Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE

J. Richard Bond; Andrew H. Jaffe

Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE

天体物理学 2007-05-23 v1

作者: J. Richard Bond , Andrew H. Jaffe

摘要

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. A simple prior probability method is used to include large scale structure observations. Estimates of the Hubble parameter, vacuum energy density, baryon fraction and primordial spectral tilt derived from the combined data are given.

关键词

cosmic microwave background cosmic microwave background polarization bayesian inference

引用

@article{arxiv.astro-ph/9610091,
  title  = {Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE},
  author = {J. Richard Bond and Andrew H. Jaffe},
  journal= {arXiv preprint arXiv:astro-ph/9610091},
  year   = {2007}
}

备注

13 pages, LaTeX, uses cmb.sty (included). To appear in the proceedings of the XXXIth Moriond meeting, ``Microwave Background Anisotropies.''

相关论文

查看更多相关论文 →