2005/11/03 by H. Hoekstra, Y. Mellier, L. van Waerbeke +6 · 5 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.1086/503249
published as Astrophys.J.647:116-127,2006 · Submitted to ApJ
arxiv created 2005/11/03 · openalex publication_date 2006/08/10 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31
We present the first measurements of the weak gravitational lensing signal induced by the large-scale mass distribution in the universe from data obtained as part of the ongoing Canada-France-Hawaii Telescope Legacy Survey (CFHTLS). The data used in this analysis are from the Wide Synoptic Survey, which aims to image ~170 deg 2 in five filters. We have analyzed an effective area of ~22 deg 2 (31 pointings) of i ' data spread over two of the three survey fields. These data are of excellent quality, and the results bode well for the remainder of the survey: we do not detect a significant " B " mode, suggesting that residual systematics are negligible at the current level of accuracy. Assuming a cold dark matter model and marginalizing over the Hubble parameter h ∈ [0.6, 0.8], the source redshift distribution, and systematics, we constrain σ 8 , the amplitude of the matter power spectrum. At a fiducial matter density Ω m = 0.3 we find σ 8 = 0.85 ± 0.06. This estimate is in excellent agreement with previous studies. A combination of our results with those from the Deep component of the CFHTLS enables us to place a constraint on a constant equation of state for the dark energy, based on cosmic shear data alone. We find that w 0 < -0.8 at 68% confidence.