N. Jarosik

TL;DR: In this paper, the authors use the Wilkinson Microwave Anisotropy Probe (WMAP) data, in combination with complementary small-scale cosmic microwave background (CMB) measurements and large-scale structure data, to explore the parameter space of inflationary models that is consistent with the WMAP data.

TL;DR: In this article, the authors examined the properties of the power spectrum data with respect to the six-parameter CDM model and found no significant anomalies, and concluded that there is no compelling evidence for deviations from the?CDM model, which is generally an acceptable statistical fit to WMAP and other cosmological data.

TL;DR: In this article, the authors used the power spectrum of differences between multi-frequency template-cleaned maps, and found no evidence for foreground contamination outside of the updated (KQ85y7) foreground mask.

TL;DR: In this paper, the authors presented WMAP seven-year observations of bright sources which are often used as calibrators at microwave frequencies, including the outer planets (Mars, Jupiter, Saturn, Uranus, and Neptune) and five fixed celestial sources (Cas A, Tau A, Cyg A, 3C274, and 3C58).

TL;DR: In this paper, the angular power spectrum of the anisotropy in the cosmic microwave background (CMB) was measured in 23 different multipole bands from l = 54 (≈ 3°) to l = 404 ( ≥ 045) and in six frequency bands from 26 to 46 GHz over three observing seasons.