Weak lensing by large scale structure
Weak lensing by large scale structure
Weak lensing by large scale structure
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Cosmic shear is everywhere<br />
Credit: Tyson et al. (2000)<br />
Cosmic shear is the <strong>lensing</strong> of distant galaxies <strong>by</strong> the overall<br />
distribution of matter in the universe: it is the most “common”<br />
<strong>lensing</strong> phenomenon.