activity
20222025
most citedThe 700 ks Chandra Spiderweb Field II: Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxy

33 citations · 52 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2025

X-ray view of a massive node of the Cosmic Web at z=3 II. Discovery of extended X-ray emission around a hyperluminous QSO

Andrea Travascio, Sebastiano Cantalupo, Gabriele Pezzulli +17

While the warm, ionized gas in the CGM at z>3 is now routinely observed around bright QSOs in Lya emission, little is known about the CGM hot phase due to its expected faintness in…

astro-ph.CO2024★ 3 cited

Cooling rate and turbulence in the intracluster medium of the cool-core cluster Abell 2667

M. Lepore, C. Pinto, P. Tozzi +8

We present a detailed analysis of the thermal X-ray emission from the intracluster medium (ICM) in the cool-core galaxy cluster Abell 2667 (). Our goal is to detect low-tem…

astro-ph.GA2023★ 14 cited

Feeding and feedback processes in the Spiderweb proto-intracluster medium

M. Lepore, L. Di Mascolo, P. Tozzi +15

We present the detailed analysis of the thermal, diffuse emission of the proto-intracluster medium (ICM) detected in the halo of the Spiderweb Galaxy at z=2.16, within a radius of…

astro-ph.GA2022★ 2 cited

Mass assembly and AGN activity at in the dense environment of XDCPJ0044.0-2033

M. Lepore, A. Bongiorno, P. Tozzi +4

XDCP0044.0-2033 is the most massive galaxy cluster known at z>1.5 and its core shows a high density of galaxies which are experiencing mergers and hosting nuclear activity. We pres…

astro-ph.GA2022★ 33 cited

The 700 ks Chandra Spiderweb Field II: Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxy

P. Tozzi, R. Gilli, A. Liu +22

We present the X-ray imaging and spectral analysis of the diffuse emission around the Spiderweb galaxy at z=2.16 and of its nuclear emission, based on a deep (700 ks) Chandra obser…