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[ascl:1704.007] PySM: Python Sky Model

PySM generates full-sky simulations of Galactic foregrounds in intensity and polarization relevant for CMB experiments. The components simulated are thermal dust, synchrotron, AME, free-free, and CMB at a given Nside, with an option to integrate over a top hat bandpass, to add white instrument noise, and to smooth with a given beam. PySM is based on the large-scale Galactic part of Planck Sky Model code and uses some of its inputs

Code site:
https://github.com/bthorne93/PySM_public
Appears in:
http://adsabs.harvard.edu/abs/2017ApJ...838...82S http://adsabs.harvard.edu/abs/2016arXiv160802841T
Bibcode:
2017ascl.soft04007T

ascl:1704.007
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