Analysis Issues for Large CMB Data Sets

Details Analysis Issues for Large CMB Data Sets Analysis Issues for Large CMB Data Sets

1998-12-18

arxiv.org/abs/astro-ph/9812350v1

Astronomy and Astrophysics

Astrophysics

6 pages, 2 postscript figures, uses tp.sty, tp9.sty. To appear in Proceedings of the MPA/ESO Conferece on Evolution of Large-S

Scientific paper

Multi-frequency, high resolution, full sky measurements of the anisotropy in both temperature and polarisation of the cosmic microwave background radiation are the goals of the satellite missions MAP (NASA) and Planck (ESA). The ultimate data products of these missions - multiple microwave sky maps, each of which will have to comprise more than 10^6 pixels in order to render the angular resolution of the instruments - will present serious challenges to those involved in the analysis and scientific exploitation of the results of both surveys. Some considerations of the relevant aspects of the mathematical structure of future CMB data sets are presented in this contribution. >>> for better on-screen rendition of the figures see <<< http://www.tac.dk/~healpix or http://www.mpa-garching.mpg.de/~cosmo/contributions.html

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