Comments on the statistical analysis of excess variance in the COBE differential microwave radiometer maps

• Published in: The Astrophysical journal Vol. 420; no. 1; p. 1
• Main Authors: Wright, E. L., Smoot, G. F., Kogut, A., Hinshaw, G., Tenorio, L., Lineweaver, C., Bennett, C. L., Lubin, P. M.
• Format: Journal Article
• Language: English
• Published: Legacy CDMS 01.01.1994
• Subjects: Astrophysics
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1086/173537

Cosmic anisotrophy produces an excess variance sq sigma(sub sky) in the Delta maps produced by the Differential Microwave Radiometer (DMR) on cosmic background explorer (COBE) that is over and above the instrument noise. After smoothing to an effective resolution of 10 deg, this excess sigma(sub sky)(10 deg), provides an estimate for the amplitude of the primordial density perturbation power spectrum with a cosmic uncertainty of only 12%. We employ detailed Monte Carlo techniques to express the amplitude derived from this statistic in terms of the universal root mean square (rms) quadrupole amplitude, (Q sq/RMS)(exp 0.5). The effects of monopole and dipole subtraction and the non-Gaussian shape of the DMR beam cause the derived (Q sq/RMS)(exp 0.5) to be 5%-10% larger than would be derived using simplified analytic approximations. We also investigate the properties of two other map statistics: the actual quadrupole and the Boughn-Cottingham statistic. Both the sigma(sub sky)(10 deg) statistic and the Boughn-Cottingham statistic are consistent with the (Q sq/RMS)(exp 0.5) = 17 +/- 5 micro K reported by Smoot et al. (1992) and Wright et al. (1992).