The Wilkinson Microwave Anisotropy Probe
Abstract
Description
The Wilkinson Microwave Anisotropy Probe (WMAP) has mapped the full sky in five frequency bands between 23 and 94 GHz. The primary goal of the mission is to produce high-fidelity, all-sky, polarization-sensitive maps that can be used to study the cosmic microwave background. Systematic errors in the maps are constrained to new levels: using all-sky data, aspects of the anisotropy may confidently be probed to sub-microKelvin levels. We give a brief description of the instrument and an overview of the first results from an analysis of maps made with one year of data. The highlights are (1) the flat Lambda-CDM model fits the data remarkably well, whereas an Einstein-de Sitter model does not; (2) we see evidence of the birth of the first generation of stars at z ~ 20; (3) when the WMAP data are combined and compared with other cosmological probes, a cosmic consistency emerges: multiple different lines of inquiry lead to the same results.
To appear in Carnegie Observatories Astrophysics Series, Vol2 Measuring and Modeling the Universe, ed. W.L. Freedman,Cambridge University Press. Version with high-quality figures at http://ophelia.princeton.edu/~page/carnegie.pdf
To appear in Carnegie Observatories Astrophysics Series, Vol2 Measuring and Modeling the Universe, ed. W.L. Freedman,Cambridge University Press. Version with high-quality figures at http://ophelia.princeton.edu/~page/carnegie.pdf