activity
19982014
most citedProbing the distribution of dark matter in the Abell 901/902 supercluster with weak lensing

111 citations · 346 across the 10 of their papers we have counts for

collaborators

10 papers

physics.class-ph2014★ 1 cited

Novel and Unique Expression for the Radiation Reaction Force, Relevance of Newton's Third Law and Tunneling

Dieter Gromes, Eduard Thommes

We derive the radiation reaction by taking into account that the acceleration of the charge is caused by the interaction with some heavy source particle. In the non relativistic ca…

astro-ph2007★ 28 cited

Narrow-band surveys for very high redshift Lyman-alpha emitters

Kim K. Nilsson, Alvaro Orsi, Cedric G. Lacey +2

Context: Many current and future surveys aim to detect the highest redshift (z >~ 7) sources through their Lyman-alpha (Ly-alpha) emission, using the narrow-band imaging method. Ho…

astro-ph2006★ 35 cited

Baryon Acoustic Oscillations and Dynamical Dark Energy

Michael Doran, Steffen Stern, Eduard Thommes

We compute the impact of dark energy at last scattering on measurements of baryon acoustic oscillations (BAOs). We show that an early dark energy component can contribute a systema…

astro-ph2005★ 42 cited

Intermediate-mass Black Hole and stellar orbits in the Galactic Center

Yuri Levin, Alice S. P. Wu, Edward W. Thommes

Many young stars reside within the central half-parsec from SgrA*, the supermassive black hole in the Galactic Center. The origin of these stars remains a puzzle. Recently, Hansen…

astro-ph2003

The expected abundance of Lyman- emitting primeval galaxies. I. General model predictions

E. Thommes, K. Meisenheimer

We present model calculations for the expected surface density of Ly- emitting primeval galaxies (PGs) at high redshifts. We assume that elliptical galaxies and bulges of spiral…

astro-ph2001★ 111 cited

Probing the distribution of dark matter in the Abell 901/902 supercluster with weak lensing

M. E. Gray, A. N. Taylor, K. Meisenheimer +3

We present a weak shear analysis of the Abell 901/902 supercluster, composed of three rich clusters at z=0.16. Using a deep R-band image from the 0.5 x 0.5 degree MPG/ESO Wide Fiel…