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Pictures for the CMB-Talkby Alexander Merle T30d Group Seminar "Neutrinos & Cosmology" 2nd/9th December 2005

Pictures for the CMB-Talk

by Alexander Merle T30d Group Seminar "Neutrinos & Cosmology" 2nd/9th December 2005

#2

Taken over from Ned Wright The universe - a perfect black body

#3

The Monopole as measured by COBE  completely boring Taken over from Wayne Hu T=2.728 ± 0.002 K (G. Börner)

#4

accuracy of 10-3  clear dipole structure: origin: motion of the observer relative to the CMB frame  has to be subtracted Taken over from Wayne Hu

#5

At 10-5: The Milky Way as further distortion  has to be subtracted, too! Taken over from Wayne Hu

#6

After subtracting everything disturbing and at an accuracy of 10-5, the final COBE picture looks like:  angular resolution: 7°  BUT: How can one imagine that? Taken over from wikipedia.de

#7

The earth, as COBE would see it: TUM Taken over from Wayne Hu

#8

More precise: WMAP ( < 0.93° angular resolution) Taken from wikipedia.de & http://map.gsfc.nasa.gov  cosmological parameters

#9

The Power Spectrum measured by WMAP  tot = 1.02 ± 0.02 Bh² = 0.0224 ± 0.009 CDMh² = 0.135 ± 0.009  = 0.73 ± 0.04 (Params: G. Börner) Taken over from wikipedia.org @Werner: "" is called "Omega" and NOT "Sigma"!!! :-)

#10

The cosmological parameters can be "read off": Taken over from Wayne Hu

#11

Different regions of the power spectrum: Taken over from Wayne Hu

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Pictures for the CMB-Talkby Alexander Merle T30d Group Seminar "Neutrinos & Cosmology" 2nd/9th December 2005
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taken | wayn | subtract | wikipedia | cosmolog | cobe | resolut | wmap
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