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Power Spectrum of Primordial Inhomogeneity Determined from the FOUR-Year [ITAL]COBE[/ITAL] DMR Sky Maps

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Górski, K. M., Banday, A. J., Bennett, C. L., Hinshaw, G., Kogut, A., Smoot, G. F., Wright, E. L.·1996·The Astrophysical Journal

Abstract

Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an incompletely sampled sky developed by Górski has been applied to the 4 yr COBE DMR 31.5, 53, and 90 GHz sky maps. Likelihood analysis using newly constructed Galaxy cuts (extended beyond | b | = 20° to excise the known foreground emission) and simultaneously correcting for the faint high-latitude Galactic foreground emission is conducted on the DMR sky maps pixelized in both ecliptic and Galactic coordinates. The Bayesian power spectrum estimation from the foreground-corrected 4 yr COBE DMR data renders n ~ 1.2 ± 0.3 and Q rms-PS ~ 15.3 −2.8 +3.7 μK (projections of the two-parameter likelihood). The results are consistent with the Harrison-Zeldovich n = 1 model of amplitude Q rms-PS ~ 18 μK detected with significance exceeding 14 σ (δ Q / Q ≲ 0.07). (A small power spectrum amplitude drop below the published 2 yr results is predominantly due to the application of the new, extended Galaxy cuts.)

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Metadata

Authors
Górski, K. M., Banday, A. J., Bennett, C. L., Hinshaw, G., Kogut, A., Smoot, G. F., & Wright, E. L.
Venue
The Astrophysical Journal
Published
1996-06-10
Volume
464
Issue
1
Pages
L11-L15
ISSN
0004-637X (ISSN-L)
OpenAlex
W2141436987
Cited by
230
References
0
FWCI
28.65
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Power Spectrum of Primordial Inhomogeneity Determined from the FOUR-Year [ITAL]COBE[/ITAL] DMR Sky Maps. https://app.cochat.ai/papers/10.1086/310077
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Górski, K. M., Banday, A. J., Bennett, C. L., Hinshaw, G., Kogut, A., Smoot, G. F., & Wright, E. L. (1996). Power Spectrum of Primordial Inhomogeneity Determined from the FOUR-Year [ITAL]COBE[/ITAL] DMR Sky Maps. The Astrophysical Journal. https://doi.org/10.1086/310077

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