Figures from the Nine-Year WMAP papers in a form suitable for use in talks.
Please acknowledge the WMAP Science Team when using
these images.
Bennett, et al. Figures from the paper "Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results" in a form suitable for use in talks. Please acknowledge the WMAP Science Team when using these images.
Hinshaw, et al. Figures from the paper "Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmology Results" in a form suitable for use in talks. Please acknowledge the WMAP Science Team when using these images.
The images below represent full-sky maps of the cosmic microwave background anisotropy and foreground signal from our galaxy (in red). The 5 frequency maps are constructed from the differential time-ordered observations of the ten WMAP differencing assemblies. Galactic foreground is stongest in K band, weakest in V and W bands.
Please acknowledge the WMAP Science Team when using
these images.
K-Band Map (23 GHz) Linear scale from -200 to 200 uK
The Internal Linear Combination Map is a weighted linear combination of the five WMAP frequency maps. The weights are computed using criteria which minimize the Galactic foreground contribution to the sky signal. The resultant map provides a low-contamination image of the CMB anisotropy.
Please acknowledge the WMAP Science Team when using
these images.
Internal Linear Combination Map Galactic coordinates, Mollweide projection Linear scale from -200 to 200 uK