我有一个伽马射线地图(图像与表面亮度)在fits格式,也.hpx作为输出的阿拉丁转换器。
我想要计算角功率谱。如何创建healpy.anafast可读的文件?我似乎弄错了数据格式(TypeErrors)。
我尝试的伽马射线图像之一是费米银河系漫射。该文件是位于以下位置的名为gll_iem_v02_P6_V11_DIFFUSE.fit的公共LAT银河漫反射贴图:
http://fermi.gsfc.nasa.gov/ssc/data/access/lat/BackgroundModels.html
我在使用时粘贴了下面的代码,但它实际上是astroml上名为plot_wmap_power_spectra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()发布于 2013-11-20 05:56:01
I have uploaded your map also to Figshare,其中很可能在未来可用。
获得HEALPix格式的地图后,只需使用healpy即可轻松读取
import healpy as hp
m = hp.ma(hp.read_map("gll_iem_v02_p6_V11_DIFFUSE.hpx"))遮罩NaN像素:
m.mask = np.isnan(m)绘制它:
hp.mollview(m, min=-1e-5, max=1e-5, xsize=2000)
title("gll_iem_v02_p6_V11_DIFFUSE")

计算并绘制角功率谱:
plt.loglog(hp.anafast(m))

另请参阅IPython笔记本:http://nbviewer.ipython.org/7553252
https://stackoverflow.com/questions/20080176
复制相似问题