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

collaborators
Showing 2024Show all

7 papers · 1 filter

astro-ph.GA2024★ 17 cited

Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey

L. D. Anderson, F. Camilo, Timothy Faerber +13

Context. Sensitive radio continuum data could remove the difference between the number of known supernova remnants (SNRs) in the Galaxy compared to that expected, but due to confus…

astro-ph.GA2024

Sifting the debris: Patterns in the SNR population with unsupervised ML methods

F. Bufano, C. Bordiu, T. Cecconello +13

Supernova remnants (SNRs) carry vast amounts of mechanical and radiative energy that heavily influence the structural, dynamical, and chemical evolution of galaxies. To this day, m…

astro-ph.IM2024★ 8 cited

Self-supervised contrastive learning of radio data for source detection, classification and peculiar object discovery

S. Riggi, T. Cecconello, S. Palazzo +14

New advancements in radio data post-processing are underway within the SKA precursor community, aiming to facilitate the extraction of scientific results from survey images through…

astro-ph.SR2024

The distance to CRL 618 through its radio expansion parallax

L. Cerrigone, G. Umana, C. Trigilio +9

CRL 618 is a post-AGB star that has started to ionize its ejecta. Its central HII region has been observed over the last 40 years and has steadily increased in flux density at radi…

astro-ph.IM2024

Classification of compact radio sources in the Galactic plane with supervised machine learning

S. Riggi, G. Umana, C. Trigilio +13

Generation of science-ready data from processed data products is one of the major challenges in next-generation radio continuum surveys with the Square Kilometre Array (SKA) and it…

astro-ph.SR2024

Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes II. Evidence for coronal emission

M. Marongiu, A. Pellizzoni, S. Righini +43

One of the most important objectives of solar physics is the physical understanding of the solar atmosphere, the structure of which is also described in terms of the density (N) an…