most citedCosmic voids: a novel probe to shed light on our Universe

48 citations · 48 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2019

Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background

P. Vielzeuf, A. Kovács, U. Demirbozan +62

Cosmic voids gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint on degree scales. We use the simulated CMB lensing convergence ma…

astro-ph.CO2019

Dark Energy Survey Year 1 results: The relationship between mass and light around cosmic voids

Y. Fang, N. Hamaus, B. Jain +74

What are the mass and galaxy profiles of cosmic voids? In this paper we use two methods to extract voids in the Dark Energy Survey (DES) Year 1 redMaGiC galaxy sample to address th…

astro-ph.CO2019

The bias of cosmic voids in the presence of massive neutrinos

Nico Schuster, Nico Hamaus, Alice Pisani +4

Cosmic voids offer an extraordinary opportunity to study the effects of massive neutrinos on cosmological scales. Because they are freely streaming, neutrinos can penetrate the int…

astro-ph.CO201948 cited

Cosmic voids: a novel probe to shed light on our Universe

Alice Pisani, Elena Massara, David N. Spergel +26

Cosmic voids, the less dense patches of the Universe, are promising laboratories to extract cosmological information. Thanks to their unique low density character, voids are extrem…

astro-ph.CO2018

On the relative bias of void tracers in the Dark Energy Survey

G. Pollina, N. Hamaus, K. Paech +61

Luminous tracers of large-scale structure are not entirely representative of the distribution of mass in our Universe. As they arise from the highest peaks in the matter density fi…

astro-ph.CO2018

Dark Energy Survey Year 1 Results: Weak Lensing Mass Calibration of redMaPPer Galaxy Clusters

T. McClintock, T. N. Varga, D. Gruen +99

We constrain the mass--richness scaling relation of redMaPPer galaxy clusters identified in the Dark Energy Survey Year 1 data using weak gravitational lensing. We split clusters i…