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On the RMS Anisotropy at 7 degrees and 10 degrees Observed in the COBE-DMR Two Year Sky Maps | | A.J. Banday
; K.M. Gorski
; L. Tenorio
; E.L. Wright
; G.F. Smoot
; C.H. Lineweaver
; A. Kogut
; G. Hinshaw
; C.L. Bennett
; | | Date: |
30 Aug 1994 | | Journal: | Amer.Astron.Soc.Meeting 185 (1994) 5701 | | Abstract: | The frequency-independent RMS temperature fluctuations determined from the COBE-DMR two year sky maps are used to infer the parameter Q_{rms-PS}, which characterizes the normalization of power law models of primordial cosmological temperature anisotropy. In particular, a ’cross’-RMS statistic is used to determine Q_{rms-PS} for a forced fit to a scale-invariant Harrison-Zel’dovich (n = 1) spectral model. Using a joint analysis of the 7 degree and 10 degree RMS temperature derived from both the 53 and 90 GHz sky maps, we find Q_{rms-PS} = 17.0^{+2.5}_{-2.1} uK when the low quadrupole is included, and Q_{rms-PS} = 19.4^{+2.3}_{-2.1} uK excluding the quadrupole. These results are consistent with the n = 1 fits from more sensitive methods (e.g. power spectrum, correlation function). The effect of the low quadrupole derived from the COBE-DMR data on the inferred Q_{rms-PS} normalization is investigated. A bias to lower Q_{rms-PS} is found when the quadrupole is included. The higher normalization for a forced n = 1 fit is then favored by the cross-RMS technique. As initially pointed out in Wright et al. (1994a) and further discussed here, analytic formulae for the RMS sky temperature fluctuations will NOT provide the correct normalization amplitude. | | Source: | arXiv, astro-ph/9408097 | | Services: | Forum | Review | PDF | Favorites | |
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