HerMES: detection of cosmic magnification of submillimetre galaxies using angular cross-correlation
Cosmic magnification is due to the weak gravitational lensing of sources in the distant Universe by foreground large-scale structure leading to coherent changes in the observed number density of the background sources. Depending on the slope of the background source number counts, cosmic magnification causes a correlation between the background and
Wang, L. et al.
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2011