activity
20092020
most citedSingle-dish and VLBI observations of Cygnus X-3 during the 2016 giant flare episode

36 citations · 136 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE202014 cited

New high-frequency radio observations of the Cygnus Loop supernova remnant with the Italian radio telescopes

S. Loru, A. Pellizzoni, E. Egron +19

Supernova remnants (SNRs) represent a powerful laboratory to study the Cosmic-Ray acceleration processes at the shocks, and their relation to the properties of the circumstellar me…

astro-ph.IM20191 cited

A multi-wavelength pipeline for pulsar searches

Maura Pilia, Alessio Trois, Matteo Bachetti +7

Pulsar studies in the recent years have shown, more than others, to have benefited from a multi-wavelength approach. The INAF - Astronomical Observatory in Cagliari (INAF-OAC) is a…

astro-ph.HE2018

Investigating the high-frequency spectral features of SNRs Tycho, W44 and IC443 with the Sardinia Radio Telescope

S. Loru, A. Pellizzoni, E. Egron +20

The main characteristics in the radio continuum spectra of Supernova Remnants (SNRs) result from simple synchrotron emission. In addition, electron acceleration mechanisms can shap…

astro-ph.HE201736 cited

Single-dish and VLBI observations of Cygnus X-3 during the 2016 giant flare episode

E. Egron, A. Pellizzoni, M. Giroletti +34

In September 2016, the microquasar Cygnus X-3 underwent a giant radio flare, which was monitored for 6 days with the Medicina Radio Astronomical Station and the Sardinia Radio Tele…

astro-ph.HE201734 cited

Imaging of SNR IC443 and W44 with the Sardinia Radio Telescope at 1.5 GHz and 7 GHz

E. Egron, A. Pellizzoni, M. N. Iacolina +33

Observations of supernova remnants (SNRs) are a powerful tool for investigating the later stages of stellar evolution, the properties of the ambient interstellar medium, and the ph…

astro-ph.HE200915 cited

Searching for pulsed emission from XTE J0929-314 at high radio frequencies

M. N. Iacolina, M. Burgay, L. Burderi +2

The aim of this work is to search for radio signals in the quiescent phase of accreting millisecond X-ray pulsars, in this way giving an ultimate proof of the recycling model, ther…