Cosmic Parameter Estimation Combining Sub-Degree Cmb Experiments With Cobe
We describe the Bayesian-based signal-to-noise eigenmode method for cosmological parameter estimation, show how it can be used to optimally compress large CMB anisotropy data sets to manageable sizes, and apply it to the DMR 4-year, South Pole and Saskatchewan data, individually and in combination....
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Format: | Text |
Language: | English |
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1996
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Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.24.7775 http://cfpa.berkeley.edu/~jaffe/papers/procs/moriond.ps.gz |