activity
20092026
most citedSwift and NuSTAR observations of GW170817: detection of a blue kilonova

579 citations · 1.1k across the 29 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.HE2022★ 11 cited

Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1

F. Barra, C. Pinto, D. J. Walton +11

Despite two decades of studies, it is still not clear whether ULX spectral transitions are due to stochastic variability in the wind or variations in the accretion rate or in the s…

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★ 6 cited

A transient ultraluminous X-ray source in NGC 55

A. Robba, C. Pinto, F. Pintore +14

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10 erg s. The average number of ULXs per galaxy is still not…

astro-ph.HE2022★ 8 cited

Investigating the nature and properties of MAXI J1810-222 with radio and X-ray observations

T. D. Russell, M. Del Santo, A. Marino +10

We present results from radio and X-ray observations of the X-ray transient MAXI J1810-222. The nature of the accretor in this source has not been identified. In this paper, we sho…

astro-ph.HE2022★ 21 cited

A blast from the infant Universe: the very high-z GRB 210905A

A. Rossi, D. D. Frederiks, D. A. Kann +52

We present a detailed follow-up of the very energetic GRB 210905A at a high redshift of z = 6.312 and its luminous X-ray and optical afterglow. We obtained a photometric and spectr…