Maximum-Likelihood Analysis of the COBE Angular Correlation Function
Astrophysics
2009-10-22 v1
Abstract
We have used maximum-likelihood estimation to determine the quadrupole amplitude and the spectral index of the density fluctuation power spectrum at recombination from the \cobe\ DMR data. We find a strong correlation between the two parameters of the form for fixed . Our result is slightly smaller than and has a smaller statistical uncertainty than the 1992 estimate of Smoot et al.
Cite
@article{arxiv.astro-ph/9309003,
title = {Maximum-Likelihood Analysis of the COBE Angular Correlation Function},
author = {Uros Seljak and Edmund Bertschinger},
journal= {arXiv preprint arXiv:astro-ph/9309003},
year = {2009}
}
Comments
9 pages, AAS Latex v3.0, ApJL, in press