return map_c
def interp_enmap(emap, nshape, nwcs, method='cubic', fill_value=np.nan):
# interpolate enmap to the new shape, and override wcs
oshape, owcs = emap.shape, emap.wcs
if nshape == oshape: return emap
oxm, oym = enmap.posmap(oshape, owcs)
nxm, nym = enmap.posmap(nshape, nwcs)
oxm, oym = oxm[:, 0], oym[0, :]
nxm, nym = nxm[:, 0], nym[0, :]
f2 = RectBivariateSpline(oxm, oym, emap)
ndata = f2(nxm, nym)
return enmap.enmap(ndata, nwcs)
def update_mask(self,rand_sigma_arcmin=2.,rand_threshold=1e-3):
if rand_sigma_arcmin>1.e-3:
if self.verbose: print( "Smoothing...")
if self.curved:
smap = hp.smoothing(self.rand_map,sigma=rand_sigma_arcmin*np.pi/180./60.)
else:
smap = enmap.smooth_gauss(self.rand_map,rand_sigma_arcmin*np.pi/180./60.)
if self.verbose: print( "Done smoothing...")
else:
if self.verbose: smap = self.rand_map
self.mask = np.zeros(self.shape)
self.mask[smap>rand_threshold] = 1
if not self.curved:
self.mask = enmap.enmap(self.mask,self.wcs)
self._counts()
def test_extract(self):
# Tests that extraction is sensible
shape, wcs = enmap.geometry(pos=(0, 0), shape=(500, 500), res=0.01)
imap = enmap.enmap(np.random.random(shape), wcs)
smap = imap[200:300, 200:300]
sshape, swcs = smap.shape, smap.wcs
smap2 = enmap.extract(imap, sshape, swcs)
pixbox = enmap.pixbox_of(imap.wcs, sshape, swcs)
# Do write and read test
filename = "temporary_extract_map.fits" # NOT THREAD SAFE
enmap.write_map(filename, imap)
smap3 = enmap.read_map(filename, pixbox=pixbox)
os.remove(filename)
assert np.all(np.isclose(smap, smap2))
assert np.all(np.isclose(smap, smap3))
assert wcsutils.equal(smap.wcs, smap2.wcs)
assert wcsutils.equal(smap.wcs, smap3.wcs)
def get_n2d(ffts, wmaps, plot_fname=None, coadd_estimator=False, dtype=None):
assert np.all(np.isfinite(ffts))
assert np.all(np.isfinite(wmaps))
shape, wcs = ffts.shape[-2:], ffts.wcs
modlmap = enmap.modlmap(shape, wcs)
Ny, Nx = shape[-2:]
nfreqs = ffts.shape[0]
npol = ffts.shape[2]
ncomps = nfreqs * npol
def ncomp_to_freq_pol(index):
ifreq = index // 3
ipol = index % 3
return ifreq, ipol
n2d = enmap.zeros((ncomps, ncomps, Ny, Nx), wcs,
dtype=dtype) # WARNING: type)
pols = ['I', 'Q', 'U']
for i in range(ncomps):
for j in range(i, ncomps):
ifreq, ipol = ncomp_to_freq_pol(i)
jfreq, jpol = ncomp_to_freq_pol(j)
isplits = ffts[ifreq, :, ipol]
iwts = wmaps[ifreq, :, 0]
if i != j:
jsplits = ffts[jfreq, :, jpol]
jwts = wmaps[jfreq, :, 0]
else:
jsplits = None
jwts = None
n2d[i, j] = noise_power(isplits,
iwts,
jsplits,
jwts,
coadd_estimator=coadd_estimator,
pfunc=naive_power)
if i != j: n2d[j, i] = n2d[i, j]
if plot_fname is not None:
plot("%s_%d_%s_%d_%s" \
% (plot_fname,ifreq,pols[ipol],
jfreq,pols[jpol]),
enmap.enmap(np.arcsinh(np.fft.fftshift(n2d[i,j])),wcs),dg=1,quantile=0)
return n2d
