Maximum-Likelihood Analysis of the COBE Angular Correlation Function
- 1 November 1993
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 417, L9
- https://doi.org/10.1086/187081
Abstract
We have used maximum-likelihood estimation to determine the quadrupole amplitude $Q_{
m rms-PS}$ and the spectral index $n$ 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 $Q_{
m rms-PS}=(15.7pm 2.6)exp[0.46(1-n)]mk$ for fixed $n$. Our result is slightly smaller than and has a smaller statistical uncertainty than the 1992 estimate of Smoot et al.Comment: 9 pages, AAS Latex v3.0, ApJL, in pres
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