pith. sign in

arxiv: 1001.3521 · v1 · pith:SD4TJCLEnew · submitted 2010-01-20 · 🌌 astro-ph.CO

ARCRAIDER II: Arc search in a sample of non-Abell clusters

classification 🌌 astro-ph.CO
keywords clusterssamplepossiblearcraidergalaxiesredshiftsearchx-ray
0
0 comments X p. Extension
pith:SD4TJCLE Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{SD4TJCLE}

Prints a linked pith:SD4TJCLE badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We present a search for gravitational arcs in a sample of X-ray luminous, medium redshift clusters of galaxies. The sample of clusters is called ARCRAIDER, is based on the ROSAT Bright Survey (RBS) and fulfills the following criteria: (a) X-ray luminosity Lx>=0.5x10^45erg/s (0.5-2keV band), (b) redshift range 0.1<=z<=0.52, (c) classified as clusters in the RBS, (d) not a member of the Abell catalogue and, finally, (e) visible from the ESO sites La Silla/Paranal (declination \delta<=20deg). In total we found more than 35 (giant) arc/arclet candidates, including a possible radial arc, one galaxy-galaxy lensing event and a possible quasar triple image in 14 of the 21 clusters of galaxies. Hence 66% of the sample members are possible lenses.

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.