papers

Publications (12)

astro-ph.CO2012

Mass, shape and thermal properties of A1689 by a multi-wavelength X-ray, lensing and Sunyaev-Zel'dovich analysis

Mauro Sereno, Stefano Ettori, Keiichi Umetsu +1

Knowledge of mass and concentration of galaxy clusters is crucial to understand their formation and evolution. Unbiased estimates require the understanding of the shape and orienta…

astro-ph2005

Accretion and nuclear activity of quiescent supermassive black holes. I: X-ray study

Roberto Soria, Giuseppina Fabbiano, Alister W. Graham +5

We have studied the nuclear activity in a sample of six quiescent early-type galaxies, with new Chandra data and archival HST optical images. Their nuclear sources have X-ray lumin…

astro-ph.CO2017

Galaxy Cluster Pressure Profiles as Determined by Sunyaev Zel'dovich Effect Observations with MUSTANG and Bolocam II: Joint Analysis of Fourteen Clusters

Charles Romero, Brian Mason, Jack Sayers +13

We present pressure profiles of galaxy clusters determined from high resolution Sunyaev-Zel'dovich (SZ) effect observations of fourteen clusters, which span the redshift range $ 0.…

astro-ph2001

A study of the core of the Shapley Concentration: VI. Spectral properties of galaxies

Alessandro Baldi, Sandro Bardelli, Elena Zucca

We present the results of a study of the spectral properties of galaxies in the central part of the Shapley Concentration, covering an extremely wide range of densities, from the r…

astro-ph.CO2011

An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters

Alessandro Baldi, Stefano Ettori, Silvano Molendi +3

We present an XMM-Newton analysis of the X-ray spectra of 39 clusters of galaxies at 0.4<z<1.4, covering a temperature range of 1.5<=kT<=11 keV. We performed a spatially resolved s…

astro-ph.CO2012

Self-similarity of temperature profiles in distant galaxy clusters: the quest for a Universal law

Alessandro Baldi, Stefano Ettori, Silvano Molendi +1

We present the XMM-Newton temperature profiles of 12 bright clusters of galaxies at 0.4<z<0.9, with 5<kT<11 keV. The normalized temperature profiles (normalized by the mean tempera…