activity
20002003
most citedAn estimate of Ω_m without priors

85 citations · 246 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph2003★ 23 cited

Addendum to "Coherent radio pulses from GEANT generated electromagnetic showers in ice"

S. Razzaque, S. Seunarine, S. Chambers +4

We reevaluate our published calculations of electromagnetic showers generated by GEANT 3.21 and the radio frequency pulses they produce in ice. We are prompted by a recent report s…

astro-ph2003★ 85 cited

An estimate of Ω_m without priors

Hume A. Feldman, Roman Juszkiewicz, Pedro Ferreira +10

Using mean relative peculiar velocity measurements for pairs of galaxies, we estimate the cosmological density parameter and the amplitude of density fluctuations . Our…

astro-ph2003★ 11 cited

Optimal Moments for the Analysis of Peculiar Velocity Surveys II: Testing

Hume A. Feldman, Richard Watkins, Adrian L. Melott +1

Analyses of peculiar velocity surveys face several challenges, including low signal--to--noise in individual velocity measurements and the presence of small--scale, nonlinear flows…

astro-ph2001★ 38 cited

Coherent Radio Pulses From GEANT Generated Electromagnetic Showers In Ice

Soebur Razzaque, Surujhdeo Seunarine, David Z. Besson +3

Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-high energy particles of 1 PeV and above. Showers occuring in Antarctic ice shou…

astro-ph2001★ 14 cited

Optimal Moments for the Analysis of Peculiar Velocity Surveys

Richard Watkins, Hume A. Feldman, Scott W. Chambers +2

We present a new method for the analysis of peculiar velocity surveys which removes contributions to velocities from small scale, nonlinear velocity modes while retaining informati…

astro-ph2001★ 22 cited

Recent Dynamical Relaxation of Galaxy Clusters: Evidence for a Low- Universe

Adrian L. Melott, Scott W. Chambers, Christopher J. Miller

We argue that there has been substantial evolution in the ellipticity of rich galaxy clusters between 0 < z < 0.1, and suggest that this is additional evidence for a low matter-den…