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...

Full description

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

Internet

http://hdl.handle.net/20.500.11937/14028

Similar Items