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The analysis of Cosmic Microwave Background (CMB) observations is a long-standing computational challenge, driven by the exponential growth in the size of the data sets being gathered. Since this growth is projected to continue for at least the next decade, it will be critical to extend the analysis algorithms and their implementations to peta-scale high performance computing (HPC) systems and beyond. The most computationally intensive part of the analysis is generating and reducing Monte Carlodoi:10.1145/1995896.1995944 dblp:conf/ics/SudarsanBCKMOZS11 fatcat:4etfpyhpbnfbtj63foexy75hkm