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Maximum-Likelihood Analysis of the COBE Angular Correlation Function

Uros Seljak, Edmund Bertschinger

astro-pharXiv:astro-ph/9309003

Abstract

We have used maximum-likelihood estimation to determine the quadrupole amplitude Q rms-PS and the spectral index n of the density fluctuation power spectrum at recombination from the \ DMR data. We find a strong correlation between the two parameters of the form Q rms-PS=(15.7 2.6)[0.46(1-n)] for fixed n. Our result is slightly smaller than and has a smaller statistical uncertainty than the 1992 estimate of Smoot et al.

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