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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.
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Journal ArticleDOI
The three-dimensional power spectrum of galaxies from the sloan digital sky survey
Max Tegmark,Michael R. Blanton,Michael A. Strauss,Fiona Hoyle,David J. Schlegel,Roman Scoccimarro,Michael S. Vogeley,David H. Weinberg,Idit Zehavi,Andreas A. Berlind,Tamás Budavári,Andrew J. Connolly,Daniel J. Eisenstein,Douglas P. Finkbeiner,Joshua A. Frieman,Joshua A. Frieman,James E. Gunn,Andrew J. S. Hamilton,Lam Hui,Bhuvnesh Jain,David Johnston,David Johnston,Stephen M. Kent,Huan Lin,Reiko Nakajima,Robert C. Nichol,Jeremiah P. Ostriker,Adrian Pope,Ryan Scranton,Uroš Seljak,Ravi K. Sheth,Albert Stebbins,Alexander S. Szalay,István Szapudi,Licia Verde,Yongzhong Xu,James Annis,Neta A. Bahcall,Jon Brinkmann,Scott Burles,Francisco J. Castander,István Csabai,Jon Loveday,Mamoru Doi,Masataka Fukugita,J. Richard Gott,Greg Hennessy,David W. Hogg,Željko Ivezić,Gillian R. Knapp,D. Q. Lamb,Brian C. Lee,Robert H. Lupton,Timothy A. McKay,Peter Z. Kunszt,Jeffrey A. Munn,Liam O'Connell,John Peoples,Jeffrey R. Pier,Michael Richmond,Constance M. Rockosi,Donald P. Schneider,Christopher Stoughton,Douglas L. Tucker,Daniel E. Vanden Berk,Brian Yanny,Donald G. York +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.
Journal ArticleDOI
The 3D power spectrum of galaxies from the SDSS
Max Tegmark,Michael R. Blanton,Michael A. Strauss,Fiona Hoyle,David J. Schlegel,Roman Scoccimarro,Michael S. Vogeley,David H. Weinberg,I. Zehavi,Andreas A. Berlind,Tamás Budavári,A. J. Connolly,Daniel J. Eisenstein,Douglas P. Finkbeiner,Josh Frieman,James E. Gunn,Andrew J. S. Hamilton,Lam Hui,Bhuvnesh Jain,David Johnston,Steve Kent,Huan Lin,R. Nakajima,Robert C. Nichol,Jeremiah P. Ostriker,A. Pope,Ryan Scranton,Uroš Seljak,Ravi K. Sheth,A. Stebbins,Alexander S. Szalay,István Szapudi,Licia Verde,Yongzhong Xu +33 more
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.
Journal ArticleDOI
Cosmological constraints from the SDSS luminous red galaxies
Max Tegmark,Daniel J. Eisenstein,Michael A. Strauss,David H. Weinberg,Michael R. Blanton,Joshua A. Frieman,Joshua A. Frieman,Masataka Fukugita,James E. Gunn,Andrew J. S. Hamilton,Gillian R. Knapp,Robert C. Nichol,Jeremiah P. Ostriker,Nikhil Padmanabhan,Will J. Percival,David J. Schlegel,Donald P. Schneider,Roman Scoccimarro,Uroš Seljak,Uroš Seljak,Hee-Jong Seo,Molly E. C. Swanson,Alexander S. Szalay,Michael S. Vogeley,Jaiyul Yoo,Idit Zehavi,Kevork N. Abazajian,Scott F. Anderson,James Annis,Neta A. Bahcall,Bruce A. Bassett,Andreas A. Berlind,Jon Brinkmann,Tamás Budavári,Francisco J. Castander,Andrew J. Connolly,István Csabai,Mamoru Doi,Douglas P. Finkbeiner,Douglas P. Finkbeiner,Bruce Gillespie,Karl Glazebrook,Gregory S. Hennessy,David W. Hogg,Željko Ivezić,Željko Ivezić,Bhuvnesh Jain,David Johnston,Stephen M. Kent,D. Q. Lamb,Brian C. Lee,Huan Lin,Jon Loveday,Robert H. Lupton,Jeffrey A. Munn,Kaike Pan,Changbom Park,John Peoples,Jeffrey R. Pier,Adrian Pope,Michael Richmond,Constance M. Rockosi,Ryan Scranton,Ravi K. Sheth,Albert Stebbins,Christopher Stoughton,István Szapudi,Douglas L. Tucker,Daniel E. Vanden Berk,Brian Yanny,Donald G. York +70 more
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.
Journal ArticleDOI
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.
Journal ArticleDOI
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.