A method for extracting maximum resolution power spectra from microwave sky maps

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 1, 1996, Pages 299-308

  Tegmark, Max ^a  

^a MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

Author keywords

Cosmic microwave background; Large scale structure of Universe; Methods: data analysis

Indexed keywords

EIGENVALUES AND EIGENFUNCTIONS; GALAXIES; POWER SPECTRUM; SIGNAL TO NOISE RATIO;

COSMIC MICROWAVES BACKGROUND; HIGH RESOLUTION; LARGE SCALE STRUCTURE OF UNIVERSE; MAXIMUM RESOLUTION; METHODS. DATA ANALYSIS; POWER-SPECTRA; RESOLUTION POWER; SKY COVERAGE; SPHERICAL HARMONICS; WEIGHT FUNCTIONS;

COSMOLOGY;

EID: 0000083018     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.1.299     Document Type: Article

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