activity
20162026
most citedThe Sardinia Radio Telescope: From a Technological Project to a Radio Observatory

82 citations · 434 across the 43 of their papers we have counts for

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12 papers · 1 filter

astro-ph.HE2026

Supernova remnants in the new radio astronomy era

A. Ingallinera, M. Arias, G. Castelletti +25

Supernova remnants (SNRs) are what is left after stellar explosions, when the stellar ejecta, the explosion shock and the circumstellar medium interact. Despite being among the fir…

astro-ph.HE2025

Broadband radio study of the supernova remnant Kes 73

S. Loru, A. Ingallinera, A. Pellizzoni +16

Strong shocks occurring in supernova remnants (SNRs), and their interaction with an often anisotropic surrounding medium, make SNRs ideal laboratories for studying the production a…

astro-ph.HE2023

EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8-6.3

Miroslav D. Filipović, Shi Dai, Bojan Arbutina +36

We present the serendipitous detection of a new Galactic Supernova Remnant (SNR), G288.8-6.3 using data from the Australian Square Kilometre Array Pathfinder (ASKAP)-Evolutionary M…

astro-ph.HE2022★ 6 cited

Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A

O. Petruk, V. Beshley, S. Orlando +7

The detected polarized radio emission from remnant of SN1987A opens the possibility to unveil the structure of the pre-supernova magnetic field in the circumstellar medium. Propert…

astro-ph.HE2022

Deep X-ray and radio observations of the first outburst of the young magnetar Swift J1818.0-1607

A. Y. Ibrahim, A. Borghese, N. Rea +23

Swift J1818.0-1607 is a radio-loud magnetar with a spin period of 1.36 s and a dipolar magnetic field strength of B~3E14 G, which is very young compared to the Galactic pulsar popu…

astro-ph.HE2020★ 8 cited

Investigating the mini and giant radio flare episodes of Cygnus X-3

E. Egron, A. Pellizzoni, S. Righini +16

The microquasar Cygnus X-3 underwent a giant radio flare in April 2017, reaching a maximum flux of Jy at 8.5 GHz. We present results from a long monitoring campaign car…