Simulated CMB maps at 0°.5 resolution: Basic results

Details Simulated CMB maps at 0°.5 resolution: Basic results Simulated CMB maps at 0°.5 resolution: Basic results

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..336..485h&link_type=abstract

Dark matter. AIP Conference Proceedings, Volume 336, pp. 485-488 (1995).

Physics

Dark Matter, Background Radiations

Scientific paper

We have simulated full-sky maps of the Cosmic Microwave Background (CMB) anisotropy expected from Cold Dark Matter (CDM) models at 0°.5 and 1°.0 angular resolution. Statistical properties of the maps are presented as a function of sky coverage, angular resolution, and instrument noise, and the implications of these results for observability of the Doppler peak are discussed. We find that sensitivity to the Doppler peak depends primarily on the fraction of sky covered, and only secondarily on the angular resolution and noise level. A sample map simulation is presented to illustrate the anisotropies.

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