activity
20062008
most citedThe Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies

415 citations · 1.2k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph200882 cited

The physical properties of Lyalpha emitting galaxies: not just primeval galaxies?

L. Pentericci, A. Grazian, A. Fontana +4

We have analyzed a sample of LBGs from z =3.5 to z=6 selected from the GOODS-S field as B,V and i-dropouts, and with spectroscopic observations showing that they have the Lyalpha l…

astro-ph200820 cited

[OIII] emitters in the field of the MRC 0316-257 protocluster

F. Maschietto, N. A. Hatch, B. P. Venemans +12

Venemans et al. (2005) found evidence for an overdensity of Ly-alpha emission line galaxies associated with the radio galaxy MRC 0316-257 at z=3.13 indicating the presence of a mas…

astro-ph200877 cited

A BLR origin for the iron K line in NGC7213

Stefano Bianchi, Fabio La Franca, Giorgio Matt +5

The X-ray spectrum of NGC7213 is known to present no evidence for Compton reflection, a unique result among bright Seyfert 1s. The observed neutral iron K line, therefore, canno…

astro-ph200874 cited

The Nascent Red Sequence at z~2

Andrew W. Zirm, S. A. Stanford, M. Postman +12

We present new constraints on the evolution of the early-type galaxy color-magnitude relation (CMR) based on deep near-infrared imaging of a galaxy protocluster at z=2.16 obtained…

astro-ph200775 cited

Physical properties of z~4 LBGs: differences between galaxies with and without Ly-alpha emission

L. Pentericci, A. Grazian, A. Fontana +5

We have analysed the physical properties of z~4 Lyman Break Galaxies observed in the GOODS-S survey, in order to investigate the possible differences between galaxies where the Ly-…

astro-ph200798 cited

A comparison among LBGs, DRGs and BzK galaxies: their contribution to the stellar mass density in the GOODS-MUSIC sample

A. Grazian, ; S. Salimbeni, ; L. Pentericci +8

The classification scheme for high redshift galaxies is complex at the present time, with simple colour selection criteria, resulting in ill-defined properties regarding stellar ma…