110 lines
3.2 KiB
Python
110 lines
3.2 KiB
Python
|
import healpy as hp
|
||
|
import numpy as np
|
||
|
import cosmotool as ct
|
||
|
import argparse
|
||
|
import h5py as h5
|
||
|
from matplotlib import pyplot as plt
|
||
|
|
||
|
Mpc=3.08e22
|
||
|
rhoc = 1.8864883524081933e-26 # m^(-3)
|
||
|
sigmaT = 6.6524e-29
|
||
|
mp = 1.6726e-27
|
||
|
lightspeed = 299792458.
|
||
|
v_unit = 1e3 # Unit of 1 km/s
|
||
|
T_cmb=2.725
|
||
|
h = 0.71
|
||
|
Y = 0.245 #The Helium abundance
|
||
|
Omega_matter = 0.26
|
||
|
Omega_baryon=0.0445
|
||
|
|
||
|
G=6.67e-11
|
||
|
MassSun=2e30
|
||
|
frac_electron = 1.0 # Hmmmm
|
||
|
frac_gas_galaxy = 0.14
|
||
|
mu = 1/(1-0.5*Y)
|
||
|
|
||
|
baryon_fraction = Omega_baryon / Omega_matter
|
||
|
|
||
|
ksz_normalization = T_cmb*sigmaT*v_unit/(lightspeed*mu*mp) * baryon_fraction
|
||
|
rho_mean_matter = Omega_matter * (3*(100e3/Mpc)**2/(8*np.pi*G))
|
||
|
|
||
|
parser=argparse.ArgumentParser(description="Generate Skymaps from CIC maps")
|
||
|
parser.add_argument('--boxsize', type=float, required=True)
|
||
|
parser.add_argument('--Nside', type=int, default=128)
|
||
|
parser.add_argument('--base_h5', type=str, required=True)
|
||
|
parser.add_argument('--base_fig', type=str, required=True)
|
||
|
parser.add_argument('--start', type=int, required=True)
|
||
|
parser.add_argument('--end', type=int, required=True)
|
||
|
parser.add_argument('--step', type=int, required=True)
|
||
|
parser.add_argument('--minval', type=float, default=-0.5)
|
||
|
parser.add_argument('--maxval', type=float, default=0.5)
|
||
|
parser.add_argument('--depth_min', type=float, default=10)
|
||
|
parser.add_argument('--depth_max', type=float, default=60)
|
||
|
parser.add_argument('--iid', type=int, default=0)
|
||
|
parser.add_argument('--ksz_map', type=str, required=True)
|
||
|
args = parser.parse_args()
|
||
|
|
||
|
L = args.boxsize
|
||
|
Nside = args.Nside
|
||
|
|
||
|
def build_sky_proj(density, dmax=60.,dmin=0,iid=0):
|
||
|
|
||
|
N = density.shape[0]
|
||
|
ix = (np.arange(N)-0.5)*L/N - 0.5 * L
|
||
|
|
||
|
|
||
|
dist2 = (ix[:,None,None]**2 + ix[None,:,None]**2 + ix[None,None,:]**2)
|
||
|
|
||
|
flux = density.transpose().astype(ct.DTYPE) # / dist2
|
||
|
dmax=N*dmax/L
|
||
|
dmin=N*dmin/L
|
||
|
if iid == 0:
|
||
|
shifter = np.array([0.5,0.5,0.5])
|
||
|
else:
|
||
|
shifter = np.array([0.,0.,0.])
|
||
|
|
||
|
projsky1 = ct.spherical_projection(Nside, flux, dmin, dmax, integrator_id=iid, shifter=shifter)
|
||
|
|
||
|
return projsky1*L/N
|
||
|
|
||
|
def build_unit_vectors(N):
|
||
|
ii = np.arange(N)*L/N - 0.5*L
|
||
|
d = np.sqrt(ii[:,None,None]**2 + ii[None,:,None]**2 + ii[None,None,:]**2)
|
||
|
d[N/2,N/2,N/2] = 1
|
||
|
ux = ii[:,None,None] / d
|
||
|
uy = ii[None,:,None] / d
|
||
|
uz = ii[None,None,:] / d
|
||
|
|
||
|
return ux,uy,uz
|
||
|
|
||
|
for i in xrange(args.start,args.end,args.step):
|
||
|
ff=plt.figure(1)
|
||
|
plt.clf()
|
||
|
with h5.File(args.base_h5 % i, mode="r") as f:
|
||
|
p = f['velocity'][:]
|
||
|
davg = np.average(np.average(np.average(f['density'][:],axis=0),axis=0),axis=0)
|
||
|
p /= davg # Now we have momentum scaled to the mean density
|
||
|
|
||
|
# Rescale by Omega_b / Omega_m
|
||
|
p = p.astype(np.float64)
|
||
|
print p.max(), p.min(), ksz_normalization, rho_mean_matter
|
||
|
p *= -ksz_normalization*rho_mean_matter*1e6
|
||
|
|
||
|
ux,uy,uz = build_unit_vectors(p.shape[0])
|
||
|
pr = p[:,:,:,0] * ux + p[:,:,:,1] * uy + p[:,:,:,2] * uz
|
||
|
print p.max(), p.min()
|
||
|
print pr.max()*Mpc, pr.min()*Mpc
|
||
|
|
||
|
@ct.timeit_quiet
|
||
|
def run_proj():
|
||
|
return build_sky_proj(pr*Mpc, dmin=args.depth_min,dmax=args.depth_max,iid=args.iid)
|
||
|
|
||
|
run_proj()
|
||
|
|
||
|
hp.write_map(args.ksz_map % i, proj)
|
||
|
|
||
|
hp.mollview(proj, fig=1, coord='CG', cmap=plt.cm.coolwarm, title='Sample %d' % i, min=args.minval,
|
||
|
max=args.maxval)
|
||
|
|
||
|
ff.savefig(args.base_fig % i)
|