HerMES: Detection of cosmic magnification of submillimetre galaxies using angular cross-correlation

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 magnificati...

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Bibliographic Details
Main Authors: Wang, L., Cooray, A., Farrah, D., Amblard, A., Auld, R., Bock, J., Brisbin, D., Burgarella, D., Chanial, P., Clements, D., Eales, S., Franceschini, A., Glenn, J., Gong, Y., Griffin, M., Heinis, S., Ibar, E., Ivison, R., Mortier, A., Oliver, S., Page, M., Papageorgiou, A., Pearson, C., Pérez-Fournon, I., Pohlen, M., Rawlings, J., Raymond, G., Rodighiero, G., Roseboom, I., Rowan-Robinson, M., Scott, D., Serra, P., Seymour, Nick, Smith, A., Symeonidis, M., Tugwell, K., Vaccari, M., Vieira, J., Vigroux, L., Wright, G.
Format: Journal Article
Published: 2011
Online Access:http://hdl.handle.net/20.500.11937/14028

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