MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets
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C. B. Netterfield | B. P. Crill | E. Hivon | IPAC | K. M. Gorski | ESO | Ipac | U. Toronto | K. Gorski | E. Hivon | F. Hansen | C. Netterfield | B. Crill | S. Prunet | Eső | Cita | Mpa | S. Prunet | MPA | CITA | F. Caltech | W. Obs. | F. Hansen Caltech | Warsaw Obs | U of Toronto | K. Górski
[1] J. R. Bond,et al. Radical Compression of Cosmic Microwave Background Data , 2000 .
[2] Alexander S. Szalay,et al. Fast Cosmic Microwave Background Analyses via Correlation Functions , 2001 .
[3] R. Bond,et al. Signal-to-noise eigenmode analysis of the two-year COBE maps. , 1994, Physical review letters.
[4] J. Magueijo,et al. OBSERVABILITY OF SECONDARY DOPPLER PEAKS IN THE COSMIC MICROWAVE BACKGROUND RADIATION POWER SPECTRUM BY EXPERIMENTS WITH SMALL FIELDS , 1996, astro-ph/9603064.
[5] C. Lawrence,et al. Evolution of Large-Scale Structure , 1998 .
[6] P. Natoli,et al. Fast Spherical Harmonic Analysis: A Quick Algorithm for Generating and/or InvertingFull-Sky, High-Resolution Cosmic Microwave Background Anisotropy Maps , 1997, astro-ph/9703084.
[7] G. Hinshaw,et al. Structure in the COBE differential microwave radiometer first-year maps , 1992 .
[8] E. Hivon,et al. Analysis issues for large CMB data sets , 1998, astro-ph/9812350.
[9] V. V. Hristov,et al. MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10'-5° , 2000, astro-ph/0005123.
[10] O. Dor'e,et al. MAPCUMBA: A fast iterative multi-grid map-making algorithm for CMB experiments , 2001, astro-ph/0101112.
[11] P. Natoli,et al. A Map-Making algorithm for the Planck Surveyor , 2001 .
[12] Max Tegmark. How to Make Maps from Cosmic Microwave Background Data without Losing Information , 1996, astro-ph/9611130.
[13] Robert Lupton,et al. Statistics in Theory and Practice , 2020 .
[14] Andrew H. Jaffe,et al. Simultaneous Estimation of Noise and Signal in Cosmic Microwave Background Experiments , 1999, astro-ph/9909250.
[15] J. Borrill,et al. Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments , 2000, astro-ph/0007212.
[16] A. Melchiorri,et al. A flat Universe from high-resolution maps of the cosmic microwave background radiation , 2000, Nature.
[17] Max Tegmark,et al. A method for extracting maximum resolution power spectra from microwave sky maps , 1994, astro-ph/9412064.
[18] Adrian T. Lee,et al. A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data , 2001, astro-ph/0104459.
[19] U. Toronto,et al. Estimating the power spectrum of the cosmic microwave background , 1997, astro-ph/9708203.
[20] Krzysztof M. Gorski. On determining the spectrum of primordial inhomogeneity from the COBE DMR sky maps: Method , 1994 .
[21] J. E. Carlstrom,et al. FIRST INTRINSIC ANISOTROPY OBSERVATIONS WITH THE COSMIC BACKGROUND IMAGER , 2001 .
[22] F Scaramuzzi,et al. Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations. , 2001, Physical review letters.
[23] David N. Spergel,et al. An Efficient Technique to Determine the Power Spectrum from Cosmic Microwave Background Sky Maps , 1998, astro-ph/9805339.
[24] Max Tegmark,et al. A Brute Force Analysis of the COBE DMR Data , 1994, astro-ph/9412005.
[25] P. Fosalba,et al. All-sky convolution for polarimetry experiments , 2000, astro-ph/0008228.