Cross-Correlation Weak Lensing of Galaxy Clusters in the SDSS Southern Survey Coadd

Details Cross-Correlation Weak Lensing of Galaxy Clusters in the SDSS Southern Survey Coadd Cross-Correlation Weak Lensing of Galaxy Clusters in the SDSS Southern Survey Coadd

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543603k&link_type=abstract

American Astronomical Society, AAS Meeting #215, #436.03; Bulletin of the American Astronomical Society, Vol. 42, p.384

Astronomy and Astrophysics

Astronomy

Scientific paper

The SDSS Southern Survey is a 300 square degree region located on the celestial equator that has been repeatedly imaged as part of the SDSS I and II programs. These individual scans have been co-added to create an imaging survey which is roughly two magnitudes deeper than the main SDSS survey. We use this increase in imaging depth to study the weak lensing cross correlation signal between optically selected foreground galaxy clusters and distant background galaxies. This study will provide an important bridge between cluster cross-correlation weak lensing in the SDSS main survey and the forthcoming Dark Energy Survey.

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