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[ascl:1712.005] draco: Analysis and simulation of drift scan radio data

draco analyzes transit radio data with the m-mode formalism. It is telescope agnostic, and is used as part of the analysis and simulation pipeline for the CHIME (Canadian Hydrogen Intensity Mapping Experiment) telescope. It can simulate time stream data from maps of the sky (using the m-mode formalism) and add gain fluctuations and correctly correlated instrumental noise (i.e. Wishart distributed). Further, it can perform various cuts on the data and make maps of the sky from data using the m-mode formalism.

Code site:
https://github.com/radiocosmology/draco
Appears in:
http://adsabs.harvard.edu/abs/2015PhRvD..91h3514S
Bibcode:
2017ascl.soft12005S

ascl:1712.005
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