activity
19982025
most citedStar formation efficiency in galaxy interactions and mergers: a statistical study

474 citations · 2.8k across the 45 of their papers we have counts for

collaborators

47 papers

astro-ph.GA2025

YOLO-CIANNA: Galaxy detection with deep learning in radio data: II. Winning the SKA SDC2 using a generalized 3D-YOLO network

D. Cornu, B. Semelin, P. Salomé +8

As the scientific exploitation of the Square Kilometre Array (SKA) approaches, there is a need for new advanced data analysis and visualization tools capable of processing large hi…

astro-ph.IM2024★ 16 cited

YOLO-CIANNA: Galaxy detection with deep learning in radio data. I. A new YOLO-inspired source detection method applied to the SKAO SDC1

D. Cornu, P. Salomé, B. Semelin +8

The upcoming Square Kilometer Array (SKA) will set a new standard regarding data volume generated by an astronomical instrument, which is likely to challenge widely adopted data-an…

astro-ph.IM2023★ 22 cited

SKA Science Data Challenge 2: analysis and results

P. Hartley, A. Bonaldi, R. Braun +105

The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomer…

astro-ph.CO2023★ 6 cited

Studying the Multi-frequency Angular Power Spectrum of the Cosmic Dawn 21-cm Signal

Abinash Kumar Shaw, Raghunath Ghara, Saleem Zaroubi +5

The light-cone (LC) anisotropy arises due to cosmic evolution of the cosmic dawn 21-cm signal along the line-of-sight (LoS) axis of the observation volume. The LC effect makes the…

astro-ph.CO2023★ 15 cited

Accurate modelling of the Lyman- coupling for the 21-cm signal, observability with NenuFAR and SKA

Benoit Semelin, Romain Mériot, Florent Mertens +6

The measurement of the cm signal from the Cosmic Dawn is a major goal for several existing and upcoming radio interferometers such as NenuFAR and the SKA. During this era befo…

astro-ph.CO2022

A bubble size distribution model for the Epoch of Reionization

Aristide Doussot, Benoit Semelin

The bubble size distribution is a summary statistics that can be computed from the observed 21-cm signal from the Epoch of Reionization. As it depends only on the ionization field…