activity
19942023
most citedThe VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6

353 citations · 8.2k across the 93 of their papers we have counts for

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32 papers · 1 filter

astro-ph2008

Large Scale Structures at High Redshift in the GOODS Field

M. Castellano, S. Salimbeni, D. Trevese +8

We present a catalogue of overdensities in the GOODS-South field. We find various high density peaks that are embedded in structures diffused on the entire field, up to z ~ 2.5. Th…

astro-ph2007

The evolution of the mass-metallicity relation at z~3

R. Maiolino, T. Nagao, A. Grazian +14

We present preliminary results of an ESO-VLT large programme (AMAZE) aimed at determining the evolution of the mass-metallicity relation at z~3 by means of deep near-IR spectroscop…

astro-ph2007★ 1 cited

A near-ultraviolet view of the Inner Region of M31 with the Large Binocular Telescope

G. Beccari, M. Bellazzini, G. Clementini +27

We present a 900 sec, wide-field U image of the inner region of the Andromeda galaxy obtained during the commissioning of the blue channel of the Large Binocular Camera mounted on…

astro-ph2007★ 236 cited

Unveiling obscured accretion in the Chandra Deep Field South

F. Fiore, A. Grazian, P. Santini +10

A large population of heavily obscured, Compton Thick AGNs is predicted by models of galaxy formation, models of Cosmic X-ray Background and by the ``relic'' super-massive black-ho…

astro-ph2007★ 46 cited

ConvPhot: A Profile-Matching Algorithm for Precision Photometry

C. De Santis, A. Grazian, A. Fontana +1

We describe in this paper a new, public software for accurate "PSF-matched" multiband photometry for images of different resolution and depth, that we have named ConvPhot, of which…

astro-ph2006★ 147 cited

The Abundance of Distant and Extremely Red Galaxies: The Role of AGN Feedback in Hierarchical Models

N. Menci, A. Fontana, E. Giallongo +2

We investigate the effect of AGN feedback associated to the bright QSO phase onto the color distribution of galaxies from z=0 up to z=4. To this aim, we insert a blast-wave model o…