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The X-ray-Optical Relations for Nine Clusters at z = 0.7-1.1
Nick Rumbaugh, Dale D. Kocevski, Roy R. Gal +4
We use Chandra observations of nine optically and X-ray selected clusters in five different structures at z ~ 0.7-1.1 from the Observations of Redshift Evolution in Large-Scale Env…
Large Synoptic Survey Telescope: Dark Energy Science Collaboration
LSST Dark Energy Science Collaboration
This white paper describes the LSST Dark Energy Science Collaboration (DESC), whose goal is the study of dark energy and related topics in fundamental physics with data from the La…
Two accurate time-delay distances from strong lensing: Implications for cosmology
S. H. Suyu, M. W. Auger, S. Hilbert +9
Strong gravitational lenses with measured time delays between the multiple images and models of the lens mass distribution allow a one-step determination of the time-delay distance…
Submillimeter Observations of Millimeter Bright Galaxies Discovered by the South Pole Telescope
T. R. Greve, J. D. Vieira, A. Weiss +65
We present APEX SABOCA 350micron and LABOCA 870micron observations of 11 representative examples of the rare, extremely bright (S_1.4mm > 15mJy), dust-dominated millimeter-selected…
SHARP - I. A high-resolution multi-band view of the infra-red Einstein ring of JVAS B1938+666
D. J. Lagattuta, S. Vegetti, C. D. Fassnacht +3
We present new mass models for the gravitational lens system B1938+666, using multi-wavelength data acquired from Keck adaptive optics (AO) and Hubble Space Telescope (HST) observa…
Luminous Satellites II: Spatial Distribution, Luminosity Function and Cosmic Evolution
A. M. Nierenberg, M. W. Auger, T. Treu +3
We infer the normalization and the radial and angular distributions of the number density of satellites of massive galaxies () between redshifts 0.1…