activity
20052009
most citedDetection of Gravitational Lensing in the Cosmic Microwave Background

374 citations · 446 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.CO200954 cited

Sharpening the Precision of the Sunyaev-Zel'dovich Power Spectrum

L. D. Shaw, O. Zahn, G. P. Holder +1

Using both halo model calculations and a large sample of simulated SZ maps, we demonstrate that high-mass clusters add significant non-Gaussian variance to measurements of the SZ p…

astro-ph.CO20094 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…

astro-ph.CO200913 cited

Strong gravitational lensing probes of the particle nature of dark matter

Leonidas A. Moustakas, Kevork Abazajian, Andrew Benson +44

There is a vast menagerie of plausible candidates for the constituents of dark matter, both within and beyond extensions of the Standard Model of particle physics. Each of these ca…

astro-ph.CO20091 cited

The Case for Deep, Wide-Field Cosmology

Ryan Scranton, Andreas Albrecht, Robert Caldwell +14

Much of the science case for the next generation of deep, wide-field optical/infrared surveys has been driven by the further study of dark energy. This is a laudable goal (and the…

astro-ph2007374 cited

Detection of Gravitational Lensing in the Cosmic Microwave Background

Kendrick M. Smith, Oliver Zahn, Olivier Dore

Gravitational lensing of the cosmic microwave background (CMB), a long-standing prediction of the standard cosmolgical model, is ultimately expected to be an important source of co…

astro-ph2005

The Cosmic Reionization History as Revealed by the CMB Doppler--21-cm Correlation

Marcelo A. Alvarez, Eiichiro Komatsu, Olivier Doré +1

We show that the epoch(s) of reionization when the ionization fraction of the universe is about half can be determined by correlating Cosmic Microwave Background (CMB) temperature…