Thursday, Jan 12, 2012, 9:00 AM - 2:00 PM
A Cosmic Shear Measurement from SDSS
Eric M. Huff
, T. Eifler
, C. M. Hirata
, R. Mandelbaum
, D. Schlegel
, U. Seljak
Center for Cosmology and AstroParticle Physics, The Ohio State University,
Department of Astrophysical Sciences, Princeton University,
Lawrence Berkeley National Laboratory,
Department of Astronomy, Department of Physics, UC Berkeley.
Weak lensing by large-scale structure is an invaluable cosmological tool in the era where most of the energy density of the concordance cosmology is invisible. Several large ground-based imaging surveys will attempt to measure this effect over the coming decade, but reliable control of the major systematic effects arising from atmospheric turbulence and telescope optics, shear miscalibration, intrinsic galaxy alignments, and photometric redshift inference remains a challenging problem.
We present a cosmic shear measurement using Sloan Digital Sky Survey imaging that addresses each of these challenges. We describe our procedure for lensing-optimized image coaddition, the results of careful modeling of each of the systematic errors, and the constraints our analysis puts on the concordance cosmology.
Austin Meeting Home
Abstract Submission Homepage
American Astronomical Society
2000 Florida Ave., NW
Washington, DC 20009
The Online Abstract Submission and Invitation System
© 1996 - 2013 Coe-Truman Technologies, Inc. All rights reserved.