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Open AccessJournal ArticleDOI

Microwave Emission at High Galactic Latitudes in the Four-Year DMR Sky Maps

TLDR
In this article, the COBE Differential Microwave Radiometers (DMR) 4 yr sky maps were used to model Galactic microwave emission at high latitudes (|b| > 20°).
Abstract
We use the COBE Differential Microwave Radiometers (DMR) 4 yr sky maps to model Galactic microwave emission at high latitudes (|b| > 20°). Cross-correlation of the DMR maps with Galactic template maps detects fluctuations in the high-latitude microwave sky brightness with the angular variation of the DIRBE far-infrared dust maps and a frequency dependence consistent with a superposition of dust and free-free emission. We find no significant correlations between the DMR maps and various synchrotron templates. On the largest angular scales (e.g., quadrupole), Galactic emission is comparable in amplitude to the anisotropy in the cosmic microwave background (CMB). The CMB quadrupole amplitude, after correction for Galactic emission, has amplitude Qrms = 10.7 μK with random uncertainty 3.6 μK and systematic uncertainty 7.1 μK from uncertainty in our knowledge of Galactic microwave emission.

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Citations
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The Cosmological Constant and Dark Energy

TL;DR: A review of dark energy can be found in this paper, where the authors present the basic physics and astronomy of the subject, reviews the history of ideas, assesses the state of the observational evidence, and comments on recent developments in the search for a fundamental theory.
Journal ArticleDOI

Interstellar dust grains

TL;DR: In this article, the authors survey the observed properties of interstellar dust grains: the wavelength-dependent extinction of starlight, including absorption features, from UV to infrared; optical luminescence; and optical luminance.
Journal ArticleDOI

Non-Gaussianity from inflation: theory and observations

TL;DR: A review of models of inflation and their predictions for the primordial non-Gaussianity in the density perturbations which are thought to be at the origin of structures in the Universe is given in this article.
References
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Journal ArticleDOI

Four-Year COBE* DMR Cosmic Microwave Background Observations: Maps and Basic Results

TL;DR: In this article, the spatial properties of the cosmic microwave background radiation based on the full 4 yr of COBE Differential Microwave Radiometer (DMR) observations, with additional details in a set of companion Letters, are presented.
Journal ArticleDOI

4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results

TL;DR: In this paper, a summary of the spatial properties of the cosmic microwave background radiation based on the full 4 years of COBE DMR observations, as detailed in a set of companion Letters, is presented.
Journal ArticleDOI

Preliminary spectral observations of the Galaxy with a 7 deg beam by the Cosmic Background Explorer (COBE)

TL;DR: The FIR absolute spectrophotometer (FIRAS) on the Cosmic Background Explorer (COBE) has carried out the first all-sky spectral line survey in the FIR region, as well as mapping spectra of the Galactic dust distribution at below 100 microns as discussed by the authors.
Journal ArticleDOI

Power spectrum of primordial inhomogeneity determined from the four year COBE DMR sky maps

TL;DR: In this paper, the authors applied Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an incompletely sampled sky developed by Gorski has been applied to the 4 yr COBE DMR 31.5, 53, and 90 GHz sky maps.
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