Massive galaxy clusters lensing analyse (Richard+, 2010)

Details Massive galaxy clusters lensing analyse (Richard+, 2010) Massive galaxy clusters lensing analyse (Richard+, 2010)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74040325r&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/404/325. Originally published in: 2010MNRAS.404..325R

Physics

Clusters: Galaxy, Gravitational Lensing, Redshifts, Photometry: Hst

Scientific paper

High-resolution imaging data taken with the Advanced Camera for Surveys (ACS) or Wide Field Planetary Camera 2 (WFPC2) instrument on HST are available for each selected cluster in one or two bands, either through our dedicated LoCuSS programme (GO-DD 11312, PI: G.P. Smith) or from the archive.
J- and KS-band data were obtained between 2003 March and 2007 April on the following near-infrared instruments: Wide Infrared Camera (WIRC) on the Palomar-200-inch telescope, Infrared Side Port Imager (ISPI) on the CTIO Blanco 4-m telescope and Florida Infrared Imaging Multi-Object Spectrograph (FLAMINGOS) on the Kitt Peak (KPNO) 4-m telescope.
We used the LRIS on the Keck-I telescope to perform long-slit and multislit observations of the clusters. The spectroscopic data used in the current paper are the outcome of six different observing runs between 2004 and 2008.
(1 data file).

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