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....
Main Authors: | , |
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Format: | Report |
Language: | unknown |
Published: |
arXiv
1996
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Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/9610091 https://arxiv.org/abs/astro-ph/9610091 |