A Python package for interfacing the Cosmoglobe Sky Model with commander3 outputs for the purpose of producing astrophysical sky maps.
Project description
cosmoglobe is a python package that interfaces the Cosmoglobe Sky Model with Commander outputs for the purpose of producing astrophysical sky maps.
Features
See the documentation for amore comprehensive guide.
Initialize Sky Model from Chain:
import cosmoglobe
chain = cosmoglobe.get_test_chain() # Downloads a minimal Commander chainfile.
model = cosmoglobe.model_from_chain(chain, nside=256)
Simulate the sky at 150 GHz in units of MJy/sr, smoothed to 40 arcmin with a gaussian beam:
import astropy.units as u
emission = model(150*u.GHz, fwhm=40*u.arcmin, output_unit="MJy/sr")
Integrate over a bandpass:
import numpy as np
import healpy as hp
import matplotlib.pyplot as plt
# Reading in WMAP K-band bandpass profile.
bandpass_frequencies, bandpass_weights = np.loadtxt(wmap_bandpass.txt, unpack=True)
# The units of the detector must be specified even if the bandpass is pre-normalized.
bandpass_weights *= u.Unit("K_RJ") # Specify K_RJ or K_CMB
bandpass_frequencies *= u.GHz
model.remove_dipole() # Remove the dipole from the CMB component
emission = model(
freqs=bandpass_frequencies,
weights=bandpass_weights,
fwhm=0.8*u.deg,
output_unit="mK_RJ",
)
hp.mollview(emission[0], hist="norm") # Plotting the intensity
plt.show()
Installation
cosmoglobe can be installed via pip
pip install cosmoglobe
Funding
This work has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreements No 776282 (COMPET-4; BeyondPlanck), 772253 (ERC; bits2cosmology) and 819478 (ERC; Cosmoglobe).
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