activity
20012026
most citedA genetic algorithm for the non-parametric inversion of strong lensing systems

126 citations · 979 across the 31 of their papers we have counts for

collaborators
Showing 2008Show all

7 papers · 1 filter

astro-ph2008★ 43 cited

Hubble Space Telescope Survey of the Perseus Cluster: II. Photometric scaling relations in different environments

S. De Rijcke, S. Penny, C. Conselice +2

We investigate the global photometric scaling relations traced by early-type galaxies in different environments, ranging from dwarf spheroidals, over dwarf elliptical galaxies, up…

astro-ph2008★ 59 cited

Hubble Space Telescope survey of the Perseus Cluster - I: The structure and dark matter content of cluster dwarf spheroidals

S. Penny, C. Conselice, S. De Rijcke +1

We present the results of a Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) study of dwarf galaxies in the core of the rich nearby Perseus Cluster, down to M_V=-12.…

astro-ph2008★ 17 cited

Sigma-drop in galaxies and the sigma-metallicity degeneracy

Mina Koleva, Philippe Prugniel, Sven De Rijcke

In some galaxies, the central velocity dispersion, sigma, is depressed with respect to the surroundings. This sigma-drop phenomenon may have different physical origins, bearing inf…

astro-ph2008★ 83 cited

Simulations of the formation and evolution of isolated dwarf galaxies

Sander Valcke, S. De Rijcke, H. Dejonghe

We present new fully self-consistent models of the formation and evolution of isolated dwarf galaxies. We have used the publicly available N-body/SPH code HYDRA, to which we have a…

astro-ph2008★ 40 cited

Non-parametric strong lens inversion of Cl~0024+1654: illustrating the monopole degeneracy

J. Liesenborgs, S. De Rijcke, H. Dejonghe +1

The cluster lens Cl 0024+1654 is undoubtedly one of the most beautiful examples of strong gravitational lensing, providing five large images of a single source with well-resolved s…

astro-ph2008★ 19 cited

Global m=1 instabilities and lopsidedness in disc galaxies

Vanessa Dury, S. De Rijcke, Victor P. Debattista +1

Lopsidedness is common in spiral galaxies. Often, there is no obvious external cause, such as an interaction with a nearby galaxy, for such features. Alternatively, the lopsidednes…