HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere
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[1] P. Frederickson,et al. Icosahedral Discretization of the Two-Sphere , 1985 .
[2] Chris Biemesderfer,et al. Astronomical Data Analysis Software and Systems X , 2001 .
[3] D. Healy,et al. Computing Fourier Transforms and Convolutions on the 2-Sphere , 1994 .
[4] E. Greisen,et al. Representations of celestial coordinates in FITS , 2002, astro-ph/0207413.
[5] Max Tegmark,et al. An Icosahedron-based Method for Pixelizing the Celestial Sphere , 1996, The Astrophysical Journal.
[6] E. Saff,et al. Distributing many points on a sphere , 1997 .
[7] A. Banday,et al. Evolution of large scale structure : from recombination to Garching : proceedings of the MPA-ESO Cosmology Conference : Garching, Germany, 2-7 August 1998 , 1999 .
[8] J. Silk. The Fundamental Parameters of Cosmology , 1999 .
[9] Alexander S. Szalay,et al. Astronomical archives of the future: a Virtual Observatory , 1999, Future Gener. Comput. Syst..
[10] Future Generation Computer Systems , 2000 .
[11] A. Melchiorri,et al. A flat Universe from high-resolution maps of the cosmic microwave background radiation , 2000, Nature.
[12] P. A. R. Ade,et al. Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the Cosmic Microwave Background from Two New Analyses of BOOMERANG Observations , 2002, astro-ph/0212229.
[13] S. Masi,et al. Cosmological constraints from archeops , 2002, astro-ph/0210306.
[14] S. Masi,et al. The cosmic microwave background anisotropy power spectrum measured by archeops , 2002, astro-ph/0210305.
[15] Edward J. Wollack,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results , 2003, astro-ph/0302207.