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.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…

astro-ph.CO2025

Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?

Facundo Toscano, Frode K. Hansen, Diego Garcia Lambas +3

We perform cosmological parameters estimation on Planck Cosmic Microwave Background (CMB) maps masking the recently discovered foreground related to nearby spiral galaxies. In addi…

astro-ph.CO2025

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter

Frode K. Hansen, Diego Garcia Lambas, Heliana E. Luparello +2

We confirm at the level previous studies reporting Cosmic Microwave Background (CMB) temperatures being significantly lower around nearby spiral galaxies than expected in t…