Context. Gravitational lensing is a powerful tool for studying the distribution of mass in the
Universe. Understanding the magnification bias effect in gravitational lensing and its impact …

Aims. The main goal of this paper is to derive observational constraints on the halo mass
fuction (HMF) by performing a tomographic analysis of the magnification bias signal on a …

Context. High-z submillimetre galaxies can be used as a background sample for
gravitational lensing studies thanks to their magnification bias. In particular, the …

We report the ALMA Band 7 observations of 86 Herschel sources that likely contain
gravitationally lensed galaxies. These sources are selected with relatively faint 500 μ m flux …

Aims. The main purpose of this work is to provide a proof-of-concept method to derive
tabulated observational constraints on the halo mass function (HMF) by studying the …

Context. The magnification bias on the submillimetre galaxies (SMGs) is a gravitational
lensing effect, where the SMGs are used as background lensed galaxies. This effect can be …

Context. The study of the magnification bias produced on high-redshift sub-millimetre
galaxies by foreground galaxies through the analysis of the cross-correlation function was …

Context. This work focuses on the submillimeter galaxy magnification bias, specifically in the
tomographic scenario. It builds upon previous works, while utilising updated data to refine …

Context. As recently demonstrated, high-z submillimetre galaxies (SMGs) are the perfect
background sample for tracing the mass density profiles of galaxies and clusters (baryonic …

Context. The magnification bias is a gravitational lensing effect that produces an increase or
decrease in the detection probability of background sources near the position of a lense …