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19992021
most citedA Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400

407 citations · 1.1k across the 18 of their papers we have counts for

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astro-ph2007★ 279 cited

Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures

Marilena LoVerde, Amber Miller, Sarah Shandera +1

The detection of primordial non-Gaussianity could provide a powerful means to test various inflationary scenarios. Although scale-invariant non-Gaussianity (often described by the…

astro-ph2005★ 20 cited

An empirical model for the polarization of pulsar radio emission

D. Melrose, A. Miller, A. Karastergiou +1

We present an empirical model for single pulses of radio emission from pulsars based on gaussian probability distributions for relevant variables. The radiation at a specific pulse…

astro-ph2005★ 79 cited

The EBEX Experiment

P. Oxley, P. Ade, C. Baccigalupi +15

EBEX is a balloon-borne polarimeter designed to measure the intensity and polarization of the cosmic microwave background radiation. The measurements would probe the inflationary e…

astro-ph2002★ 56 cited

Measurement of Arcminute Scale Anisotropy with the BIMA Array

K. S. Dawson, W. L. Holzapfel, J. E. Carlstrom +4

We report the results of our continued study of arcminute scale anisotropy in the Cosmic Microwave Background (CMB) with the Berkeley-Illinois-Maryland Array. The survey consists o…

astro-ph2001

The CMB - Contemporary Measurements and Cosmology

A. D. Miller

Since the discovery of the Cosmic Microwave Background (CMB) in 1965, characterization of the CMB anisotropy angular power spectrum has become somewhat of a holy grail for experime…

astro-ph1999★ 407 cited

A Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400

A. D. Miller, R. Caldwell, M. J. Devlin +7

We report on a measurement of the angular spectrum of the CMB between and made at 144 GHz from Cerro Toco in the Chilean altiplano. When the new data…