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19952026
most citedDark Matter Substructure in Galactic Halos

3k citations · 15.7k across the 170 of their papers we have counts for

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Showing 2014Show all

7 papers · 1 filter

astro-ph.CO2014

The SKA view of cool-core clusters: evolution of radio mini-halos and AGN feedback

Myriam Gitti, Paolo Tozzi, Gianfranco Brunetti +10

In about 70% of the population of relaxed, cool-core galaxy clusters, the brightest cluster galaxy (BCG) is radio loud, showing non-thermal radio jets and lobes ejected by the cent…

astro-ph.CO2014★ 50 cited

Chandra deep observation of XDCP J0044.0-2033, a massive galaxy cluster at z>1.5

P. Tozzi, J. S. Santos, M. J. Jee +11

We report the analysis of the Chandra observation of XDCP J0044.0-2033, a massive, distant (z=1.579) galaxy cluster discovered in the XDCP survey. The total exposure time of 380 ks…

astro-ph.GA2014★ 77 cited

The reversal of the SF-density relation in a massive, X-ray selected galaxy cluster at z=1.58: results from Herschel

Joana S. Santos, . Bruno Altieri, Ivan Valtchanov +8

Dusty, star-forming galaxies have a critical role in the formation and evolution of massive galaxies in the Universe. Using deep far-infrared imaging in the range 100-500um obtaine…

astro-ph.GA2014★ 23 cited

On the Fe abundance peak formation in cool-core clusters of galaxies: hints from cluster WARPJ1415.1+3612 at z=1.03

Sabrina De Grandi, Joana S. Santos, Mario Nonino +5

We present a detailed study of the iron content of the core of the high-redshift cluster WARPJ1415.1+3612 (z=1.03). By comparing the central Fe mass excess observed in this system,…

astro-ph.CO2014★ 6 cited

The Swift X-ray Telescope Cluster Survey II. X-ray spectral analysis

P. Tozzi, A. Moretti, E. Tundo +7

(Abridged) We present a spectral analysis of a new, flux-limited sample of 72 X-ray selected clusters of galaxies identified with the X-ray Telescope (XRT) on board the Swift satel…

astro-ph.CO2014★ 89 cited

Intra Cluster Light properties in the CLASH-VLT cluster MACS J1206.2-0847

V. Presotto, M. Girardi, M. Nonino +46

We aim at constraining the assembly history of clusters by studying the intra cluster light (ICL) properties, estimating its contribution to the fraction of baryons in stars, f*, a…