activity
20172022
most citedThe ASTRI Mini-Array of Cherenkov Telescopes at the Observatorio del Teide

58 citations · 168 across the 5 of their papers we have counts for

collaborators

6 papers

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★ 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★ 14 cited

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

F. G. Saturni, C. H. E. Arcaro, B. Balmaverde +47

The ASTRI Mini-Array is a next-generation system of nine imaging atmospheric Cherenkov telescopes that is going to be built at the Observatorio del Teide site. After a first phase,…

astro-ph.HE2021★ 14 cited

Dramatic changes in the observed velocity of the accretion disk wind in MCG-03-58-007 are revealed by XMM-Newton and NuSTAR

V. Braito, J. N. Reeves, G. Matzeu +6

Past X-ray observations of the nearby Seyfert 2 MCG-03-58-007 revealed the presence of a powerful and highly variable disk wind, where two possible phases outflowing with $v_{\rm o…

astro-ph.HE2021★ 26 cited

Direct observation of an extended X-ray jet at =6.1

L. Ighina, A. Moretti, F. Tavecchio +6

We report on the direct observation of an extended X-ray jet in the =6.1 radio-loud Active Galactic Nucleus PSO J030947.49+271757.31 from a deep Chandra X-ray observation (128 k…

astro-ph.GA2017

AGN with discordant optical and X-ray classification are not a physical family: Diverse origin in two AGN

I. Ordovás-Pascual, S. Mateos, F. J. Carrera +7

Approximately 3-17 percent of Active Galactic Nuclei (AGN) without detected rest-frame UV/optical broad emission lines (type-2 AGN) do not show absorption in X-rays. The physical o…