activity
20042026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 13.4k across the 179 of their papers we have counts for

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Showing 2014Show all

6 papers · 1 filter

astro-ph.GA2014★ 15 cited

Clustering of gamma-ray selected 2LAC Fermi Blazars

Viola Allevato, Alexis Finoguenov, Nico Cappelluti

We present the first measurement of the projected correlation function of 485 gamma-ray selected Blazars, divided in 175 BLLacertae (BL Lacs) and 310 Flat Spectrum Radio Quasars (F…

astro-ph.GA2014★ 62 cited

Clustering properties of moderate luminosity X-ray selected Type 1 and Type 2 AGN at z~3

V. Allevato, A. Finoguenov, F. Civano +11

We investigate, for the first time at z~3, the clustering properties of 189 Type 1 and 157 Type 2 X-ray active galactic nuclei (AGN) of moderate luminosity (log<Lbol> = 45.3 erg/s)…

astro-ph.GA2014★ 99 cited

The Hard X-Ray Luminosity Function of High-Redshift () Active Galactic Nuclei

Fabio Vito, Roberto Gilli, Cristian Vignali +4

We present the hard-band () X-ray luminosity function (HXLF) of band selected AGN at high redshift. We have assembled a sample of 141 AGN…

astro-ph.GA2014★ 18 cited

The evolution of star formation activity in galaxy groups

G. Erfanianfar, P. Popesso, A. Finoguenov +30

We study the evolution of the total star formation (SF) activity, total stellar mass and halo occupation distribution in massive halos by using one of the largest X-ray selected sa…

astro-ph.GA2014★ 90 cited

Compton Thick AGN in the XMM-COSMOS survey

G. Lanzuisi, P. Ranalli, I. Georgantopoulos +27

Heavily obscured, Compton Thick (CT, NH>10^24 cm^-2) AGN may represent an important phase in AGN/galaxy co-evolution and are expected to provide a significant contribution to the c…

astro-ph.GA2014★ 82 cited

The primordial environment of super massive black holes: large scale galaxy overdensities around QSOs with LBT

L. Morselli, M. Mignoli, R. Gilli +8

We investigated the presence of galaxy overdensities around four QSOs, namely SDSS J1030+0524 (z = 6.28), SDSS J1148+5251 (z = 6.41), SDSS J1048+4637 (z = 6.20) and SDSS J…