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19922011
most citedEstimating the Power Spectrum of the Cosmic Microwave Background

431 citations · 1.4k across the 11 of their papers we have counts for

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10 papers · 1 filter

astro-ph2006★ 36 cited

Reduction of Cosmological Data for the Detection of Time-varying Dark Energy Density

Jason Dick, Lloyd Knox, Mike Chu

We present a method for reducing cosmological data to constraints on the amplitudes of modes of the dark energy density as a function of redshift. The modes are chosen so that (1)…

astro-ph2004★ 61 cited

Cosmological Parameter Constraints as Derived from the Wilkinson Microwave Anisotropy Probe Data via Gibbs Sampling and the Blackwell-Rao Estimator

M. Chu, H. K. Eriksen, L. Knox +5

We study the Blackwell-Rao (BR) estimator of the probability distribution of the angular power spectrum, P(C_l|d), by applying it to samples of full-sky no-noise CMB maps generated…

astro-ph2002★ 151 cited

Probing the Reionization History of the Universe using the Cosmic Microwave Background Polarization

M. Kaplinghat, M. Chu, Z. Haiman +3

The recent discovery of a Gunn--Peterson (GP) trough in the spectrum of the redshift 6.28 SDSS quasar has raised the tantalizing possibility that we have detected the reionization…

astro-ph2002★ 5 cited

Using Galaxy Cluster Peculiar Velocities to Constrain Cosmological Parameters

A. Peel, L. Knox

Galaxy cluster peculiar velocities can be inferred from high-sensitivity, high-resolution multiple-frequency observations in the 30 to 400 GHz range. While galaxy cluster counts an…

astro-ph2002★ 51 cited

Rapid Calculation of Theoretical CMB Angular Power Spectra

Manoj Kaplinghat, Lloyd Knox, Constantinos Skordis

We have developed a fast method for predicting the angular power spectrum, C_l, of the cosmic microwave background given cosmological parameters and a primordial power spectrum of…

astro-ph2000★ 145 cited

Annihilating Cold Dark Matter

M. Kaplinghat, L. Knox, M. S. Turner

Structure formation with cold dark matter (CDM) predicts halos with a central density cusp, which are observationally disfavored. If CDM particles have an annihilation cross sectio…