我有一个适合格式的伽马射线图(具有表面亮度的图像)以及 .hpx 作为 Aladin 转换器的输出。
我希望计算角功率谱。如何创建可读的文件
healpy.anafast
?我似乎弄错了数据格式(TypeErrors
)。
我试过的伽马射线图像之一是费米银河漫反射。该文件是一个公共 LAT 银河漫反射贴图,名称为gll_iem_v02_P6_V11_DIFFUSE.fit
:
http://fermi.gsfc.nasa.gov/ssc/data/access/lat/BackgroundModels.html
我在使用时粘贴了下面的代码,但它本质上是plot_wmap_power_spectra
在astroml上调用的脚本:
"""
WMAP power spectrum analysis with HealPy
----------------------------------------
This demonstrates how to plot and take a power spectrum of the WMAP data
using healpy, the python wrapper for healpix. Healpy is available for
download at the `github site <https://github.com/healpy/healpy>`_
"""
# Author: Jake VanderPlas <vanderplas@astro.washington.edu>
# License: BSD
# The figure is an example from astroML: see http://astroML.github.com
import numpy as np
from matplotlib import pyplot as plt
# warning: due to a bug in healpy, importing it before pylab can cause
# a segmentation fault in some circumstances.
import pylab
import healpy as hp
###
from astroML.datasets import fetch_wmap_temperatures
###
#------------------------------------------------------------
# Fetch the data
###
wmap_unmasked = fetch_wmap_temperatures(masked=False)
#PredictedSurfaceFluxFromModelMap = np.arange(hp.read_map('PredictedSurfaceFluxFromModelMap.hpx[1]'))
PredictedSurfaceFluxFromModelMap = hp.read_map('gll_iem_v02_p6_V11_DIFFUSE.fit',dtype=np.float,verbose=True)
#PredictedSurfaceFluxFromModelMap = hp.read_map('all.fits',dtype=np.float,verbose=True)
#cl_out = hp.read_cl('PredictedSurfaceFluxFromModelMap.hpx',dtype=np.float)#,verbose=True)
wmap_masked = fetch_wmap_temperatures(masked=True)
###
white_noise = np.ma.asarray(np.random.normal(0, 0.062, wmap_masked.shape))
len(cl_out)
#------------------------------------------------------------
# plot the unmasked map
fig = plt.figure(1)
#hp.mollview(wmap_unmasked, min=-1, max=1, title='Unmasked map',
# fig=1, unit=r'$\Delta$T (mK)')
########----------------
##hp.mollview(PredictedSurfaceFluxFromModelMap, min=-1, max=1, title='Unmasked map',
## fig=1, unit=r'$\Delta$T (mK)')
########----------------
#------------------------------------------------------------
# plot the masked map
# filled() fills the masked regions with a null value.
########----------------
#fig = plt.figure(2)
#hp.mollview(wmap_masked.filled(), title='Masked map',
# fig=2, unit=r'$\Delta$T (mK)')
########----------------
#------------------------------------------------------------
# compute and plot the power spectrum
########----------------
#cl = hp.anafast(wmap_masked.filled(), lmax=1024)
cl = hp.anafast(PredictedSurfaceFluxFromModelMap, lmax=1024)
#cl = cl_out
########----------------
ell = np.arange(len(cl))
cl_white = hp.anafast(white_noise, lmax=1024)
fig = plt.figure(3)
ax = fig.add_subplot(111)
ax.scatter(ell, ell * (ell + 1) * cl,
s=4, c='black', lw=0,
label='data')
ax.scatter(ell, ell * (ell + 1) * cl_white,
s=4, c='gray', lw=0,
label='white noise')
ax.set_xlabel(r'$\ell$')
ax.set_ylabel(r'$\ell(\ell+1)C_\ell$')
ax.set_title('Angular Power (not mask corrected)')
ax.legend(loc='upper right')
ax.grid()
ax.set_xlim(0, 1100)
plt.show()