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Robert C. Nichol

Researcher at Institute of Cosmology and Gravitation, University of Portsmouth

Publications -  860
Citations -  176885

Robert C. Nichol is an academic researcher from Institute of Cosmology and Gravitation, University of Portsmouth. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 187, co-authored 851 publications receiving 162994 citations. Previous affiliations of Robert C. Nichol include University of Chicago & South East Physics Network.

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The three-dimensional power spectrum of galaxies from the sloan digital sky survey

Max Tegmark, +66 more
TL;DR: In this paper, the authors employed a matrix-based method using pseudo-Karhunen-Loeve eigenmodes, producing uncorrelated minimum-variance measurements in 22 k-bands of both the clustering power and its anisotropy due to redshift-space distortions.
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The ninth data release of the sloan digital sky survey: First spectroscopic data from the sdss-iii baryon oscillation spectroscopic survey

Christopher P. Ahn, +259 more
TL;DR: In this paper, the authors presented the first spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS) for the Sloan Digital Sky Survey III (SDSS-III) dataset.
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The Sixth Data Release of the Sloan Digital Sky Survey

Jennifer K. Adelman-McCarthy, +173 more
TL;DR: The Sixth Data Release of the Sloan Digital Sky Survey (SDS) as discussed by the authors contains images and parameters of roughly 287 million objects over 9583 deg(2), including scans over a large range of Galactic latitudes and longitudes.
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The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III

Hiroaki Aihara, +194 more
TL;DR: The first data release of SDSS-III is described in this article, which includes five-band imaging of roughly 5200 deg2 in the southern Galactic cap, bringing the total footprint of the Sloan Digital Sky Survey imaging to 14,555 deg2, or over a third of the Celestial Sphere.
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Quantifying the Bimodal Color-Magnitude Distribution of Galaxies

TL;DR: In this article, the bimodality of the distribution from luminous to faint galaxies is traced by fitting double Gaussians to the color functions separated in absolute magnitude bins.