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H-ATLAS/GAMA: magnification bias tomography. Astrophysical constraints above ~1 arcmin
journal contribution
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. ValianteAn 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
History
Publication status
- Published
File Version
- Accepted version
Journal
Journal of Cosmology and Astroparticle PhysicsISSN
1475-7516Publisher
Institute of PhysicsExternal DOI
Issue
24Volume
2017Department affiliated with
- Physics and Astronomy Publications
Full text available
- Yes
Peer reviewed?
- Yes
Legacy Posted Date
2017-10-30First Open Access (FOA) Date
2018-10-18First Compliant Deposit (FCD) Date
2017-10-30Usage metrics
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