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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Bibliographic Details
Main Authors: Bond, J. Richard, Jaffe, Andrew H.
Format: Report
Language:unknown
Published: arXiv 1996
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/9610091
https://arxiv.org/abs/astro-ph/9610091