English

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 QrmsPSQ_{\rm rms-PS} and the spectral index nn 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 QrmsPS=(15.7±2.6)exp[0.46(1n)]\mkQ_{\rm rms-PS}=(15.7\pm 2.6)\exp[0.46(1-n)]\mk for fixed nn. 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