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Andrew J. S. Hamilton

Researcher at University of Colorado Boulder

Publications -  170
Citations -  14049

Andrew J. S. Hamilton is an academic researcher from University of Colorado Boulder. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 52, co-authored 170 publications receiving 13387 citations. Previous affiliations of Andrew J. S. Hamilton include Joint Institute for Nuclear Research & JILA.

Papers
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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 3D power spectrum of galaxies from the SDSS

TL;DR: In this article, 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, with narrow and well-behaved window functions in the range 0.02 h/mpc < k < 0.3h/Mpc.
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Cosmological constraints from the SDSS luminous red galaxies

Max Tegmark, +70 more
- 11 Dec 2006 - 
TL;DR: In this paper, the authors employed a matrix-based power spectrum estimation method using pseudo-Karhunen-Loeve eigenmodes, producing uncorrelated minimum-variance measurements in 20 k-bands of both the clustering power and its anisotropy due to redshift-space distortions.
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Significance of the largest scale CMB fluctuations in WMAP

TL;DR: In this article, the authors investigate anomalies reported in the cosmic microwave background maps from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite on very large angular scales and discuss possible interpretations.
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High resolution foreground cleaned CMB map from WMAP

TL;DR: In this paper, an independent foreground analysis of the Wilkinson Microwave Anisotropy Probe (WMAP) maps is performed to produce a cleaned cosmic microwave background (CMB) map, which is useful for cross-correlation with, e.g., galaxy and x-ray maps.