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

Cosmic homogeneity: the effect of redshift-space distortions and bias and cosmological constraints

Xiaoyun Shao, Rodrigo Gonçalves, Carlos A. P. Bengaly +2

We present a novel cosmological analysis based on the angular correlation dimension curve, a cumulative statistic derived from the two-point correlation function. Unlike trad…

astro-ph.CO2026

Measurements of the Angular Homogeneity Scale from DESI DR1

Mariana Lopes-Dias, Carlos A. P. Bengaly, Xiaoyun Shao +4

The study of the large-scale distribution of galaxies provides essential information for testing the standard cosmological model, namely the CDM paradigm. This scenario is base…

astro-ph.CO2026

Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae

Xiaoyun Shao, Carlos A. P. Bengaly

According to the perturbed Friedmann model, the difference between Hubble constant measurements in two rest frames, at leading order in velocity, is determined solely by the relati…

astro-ph.CO2025

Cosmological constraints from angular homogeneity scale measurements

Xiaoyun Shao, Carlos A. P. Bengaly, Rodrigo S. Gonçalves +2

In this paper, we obtain new measurements of the angular homogeneity scale () from the BOSS DR12 and eBOSS DR16 catalogs of Luminous Red Galaxies of the Sloan Digital Sky Sur…