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External
Correlations of the CMB
and Cosmology May 25-27, 2006. Fermilab, Batavia, IL ![]() |
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The workshop is over! Many thanks to all of the participants most of whose talks are now available on the Agenda Page We encourage all who are working on or with these correlations, or any interested in them to attend. BACKGROUND: Subtle correlations between the Cosmic Microwave Background (CMB) and foreground large scale structure (LSS) provide a new and different window on cosmology than that obtained from CMB and LSS analyzed separately. A variety of physical effects associated with the LSS will cause small changes in the CMB temperature/polarization pattern which in turn induces small but measurable angular correlations between the CMB and the LSS.
The various effects and the corresponding LSS properties they probe can be differentiated by the angular, redshift, and spectral patterns of the correlations. The different properties are themselves sensitive to the cosmological model in different ways. It is only with the recent availability of the combination of large area and fine resolution/sampling in overlapping CMB maps (e.g. WMAP) and deep LSS surveys (e.g. SDSS or 2dF) that these small correlations could be measured. In the near future the amount and quality of data for these studies will increase enormously with projects such as ACT, AMiBA, APEX, CFHTLS, DES, LSST, JDEM, Pan-STARRS, Planck, and SPT. The workshop will cover
1st Announcement 2nd Announcement 3rd Announcement Administrative Contact: sazama.at. fnal.gov |
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