activity
20102015
most citedThe sub-mJy radio sky in the Extended Chandra Deep Field South: source population

154 citations · 548 across the 9 of their papers we have counts for

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astro-ph.CO2013★ 154 cited

The sub-mJy radio sky in the Extended Chandra Deep Field South: source population

M. Bonzini, P. Padovani, V. Mainieri +5

The sub-mJy radio population is a mixture of active systems, that is star forming galaxies (SFGs) and active galactic nuclei (AGNs). We study a sample of 883 radio sources detected…

astro-ph.CO2013★ 130 cited

The VLA 1.4GHz Survey of the Extended Chandra Deep Field South: Second Data Release

N. A. Miller, M. Bonzini, E. B. Fomalont +6

Deep radio observations at 1.4GHz for the Extended Chandra Deep Field South were performed in June through September of 2007 and presented in a first data release (Miller et al. 20…

astro-ph.CO2012★ 47 cited

Spectrum of the unresolved cosmic X ray background: what is unresolved 50 years after its discovery

A. Moretti, S. Vattakunnel, P. Tozzi +5

We study the spectral properties of the unresolved cosmic X-ray background (CXRB) in the 1.5-7.0 keV energy band with the aim of providing an observational constraint on the statis…

astro-ph.CO2012★ 40 cited

The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification

M. Bonzini, V. Mainieri, P. Padovani +9

We study a sample of 883 sources detected in a deep Very Large Array survey at 1.4 GHz in the Extended Chandra Deep Field South. The paper focuses on the identification of their op…

astro-ph.CO2011★ 39 cited

The Radio - X-ray relation as a star formation indicator: Results from the VLA--E-CDFS Survey

S. Vattakunnel, P. Tozzi, F. Matteucci +10

In order to trace the instantaneous star formation rate at high redshift, and hence help understanding the relation between the different emission mechanisms related to star format…

astro-ph.CO2010★ 5 cited

Accretion and nuclear activity in Virgo early-type galaxies

Shaji Vattakunnel, Edoardo Trussoni, Alessandro Capetti +1

We use Chandra observations to estimate the accretion rate of hot gas onto the central supermassive black hole in four giant (of stellar mass 10E11 - 10E12 solar masses) early-type…