Abstract:
Spherical pixelization schemes are reviewed that allow analyzing extended emission and, in particular, the cosmic microwave background. Problems with implementing different schemes are considered. The nonhierarchical Gauss–Legendre sky pixelization (GLESP) approach is discussed in detail.
Keywords:sky pixelization, data analysis, cosmic microwave background.
PACS:95.75.-z, 95.85.Bh, 98.80.-k, 98.80.Es
Received:June 14, 2012 Revised:July 18, 2012 Accepted: July 27, 2012