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David T. Wilkinson

Researcher at Princeton University

Publications -  105
Citations -  12738

David T. Wilkinson is an academic researcher from Princeton University. The author has contributed to research in topics: Cosmic microwave background & Microwave. The author has an hindex of 42, co-authored 105 publications receiving 12243 citations. Previous affiliations of David T. Wilkinson include University of Colorado Boulder & University of Chicago.

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Structure in the COBE differential microwave radiometer first year maps

TL;DR: In this paper, the first year of data from the differential microwave radiometers on the Cosmic Background Explorer was presented, and the angular autocorrelation of the signal in each radiometer channel and cross-correlation between channels were consistent and gave a primordial fluctuation power-law spectrum with index of 1.1 +/- 0.5, and an rms-quadrupole-normalized amplitude of 16 +/- 4 micro-K.
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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.
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The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and Detections

TL;DR: The results of the DIRBE search were presented in this paper, showing that only the 140 and 240 μm data provided candidate detections of the CIB. But no plausible solar system or Galactic source of the observed 140 and 120 μm residuals can be identified, leading to the conclusion that the C IB has been detected at levels of νIν = 25 ± 7 and 14 ± 3 nW m-2 sr-1 at 140 and240 μm, respectively.