activity
19972025
most citedDust in active nuclei. II. Powder or gravel?

214 citations · 1.5k across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.GA2025

The accretion of quasars at the epoch of reionisation: catches the primeval monsters slowly feasting

B. Trefoloni, E. Nardini, S. Carniani +8

Quasars (QSOs) emit an enormous amount of light as a result of the accretion of gas onto supermassive black holes (SMBHs). Thanks to their luminosity, the most distant known QSOs a…

astro-ph.GA2024★ 6 cited

The near-infrared SED of blue quasars: what drives the evolution of the dusty torus?

Bartolomeo Trefoloni, Roberto Gilli, Elisabeta Lusso +5

A fundamental ingredient in the unified model of active galactic nuclei (AGN) is the obscuring torus, whose innermost, hottest region dominates the near infrared (NIR) emission. Ch…

astro-ph.GA2024★ 12 cited

Quasars as standard candles VI: spectroscopic validation of the cosmological sample

Bartolomeo Trefoloni, Elisabeta Lusso, Emanuele Nardini +5

A sample of quasars has been recently assembled to investigate the non-linear relation between their monochromatic luminosities at 2500Å, and 2 keV and to exploit quasars as a new…

astro-ph.GA2020★ 176 cited

Quasars as standard candles III. Validation of a new sample for cosmological studies

E. Lusso, G. Risaliti, E. Nardini +15

We present a new catalogue of ~2,400 optically selected quasars with spectroscopic redshifts and X-ray observations from either Chandra or XMM-Newton. The sample can be used to inv…

astro-ph.IM2020★ 1 cited

End to end simulators: A flexible and scalable Cloud-Based architecture. Application to High Resolution Spectrographs ESPRESSO and ELT-HIRES

M. Genoni, M. Landoni, G. Pariani +7

Simulations of frames from existing and upcoming high-resolution spectrographs, targeted for high accuracy radial velocity measurements, are computationally demanding (both in time…

astro-ph.GA2018★ 18 cited

The VLT/MUSE view of the central galaxy in Abell 2052. Ionized gas swept by the expanding radio source

B. Balmaverde, A. Capetti, A. Marconi +1

We report observations of the radio galaxy 3C317 (at z=0.0345) located at the center of the Abell cluster A2052, obtained with the VLT/MUSE integral field spectrograph. The Chandra…