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Adam S. Bolton

Researcher at University of Utah

Publications -  68
Citations -  5976

Adam S. Bolton is an academic researcher from University of Utah. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 29, co-authored 68 publications receiving 5354 citations. Previous affiliations of Adam S. Bolton include Kitt Peak National Observatory & University of Hawaii.

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The Multi-object, Fiber-fed Spectrographs for the Sloan Digital Sky Survey and the Baryon Oscillation Spectroscopic Survey

Stephen A. Smee, +63 more
TL;DR: In this article, the design and performance of the multi-object fiber spectrographs for the Sloan Digital Sky Survey (SDSS) and their upgrade for the Baryon Oscillation Spectroscopic Survey (BOSS) were presented.
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The sloan lens acs survey. x. stellar, dynamical, and total mass correlations of massive early-type galaxies

TL;DR: In this paper, the authors used stellar masses, surface photometry, strong-lensing masses, and stellar velocity dispersions (σ e/2) to investigate empirical correlations for the definitive sample of 73 early-type galaxies (ETGs) that are strong gravitational lenses from the SLACS survey.
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The Initial Mass Function of Early-Type Galaxies

TL;DR: In this article, the authors determine an absolute calibration of the initial mass function (IMF) of early-type galaxies, by studying a sample of 56 gravitational lenses identified by the Sloan Lenses ACS Survey.
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measurements of the growth of structure and expansion rate at z = 0.57 from anisotropic clustering

TL;DR: In this paper, anisotropic clustering of massive galaxies from the Sloan Digital Sky Survey III Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 9 (DR9) sample is analyzed.
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The PRIsm MUlti-object Survey (PRIMUS). I. Survey Overview and Characteristics

TL;DR: The PRIMUS survey as mentioned in this paper uses a low-dispersion prism and slitmasks to observe ~2500 objects at once in a 0.18-deg2 field of view, using the Inamori Magellan Areal Camera and Spectrograph camera on the Magellan I Baade 6.5m telescope at Las Campanas Observatory.