H-ATLAS/GAMA: magnification bias tomography. Astrophysical constraints above ∼1 arcmin

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H-ATLAS/GAMA: magnification bias tomography. Astrophysical constraints above ∼1 arcmin

An unambiguous manifestation of the magnification bias is the cross-correlation between two source samples with non-overlapping redshift distributions. In this work we measure and study the cross-correlation signal between a foreground sample of GAMA galaxies with spectroscopic redshifts in the rang...

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Bibliographic Details
Main Authors:	González-Nuevo, J., Lapi, A., Bonavera, L., Danese, L., de Zotti, G., Negrello, M., Bourne, N., Cooray, A., Dunne, L., Dye, S., Eales, S., Furlanetto, C., Ivison, R.J., Loveday, J., Maddox, S., Smith, M.W.L., Valiante, E.
Format:	Article
Published:	IOP Publishing 2017
Subjects:	galaxy clustering weak gravitational lensing gravitational lensing
Online Access:	https://eprints.nottingham.ac.uk/48825/

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