activity
20002016
most citedThe M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6

91 citations · 314 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2016★ 28 cited

Detection of faint broad emission lines in type 2 AGN: I. Near infrared observations and spectral fitting

F. Onori, F. La Franca, F. Ricci +8

We present medium resolution near infrared spectroscopic observations of 41 obscured and intermediate class AGN (type 2, 1.9 and 1.8; AGN2) with redshift 0.1, selected…

astro-ph.GA2014★ 91 cited

The M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6

A. Bongiorno, R. Maiolino, M. Brusa +12

We present near-infrared spectra, obtained with SINFONI and XShooter observations at ESO VLT, of nine dusty, red QSOs at 1.2<z<2.6. The sources are hard X-ray detected, characteriz…

astro-ph.CO2010★ 31 cited

The HELLAS2XMM survey. XIII. Multi-component analysis of the spectral energy distribution of obscured AGN

F. Pozzi, C. Vignali, A. Comastri +9

We combine near-to-mid-IR Spitzer data with shorter wavelength observations (optical to X-rays) to get insights on the properties of a sample of luminous, obscured Active Galactic…

astro-ph.CO2009★ 65 cited

Exploring the active galactic nucleus and starburst content of local ultraluminous infrared galaxies through 5-8 micron spectroscopy

E. Nardini, G. Risaliti, M. Salvati +4

We present a 5-8 micron analysis of the Spitzer-IRS spectra of 71 ultraluminous infrared galaxies (ULIRGs) with redshift z < 0.15, devoted to the study of the role of active galact…

astro-ph2008★ 24 cited

Prospects for AGN studies with ALMA

R. Maiolino

These lecture notes provide an introduction to mm/submm extragalactic astronomy, focused on AGN studies, with the final goal of preparing students to their future exploitation of t…

astro-ph2001★ 33 cited

A new population of soft X-ray weak quasars

G. Risaliti, A. Marconi, R. Maiolino +2

Quasars selected in optical surveys by means of their blue or UV excess are known to be strong emitters in the X-rays, except for Broad Absorption Line (BAL) objects. In this paper…