collaborators

5 papers

astro-ph.CO2026

Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking

Xiaoyun Shao, Facundo Toscano, Diego Garcia Lambas +5

The Cosmic Microwave Background (CMB) reaches homogeneity at relatively modest angular scales compared to the expectation of the standard CDM model revealing an important chall…

astro-ph.CO2026

Evidence for a sign change of the ISW effect in the very recent universe? hot voids and cold overdensities at

Frode K. Hansen, Diego Garcia Lambas, Andrés N. Ruiz +2

We find a significant CMB temperature excess in the direction of local underdensities within . By contrast, less than of simulated CMB maps show a similarly signifi…

astro-ph.CO2026

Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges

Juan Ignacio Domínguez Feldman, Luis A. Pereyra, Frode K. Hansen +2

Recent papers have reported an unexplained cooling of CMB photons passing through galaxies in nearby cosmic filaments at the level. Here we show for the first time…

astro-ph.GA2026

The connection between surface brightness and satellite systems for central galaxies through Illustris TNG

Silvio Rodriguez, Yamila Yaryura, Jose A. Benavides +7

We analyse different properties of central low-surface-brightness galaxies (LSBGs) and their satellite systems using the simulation Illustris TNG-100, in order to deepen our unders…

astro-ph.CO2025

Quasar Pairs as Large--Scale Structure tracers

Martín G. Richarte, Facundo Toscano, Diego G. Lambas +3

Quasars are effective tracers of the large-scale distribution of galaxies at high redshift thanks to their high luminosity and dedicated surveys. Previous studies have shown that q…