activity
19972023
most citedExtreme Ultraviolet Emission from Clusters of Galaxies: Inverse Compton Radiation from a Relic Population of Cosmic Ray Electrons?

101 citations · 826 across the 67 of their papers we have counts for

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Showing 2004Show all

6 papers · 1 filter

astro-ph2004★ 13 cited

On the absence of gravitational lensing of the cosmic microwave background

Richard Lieu, Jonathan P. D. Mittaz

The magnification of distant sources by mass clumps at lower () redshifts is calculated analytically. The clumps are initially assumed to be galaxy group isothermal spher…

astro-ph2004★ 50 cited

Average magnification effect of clumping of matter

T. W. B. Kibble, Richard Lieu

The aim of this paper is to re-examine the question of the average magnification in a universe with some inhomogeneously distributed matter. We present an analytic proof, valid und…

astro-ph2004

WHIM emission and the cluster soft excess: a model comparison

J. Mittaz, R. Lieu, R. Cen +1

The confirmation of the cluster soft excess (CSE) by XMM-Newton has rekindled interest as to its origin. The recent detections of CSE emission at large cluster radii together with…

astro-ph2004★ 1 cited

Proving the conservation of surface brightness during the strong and weak lensing of light by an isothermal sphere

Richard Lieu

An analytical proof of the conservation of surface brightness during the strong and weak lensing of light by a singular isothermal sphere is provided. It is shown that the movement…

astro-ph2004★ 6 cited

Are the WMAP angular magnification measurements consistent with an inhomogeneous critical density Universe?

R. Lieu, J. P. D. Mittaz

The propagation of light through a Universe of (a) isothermal mass spheres amidst (b) a homogeneous matter component, is considered. We demonstrate by an analytical proof that as l…

astro-ph2004★ 1 cited

Warm gas in the outskirts of galaxy clusters -- The cluster soft excess phenomenon

M. Bonamente, R. Lieu, J. P. D. Mittaz

The cluster soft excess emission indicates the presence of large amounts of warm gas (T ~ 10^6 K) in the neighborhood of galaxy clusters. Among the clusters that display this pheno…