Antonio Ferragamo | Ricerc@Sapienza

Pubblicazioni

Titolo	Pubblicato in	Anno
Galaxy cluster mass bias from projected mass maps	ASTRONOMY & ASTROPHYSICS	2024
The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data	ASTRONOMY & ASTROPHYSICS	2024
The three hundred project: mapping the matter distribution in galaxy clusters via deep learning from multiview simulated observations	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY	2024
Impact of filaments on galaxy cluster properties in The Three Hundred simulation	EPJ WEB OF CONFERENCES	2024
The three hundred. Contrasting cluster galaxy density in hydrodynamical and dark matter simulations	ASTRONOMY & ASTROPHYSICS	2024
A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps with THE THREE HUNDRED clusters	EPJ WEB OF CONFERENCES	2024
Generating galaxy clusters mass density maps from mock multiview images via deep learning	EPJ WEB OF CONFERENCES	2024
Towards the first mean pressure profile estimate with the NIKA2 Sunyaev-Zeldovich Large Program	EPJ WEB OF CONFERENCES	2024
Impact of filaments on galaxy cluster properties in THE THREE HUNDRED simulation	EPJ WEB OF CONFERENCES	2024
Galaxy clusters morphology with Zernike polynomials: the first application on Planck Compton parameter maps	EPJ WEB OF CONFERENCES	2024
3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples	EPJ WEB OF CONFERENCES	2024
THE THREE HUNDRED project: Contrasting clusters optical and IR properties in hydrodynamical and dark matter only simulations	EPJ WEB OF CONFERENCES	2024
The NIKA2 Sunyaev-Zeldovich Large Program Sample and upcoming product public release	EPJ WEB OF CONFERENCES	2024
Estimation of the hydrostatic-to-lensing mass bias from resolved cluster masses	EPJ WEB OF CONFERENCES	2024
THE THREE HUNDRED project: Estimating the dependence of gas filaments on the mass of galaxy clusters	ASTRONOMY & ASTROPHYSICS	2024
The three hundred project. A machine learning method to infer clusters of galaxy mass radial profiles from mock Sunyaev–Zel’dovich maps	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY	2023
Multi-probe analysis of the galaxy cluster CL J1226.9+3332: Hydrostatic mass and hydrostatic-To-lensing bias	ASTRONOMY & ASTROPHYSICS	2023
CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles	ASTRONOMY & ASTROPHYSICS	2023
CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles	ASTRONOMY & ASTROPHYSICS	2023
PSZ2 G091: A massive double cluster at z ~ 0.822 observed by the NIKA2 camera	EPJ WEB OF CONFERENCES	2022