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James E. Gunn

Researcher at Princeton University

Publications -  405
Citations -  62562

James E. Gunn is an academic researcher from Princeton University. The author has contributed to research in topics: Galaxy & Quasar. The author has an hindex of 124, co-authored 399 publications receiving 59599 citations. Previous affiliations of James E. Gunn include California Institute of Technology & Pennsylvania State University.

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The clustering of galaxies in the sdss-iii baryon oscillation spectroscopic survey: Baryon acoustic oscillations in the data release 9 spectroscopic galaxy sample

Lauren Anderson, +76 more
TL;DR: In this paper, the authors present a measurement of the cosmic distance scale from detections of the baryon acoustic oscillations in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey III (SDSS-III).
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SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

Daniel J. Eisenstein, +239 more
TL;DR: SDSS-III as discussed by the authors is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars.
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The u'g'r'i'z' Standard Star Network

TL;DR: In this paper, the 158 standard stars that define the u'g'r'i'z' photometric system were presented, which form the basis for the photometric calibration of the Sloan Digital Sky Survey (SDSS).
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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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The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies

TL;DR: In this paper, the authors explored the impact of uncertainties in key phases of stellar evolution and the IMF on the derived physical properties of galaxies and the expected luminosity evolution for a passively evolving set of stars.