activity
19952007
most citedCombining Strong and Weak Gravitational Lensing in Abell 1689

304 citations · 865 across the 9 of their papers we have counts for

collaborators
Showing 1999Show all

6 papers · 1 filter

astro-ph1999

The X-ray Morphology of the Lensing Galaxy Cluster Cl0024+17

H. Böhringer, G. Soucail, Y. Mellier +2

The paper reports the analysis of a very deep ROSAT HRI observation of the distant lensing cluster, CL0024+17. The morphology of the cluster is studied and the small core radius in…

astro-ph1999

An ISOCAM Mid-IR Survey through Gravitationally Lensing Galaxy Clusters

A. Biviano, L. Metcalfe, B. Altieri +10

We present imaging results and source counts from a deep ISOCAM cosmological survey at 15 microns, through gravitationally lensing galaxy clusters. We take advantage of the cluster…

astro-ph1999

Depletion curves of galaxy number counts behind cluster lenses

C. Mayen, G. Soucail

When the logarithmic slope of the galaxy counts is lower than 0.4 (this is the case in all filters at high magnitude), the magnification bias due to the lens makes the number densi…

astro-ph1999

A Wide-Field Spectroscopic Survey In The Cluster Lens Cl0024+17

Oliver Czoske, Genevieve Soucail, Jean-Paul Kneib +3

We present a detailed velocity histogram from a wide-field spectroscopic survey in the field of the cluster lens Cl0024 showing an unrelaxed foreground structure in addition to the…

astro-ph1999

Lensed galaxies in Abell 370 II. The ultraviolet properties of arclets and the star formation rate at high redshift

J. Bezecourt, G. Soucail, R. S. Ellis +1

We discuss the statistical properties of faint background galaxies detected in a deep Hubble Space Telescope ultraviolet (F336W) Wide Field Planetary Camera 2 image of the lensing…

astro-ph1999

Emission-Line Properties of MG2016+112: A Luminous Type-2 Quasar at High Redshift

T. Yamada, S. Yamazaki, M. Hattori +2

We present new high signal-to-noise ratio spectra of the components B and C of the gravitational lensing system MG2016+112. We show that image C displays strong emission lines of L…