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

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posted on 2023-06-09, 08:30 authored by J. Gonzalez-Nuevo, A. Lapi, L. Bonavera, L. Danese, G. de Zotti, M. Negrello, N. Bourne, A. Cooray, L. Dunne, S. Dye, S. Eales, C. Furlanetto, R. J. Ivison, Jonathan LovedayJonathan Loveday, S. Maddox, M. W. L. Smith, E. Valiante
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 range 0.2

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Publication status

  • Published

File Version

  • Accepted version

Journal

Journal of Cosmology and Astroparticle Physics

ISSN

1475-7516

Publisher

Institute of Physics

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Issue

24

Volume

2017

Department affiliated with

  • Physics and Astronomy Publications

Full text available

  • Yes

Peer reviewed?

  • Yes

Legacy Posted Date

2017-10-30

First Open Access (FOA) Date

2018-10-18

First Compliant Deposit (FCD) Date

2017-10-30

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