File:WMAP 5 year CMB Power Spectra.png
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| Description | WMAP 5-year EE power spectrum, compared with results from the Boomerang (Montroy et al., 2006, green), CBI (Sievers et al. 2007, red), CAPMAP (Bischoff et al., 2008, orange), QUAD (Ade, et al., 2007, purple), and DASI (Leitch et al., 2005, blue) experiments. The pink curve is the best-fit theory spectrum from the ΛCDM/WMAP Markov chain (Dunkley et al., 2008). |
| Date | 03/18/08 |
| Source | http://lambda.gsfc.nasa.gov/product/map/pub_papers/fiveyear/power_spectra/wmap_mn5_images.cfm |
| Author | M. Nolta, et al., 2009, ApJS, 180, 296-305 |
| Permission (Reusing this file) |
U.S. Goveernment |
| Other versions | http://lambda.gsfc.nasa.gov/product/map/pub_papers/fiveyear/power_spectra/wmap_mn5_images.cfm |
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 07:54, 10 July 2010 | | 2,048 × 1,381 (29 KB) | Black Shadow | {{Information |Description = WMAP 5-year EE power spectrum, compared with results from the Boomerang (Montroy et al., 2006, green), CBI (Sievers et al. 2007, red), CAPMAP (Bischoff et al., 2008, orange), QUAD (Ade, et al., 2007, purple), and DASI (Leitch |
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