no code implementations • 23 Feb 2024 • S. Riggi, G. Umana, C. Trigilio, C. Bordiu, F. Bufano, A. Ingallinera, F. Cavallaro, Y. Gordon, R. P. Norris, G. Gürkan, P. Leto, C. Buemi, S. Loru, A. M. Hopkins, M. D. Filipović, T. Cecconello
To this aim, we produced a curated dataset of ~20, 000 images of compact sources of different astronomical classes, obtained from past radio and infrared surveys, and novel radio data from pilot surveys carried out with the Australian SKA Pathfinder (ASKAP).
no code implementations • 15 Oct 2021 • S. Riggi, C. Bordiu, F. Vitello, G. Tudisco, E. Sciacca, D. Magro, R. Sortino, C. Pino, M. Molinaro, M. Benedettini, S. Leurini, F. Bufano, M. Raciti, U. Becciani
Innovative developments in data processing, archiving, analysis, and visualization are nowadays unavoidable to deal with the data deluge expected in next-generation facilities for radio astronomy, such as the Square Kilometre Array (SKA) and its precursors.
no code implementations • 11 Jan 2021 • S. Riggi, G. Umana, C. Trigilio, F. Cavallaro, A. Ingallinera, P. Leto, F. Bufano, R. P. Norris, A. M. Hopkins, M. D. Filipović, H. Andernach, J. Th. van Loon, M. J. Michałowski, C. Bordiu, T. An, C. Buemi, E. Carretti, J. D. Collier, T. Joseph, B. S. Koribalski, R. Kothes, S. Loru, D. McConnell, M. Pommier, E. Sciacca, F. Schilliró, F. Vitello, K. Warhurst, M. Whiting
We present observations of a region of the Galactic plane taken during the Early Science Program of the Australian Square Kilometre Array Pathfinder (ASKAP).
no code implementations • 14 Dec 2020 • C. Bordiu, F. Bufano, E. Sciacca, S. Riggi, M. Molinaro, G. Vizzari, M. Krokos, C. Brandt
We report the outcomes of a survey that explores the current practices, needs and expectations of the astrophysics community, concerning four research aspects: open science practices, data access and management, data visualization, and data analysis.
Data Visualization Instrumentation and Methods for Astrophysics
1 code implementation • 13 Sep 2019 • S. Riggi, F. Vitello, U. Becciani, C. Buemi, F. Bufano, A. Calanducci, F. Cavallaro, A. Costa, A. Ingallinera, P. Leto, S. Loru, R. P. Norris, F. Schillirò, E. Sciacca, C. Trigilio, G. Umana
Given the increased scale of the data, source extraction and characterization, even in this Early Science phase, have to be carried out in a mostly automated way.