pith. sign in

arxiv: astro-ph/9801208 · v2 · submitted 1998-01-22 · 🌌 astro-ph

Weak Lensing by Two z~0.8 Clusters of Galaxies

classification 🌌 astro-ph
keywords clustergalaxiesclusterslensingweakbackgroundlightmapsmass
0
0 comments X
read the original abstract

We report the detection of weak gravitational lensing of distant background galaxies by two rich, X-ray luminous clusters of galaxies, MS 1137+66 at z=0.783 and RXJ 1716+67 at z=0.813. We detect a shear signal in each cluster over the radial range 100<r<700 h^-1 kpc. Assuming the background galaxies lie in a sheet at z=2, we measure a mass of 2.45*10^14 h^-1 Msolar and M/Lv = 270 at 500 h^-1 kpc radius for MS 1137+66, and a mass of 2.6*10^14 h^-1 Msolar and M/Lv = 190 for RXJ 1716+67 at the same radius. Both the optical lightmaps and weak lensing massmaps of RXJ 1716+67 show two spatially distinct sub-clusters, as well as a long filamentary structure extending out of the cluster to the northeast. In contrast, MS 1137+66 is an ultra-compact massive cluster in both massmaps and optical lightmaps, and contains a strongly-lensed arc system in the cluster core. These data add to the growing number of massive clusters at z>~0.8.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.