activity
20042026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 10.1k across the 112 of their papers we have counts for

collaborators

107 papers

astro-ph.GA2026

Deep radio characterization of the supernova remnant G343.1-00.7

S. Loru, A. Ingallinera, C. Trigilio +21

Supernova remnants (SNRs) are extended radio sources whose morphology and evolution are shaped by the interaction of strong shocks with the surrounding medium. We combined the 0.94…

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.SR2023★ 3 cited

The rich molecular environment of the luminous blue variable star AFGL 2298

J. R. Rizzo, C. Bordiu, C. Buemi +6

We investigated the molecular environment of AFGL 2298, an obscured Galactic Luminous blue variable (LBV) star which hosts a highly structured circumstellar environment with hints…

cs.CV2023★ 1 cited

RADiff: Controllable Diffusion Models for Radio Astronomical Maps Generation

Renato Sortino, Thomas Cecconello, Andrea DeMarco +10

Along with the nearing completion of the Square Kilometre Array (SKA), comes an increasing demand for accurate and reliable automated solutions to extract valuable information from…

astro-ph.GA2023★ 31 cited

A Catalogue of Radio Supernova Remnants and Candidate Supernova Remnants in the EMU/POSSUM Galactic Pilot Field

Brianna D. Ball, Roland Kothes, Erik Rosolowsky +15

We use data from the pilot observations of the EMU/POSSUM surveys to study the "missing supernova remnant (SNR) problem", the discrepancy between the number of Galactic SNRs that h…

astro-ph.EP2023★ 6 cited

Star-Planet Interaction at radio wavelengths in YZ Ceti: Inferring planetary magnetic field

Corrado Trigilio, Ayan Biswas, Paolo Leto +13

In exoplanetary systems, the interaction between the central star and the planet can trigger Auroral Radio Emission (ARE), due to the Electron Cyclotron Maser mechanism. The high b…