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Josh Frieman

Researcher at Fermilab

Publications -  176
Citations -  11356

Josh Frieman is an academic researcher from Fermilab. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 38, co-authored 176 publications receiving 9344 citations. Previous affiliations of Josh Frieman include Stanford University & University of Chicago.

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Journal ArticleDOI

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.
Posted Content

LSST Science Book, Version 2.0

Paul A. Abell, +245 more
TL;DR: The Large Synoptic Survey Telescope (LSST) as discussed by the authors will have an effective aperture of 6.7 meters and an imaging camera with field of view of 9.6 degrees.
Journal ArticleDOI

The dark energy camera

B. Flaugher, +121 more
TL;DR: The Dark Energy Camera as mentioned in this paper was designed and constructed by the Dark Energy Survey Collaboration, and meets or exceeds the stringent requirements designed for the wide-field and supernova surveys for which the collaboration uses it.
Journal ArticleDOI

The Dark Energy Camera

B. Flaugher, +117 more
TL;DR: The Dark Energy Camera as discussed by the authors was designed and constructed by the Dark Energy Survey Collaboration, and meets or exceeds the stringent requirements designed for the wide-field and supernova surveys for which the collaboration uses it.
Journal ArticleDOI

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

Philip S. Cowperthwaite, +99 more
TL;DR: In this article, the spectral energy distribution (SED) of the binary neutron star merger GW170817 was inferred from the optical and NIR spectrograms of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo.