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20212026
most citedMethodological refinement of the submillimeter galaxy magnification bias. II. Cosmological analysis with tomography

6 citations · 10 across the 15 of their papers we have counts for

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9 papers · 1 filter

astro-ph.GA2025

AtLAST -- A five fold increase in the number of identified Strongly Lensed Galaxies in the sub-millimetre and its consequences

Joaquín González-Nuevo, Laura Bonavera, Juan Alberto Cano +6

Strong gravitational lensing is a powerful probe of cosmology, dark matter (DM), and high-redshift galaxy evolution, but current samples of strongly lensed galaxies (SLGs) remain f…

astro-ph.CO2025

AtLAST -- Determination of Halo Mass Density Profiles at kpc Scales through Magnification Bias

Joaquín González-Nuevo, Laura Bonavera, Juan Alberto Cano +9

Magnification bias, the lensing-induced modification of background source number counts, provides a uniquely powerful probe of the mass density profiles of galaxies and clusters do…

astro-ph.CO2025

AtLAST -- Cosmology with submillimetre galaxies magnification bias

Laura Bonavera, Joaquin Gonzalez-Nuevo, Juan Alberto Cano +10

Magnification bias offers a uniquely powerful and independent route to cosmological information. As a gravitational-lensing observable, it probes galaxy-matter correlations without…

astro-ph.CO2025

Cosmic magnification on multi-catalogue Herschel submillimetre galaxies

R. Fernandez-Fernandez, M. M. Cueli, J. González-Nuevo +6

{Submillimetre galaxies (SMGs) are excellent background sources for magnification-bias studies, but the limited sky coverage in the submillimetre (sub-mm) band constrains their sta…

astro-ph.GA2025

Candidate gravitationally lensed submillimeter galaxies in Herschel-ATLAS associated with WISE elliptical counterparts

Juan Alberto Cano, Joaquín González-Nuevo, Laura Bonavera +5

We present a new and independent methodology for identifying gravitational lens candidates using data from the H-ATLAS and AllWISE surveys. Unlike previous approaches, which are ty…

astro-ph.GA2025

Spatial Variations of Polarized Synchrotron Emission in the QUIJOTE MFI Data using Neural Networks

J. M. Casas, L. Bonavera, J. González-Nuevo +7

Polarized synchrotron emission from ultra-relativistic electrons spiraling the Galactic magnetic field has become one of the most relevant emissions in the Interstellar medium thes…

astro-ph.GA2025

Spectral Properties of Anomalous Microwave Emission in 144 Galactic Clouds

Roke Cepeda-Arroita, J. A. Rubiño-Martín, R. T. Génova-Santos +23

Anomalous Microwave Emission (AME) is a diffuse microwave component thought to arise from spinning dust grains, yet remains poorly understood. We analyze AME in 144 Galactic clouds…

astro-ph.GA2025

The Einstein Gap: an unrecognised strong lensing feature in weak lensing mass density profiles

David Crespo, Joaquín González-Nuevo, Laura Bonavera +4

Magnification bias cross-correlations between galaxy clusters and high-redshift submillimetre galaxies have recently revealed a characteristic signal deficit at intermediate angula…

astro-ph.CO2025

Recovering the CMB signal with neural networks

J. M. Casas, L. Bonavera, J. González-Nuevo +2

Component separation is the process of extracting one or more emission sources in astrophysical maps. It is therefore crucial to develop models that can accurately clean the cosmic…