Searching for lensing by groups and clusters of galaxies
Paul M. Phillips, (NRAL)
The JVAS and CLASS searches for gravitational lens systems with image
separations between 0.3 and 6 arcsec hope to reveal
more than 20 new gravitational lens systems from a parent population of
>10000 flat spectrum radio sources. We have recently reanalysed this
data and have selected 17 candidate lens systems with image
separations in the range 6 to 15 arcsec. These
candidates are in the process of being followed up with multi-frequency
VLA observations. Whilst providing constraints on the prevalence of mass
structures associated with groups and small clusters of galaxies, this
search also covers the contentious angular scales involved in the `dark
lens'/binary quasar debate.
The ARCS project uses a parent sample selected from the FIRST survey to
look for lensing events on scales between 15 and
60 arcsec, which are associated with cluster-sized masses. The
sample was defined from extended radio
sources to eliminate questions of variability hampering multiple image
identification. A second stage of selection using stellar optical
counterparts from the APM catalogue provides a sample with high
mean redshift to increase lensing probability. The final parent sample
of approximately 1500 sources has yielded no lens systems. A detailed
analysis of the result is currently underway.
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