activity
20042014
most citedPhysical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9

96 citations · 257 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2014★ 8 cited

Constraining the mass-concentration relation through weak lensing peak function

Roberto Mainini, Anna Romano

Halo masses and concentrations have been studied extensively, by means of N-body simulations as well as observationally, during the last decade. Nevertheless, the exact form of the…

astro-ph.CO2012★ 22 cited

Weak lensing peak count as a probe of f(R) theories

V. F. Cardone, S. Camera, R. Mainini +4

Weak gravitational lensing by galaxy clusters on faint higher redshift galaxies has been traditionally used to study the cluster mass distribution and as a tool to identify cluster…

astro-ph.CO2011★ 15 cited

An X-ray underluminous cluster of galaxies in the 4Ms CDFS observations

M. Castellano, L. Pentericci, N. Menci +8

[Abridged] We use the large public spectroscopic database available in the GOODS-South field to estimate the dynamical mass and the virialization status of cluster ClG 0332-2747 at…

astro-ph.CO2011★ 23 cited

A weak lensing analysis of the Abell 383 cluster

Zhuoyi Huang, Mario Radovich, Aniello Grado +4

In this paper we use deep CFHT and SUBARU archival images of the Abell 383 cluster (z=0.187) to estimate its mass by weak lensing. To this end, we first use simulated imag…

astro-ph.CO2010★ 33 cited

Abell 611: I. weak lensing analysis with LBC

A. Romano, L. Fu, F. Giordano +24

Aims. The Large Binocular Cameras (LBC) are two twin wide field cameras (FOV ~ 23'x 25') mounted at the prime foci of the 8.4m Large Binocular Telescope (LBT). We performed a weak…

astro-ph.CO2010★ 30 cited

Abell 611. II. X-ray and strong lensing analyses

A. Donnarumma, S. Ettori, M. Meneghetti +10

We present the results of our analyses of the X-ray emission and of the strong lensing systems in the relaxed galaxy cluster Abell 611 (z=0.288). We infer the X-ray mass estimate d…