Chandra and HST Observations of the Brightest Cluster Lenses

Details Chandra and HST Observations of the Brightest Cluster Lenses Chandra and HST Observations of the Brightest Cluster Lenses

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8882a&link_type=abstract

HST Proposal ID #8882

Physics

Hst Proposal Id #8882

Scientific paper

We propose Chandra and Hubble Space Telescope observations of the four X-ray brightest, cooling-flow clusters with bright gravitational arcs, newly identified from the ROSAT XBACS/BCS lensing study. Our primary aim is to measure the cluster mass profiles, using both the X-ray and lensing data. Secondary goals include measurements of the X-ray gas/total mass ratio as a function of radius, and the properties and ages of the cooling flows. Our targets are the X-ray brightest, dynamically-relaxed lensing clusters not yet studied with Chandra or HST and are amongst the most massive and X-ray luminous clusters known.

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