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Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
D. Crespo, J. González-Nuevo, L. Bonavera +3
In this work, we want to exploit the magnification bias of the SMGs using two different foreground samples, quasi-stellar objects (QSOs) and galaxies. Our aim is to study and compa…
Selecting a complete sample of blazars in sub-millimetre catalogues
M. Massardi, M. Bonato, M. Lopez-Caniego +6
The \textit{Herschel} Astrophysical Terahertz Large Area Survey (H-ATLAS), that has covered about 642 sq. deg. in 5 bands from 100 to 500 , allows a blind flux-limited sele…
CENN: A fully convolutional neural network for CMB recovery in realistic microwave sky simulations
J. M. Casas, L. Bonavera, J. González-Nuevo +7
Component separation is the process with which emission sources in astrophysical maps are generally extracted by taking multi-frequency information into account. It is crucial to d…
Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
M. M. Cueli, L. Bonavera, J. Gonzalez-Nuevo +3
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 s…