activity
20012025
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 2.9k across the 61 of their papers we have counts for

collaborators

66 papers

astro-ph.HE2025★ 6 cited

Energy-resolved pulse profile changes in V 0332+53: Indications of wings in the cyclotron absorption line profile

Antonino D'Aì, Dimitrios K. Maniadakis, Carlo Ferrigno +15

We aim to investigate the energy-resolved pulse profile changes of the accreting X-ray pulsar V 0332+53, focusing in the cyclotron line energy range, using the full set of availabl…

astro-ph.IM2022★ 58 cited

The ASTRI Mini-Array of Cherenkov Telescopes at the Observatorio del Teide

Scuderi S., Giuliani A., Pareschi G. +95

The ASTRI Mini-Array (MA) is an INAF project to build and operate a facility to study astronomical sources emitting at very high-energy in the TeV spectral band. The ASTRI MA consi…

astro-ph.HE2022★ 12 cited

Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide

A. D'Aì, E. Amato, A. Burtovoi +52

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array will be composed of nine imaging atmospheric Cherenkov telescopes at the Observatorio del Teide site…

astro-ph.HE2022★ 56 cited

ASTRI Mini-Array Core Science at the Observatorio del Teide

S. Vercellone, C. Bigongiari, A. Burtovoi +84

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the Obse…

astro-ph.HE2022

Chandra Follow-up Observations of Swift-BAT-selected AGNs II

Ross Silver, Nuria Torres-Alba, Xiurui Zhao +7

We present the combined Chandra and Swift-BAT spectral analysis of nine low-redshift (z <= 0.10), candidate heavily obscured active galactic nuclei (AGN) selected from the Swift-BA…

astro-ph.HE2020★ 37 cited

Unveiling sub-parsec supermassive black hole binary candidates in active galactic nuclei

Roberto Serafinelli, Paola Severgnini, Valentina Braito +11

Elusive supermassive black hole binaries (SMBHBs) are thought to be the penultimate stage of galaxy mergers, preceding a final coalescence phase. SMBHBs are sources of continuous g…