activity
20152026
most citedMapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zel'dovich imaging

37 citations · 179 across the 33 of their papers we have counts for

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Showing 2023Show all

8 papers · 1 filter

astro-ph.CO2023

The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data

M. Muñoz-Echeverría, J. F. Macías-Pérez, G. W. Pratt +11

An accurate reconstruction of galaxy cluster masses is key to use this population of objects as a cosmological probe. In this work we present a study on the hydrostatic-to-lensing…

astro-ph.CO2023

CHEX-MATE: Characterization of the intra-cluster medium temperature distribution

L. Lovisari, S. Ettori, E. Rasia +23

We study the perturbations in the temperature (and density) distribution for 28 clusters selected from the CHEX-MATE sample to evaluate and characterize the level of inhomogeneitie…

astro-ph.CO2023

A radio bubble shredded by gas sloshing?

A. Botteon, F. Gastaldello, J. A. ZuHone +7

We report on the detection of diffuse radio emission with peculiar morphology in the central region of the galaxy cluster Abell 2657. The most striking feature identified in our 14…

astro-ph.CO2023

The NIKA2 Sunyaev-Zeldovich Large Program: Sample and upcoming product public release

L. Perotto, R. Adam, P. Ade +52

The NIKA2 camera operating at the IRAM 30 m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zeldovich effect towards galaxy clusters at intermediate and…

astro-ph.CO2023

Towards the first mean pressure profile estimate with the NIKA2 Sunyaev-Zeldovich Large Program

C. Hanser, R. Adam, P. Ade +51

High-resolution mapping of the hot gas in galaxy clusters is a key tool for cluster-based cosmological analyses. Taking advantage of the NIKA2 millimeter camera operated at the IRA…

astro-ph.CO2023

Systematic effects on the upcoming NIKA2 LPSZ scaling relation

A. Moyer-Anin, R. Adam, P. Ade +49

In cluster cosmology, cluster masses are the main parameter of interest. They are needed to constrain cosmological parameters through the cluster number count. As the mass is not a…