collaborators

10 papers

astro-ph.GA2026

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…

gr-qc2026

Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data

Daniel Lanchares, Osvaldo G. Freitas, Lysiane Mornas +4

The speed-up of parameter estimation is an active field of research in gravitational-wave data analysis. In this paper we present GP15, a deep-learning method that merges residual…

astro-ph.GA2026

Breathless BEARS: [O] 88m Emission of Dusty Star-Forming Galaxies at

T. J. L. C. Bakx, Hiddo S. B. Algera, Prachi Prajapati +13

We present [O] 88m observations towards four -selected dusty star-forming galaxies (DSFGs; log L/L = 13.5 - 14 at…

astro-ph.GA2025

Surveying Galaxy Clusters (in formation) in the Distant Universe

J. M. Pérez-Martínez, H. Dannerbauer, E. van Kampen +8

Present-day galaxy clusters are the largest virialized structures in the Universe, yet their early assembly remains poorly understood. At z2, clusters in formation span tens of…

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…