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20242026
most citedModel-Independent Dark Energy Measurements from DESI DR2 and Planck 2015 Data

6 citations · 10 across the 7 of their papers we have counts for

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astro-ph.CO2026

Towards precision cosmology with Void x CMB correlations (II): Impact of mock catalogs on the Void x CMB lensing signal

Mar Pérez Sar, Carlos Hernández Monteagudo, András Kovács +2

Gravitational lensing by large-scale structure imprints secondary anisotropies on the Cosmic Microwave Background (CMB) that can be exploited to probe cosmology. In particular, cos…

astro-ph.CO2026

Lossless Compression of Cosmological Information from Type Ia Supernova Distance Measurements

Zhenyuan Wang, Yun Wang

We perform model-independent distance measurements on four Type Ia supernovae (SNe Ia) compilations (Pantheon, Pantheon+, DES-Dovekie, Union3) and compress each dataset into the va…

astro-ph.CO2026

Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy

Zhenyuan Wang, Yun Wang

Recent analyses combining DESI DR2 BAO with CMB and SNe Ia data have reported -- evidence for dynamical dark energy, but the significance depends strongly on the superno…

astro-ph.CO2025

Clustering analysis of BOSS-CMASS galaxies with semi-analytical model for galaxy formation and halo occupation distribution

Zhongxu Zhai, Andrew Benson, Yun Wang

The spatial distribution of massive and luminous galaxies have provided important constraints on the fundamental cosmological parameters and physical processes governing galaxy for…

astro-ph.CO2025★ 6 cited

Model-Independent Dark Energy Measurements from DESI DR2 and Planck 2015 Data

Yun Wang, Katherine Freese

Using DESI DR2 baryon acoustic oscillation (BAO) distance measurements and Planck cosmic microwave background distance priors, we have measured the dark energy density and…

astro-ph.CO2024★ 4 cited

Cosmology with voids from the Nancy Grace Roman Space Telescope

Giovanni Verza, Giulia Degni, Alice Pisani +7

We provide an accurate forecast of the expected constraining power from the main void statistics -- the void size function and the void-galaxy cross-correlation function -- to be m…