activity
20222026
most citedThe stratification of ISM properties in the edge-on galaxy NGC 891 revealed by NIKA2

12 citations · 17 across the 9 of their papers we have counts for

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9 papers · 1 filter

astro-ph.CO20242 cited

Exploiting the high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116

A. Paliwal, M. De Petris, A. Ferragamo +54

Having a detailed knowledge of the intracluster medium (ICM) to infer the exact cluster physics such as the cluster dynamical state is crucial for cluster-based cosmological studie…

astro-ph.CO2024

Toward the first cosmological results of the NIKA2 Sunyaev-Zeldovich Large Program: The SZ-Mass scaling relation

A. Moyer-Anin, R. Adam, P. Ade +53

In Sunyaev-Zeldovich (SZ) cluster cosmology, two tools are needed to be able to exploit data from large scale surveys in the millimeter-wave domain. An accurate description of the…

astro-ph.CO2023

NIKA2 observations of 3 low-mass galaxy clusters at : pressure profile and - relation

R. Adam, M. Ricci, D. Eckert +64

Three galaxy clusters selected from the XXL X-ray survey at high redshift and low mass ( and M) were observed with NIKA2 to imag…

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…