works on

From the 1 of 6 linked papers with an AI index.

activity
20242026
collaborators

6 papers

astro-ph.GA2026

The Nearest Galactic Nucleus: Studying the Galactic Centre with SKA-Mid

Rainer Schoedel, Antxon Alberdi, Izaskun Jiménez-Serra +24

The paper proposes a large-area, multi‑wavelength continuum survey of the Galactic Centre using SKA‑Mid, covering ~2°×0.4° around Sagittarius A* and repeated deep observations of t…

astro-ph.GA2025

Gas-rich dwarf galaxy multiples in the Apertif HI survey

B. Å iljeg, E. A. K. Adams, F. Fraternali +8

Dwarf-dwarf galaxy encounters are a key aspect of galaxy evolution as they can ignite or temporarily suppress star formation in dwarfs and can lead to dwarf mergers. However, the f…

astro-ph.IM2025

3D radio data visualisation in open science platforms for next-generation observatories

I. Labadie-García, J. Garrido, L. Verdes-Montenegro +4

Next-generation telescopes will bring groundbreaking discoveries but they will also present new technological challenges. The Square Kilometre Array Observatory (SKAO) will be one…

astro-ph.IM2025

Open Science and Artificial Intelligence for supporting the sustainability of the SRC Network: The espSRC case

J. Garrido, S. Sánchez-Expósito, A. Ruiz-Falcó +11

The SKA Observatory (SKAO), a landmark project in radio astronomy, seeks to address fundamental questions in astronomy. To process its immense data output, approximately 700 PB/yea…

astro-ph.IM2025

Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experiment

A. Bonaldi, P. Hartley, R. Braun +179

We present and analyse the results of the Science data challenge 3a (SDC3a, https://sdc3.skao.int/challenges/foregrounds), an EoR foreground-removal community-wide exercise organis…

astro-ph.GA2024

Photometry and kinematics of dwarf galaxies from the Apertif HI survey

Barbara Å iljeg, Elizabeth A. K. Adams, Filippo Fraternali +13

Context. Understanding the dwarf galaxy population in low density environments is crucial for testing the LCDM cosmological model. The increase in diversity towards low mass galaxi…