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PySM: Python Sky Model

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Ada Coda
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PySM: Python Sky Model

Postby Ada Coda » Sun Apr 30, 2017 12:25 am

PySM: Python Sky Model

Abstract: 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

Credit: Thorne, Ben; Alonso, David; Naess, Sigurd; Dunkley, Jo

Site: https://github.com/bthorne93/PySM_public
http://adsabs.harvard.edu/abs/2016arXiv160802841T

Bibcode: 2017ascl.soft04007T

Preferred citation method: http://adsabs.harvard.edu/abs/2016arXiv160802841T

ID: ascl:1704.007

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