no code implementations • 18 Dec 2020 • T. H. Jarrett, A. Comrie, L. Marchetti, A. Sivitilli, S. Macfarlane, F. Vitello, U. Becciani, A. R. Taylor, J. M. van der Hulst, P. Serra, N. Katz, M. Cluver
In the new era of Big Data ushered in by major facilities such as the SKA and LSST that render past analysis and refinement methods highly constrained, we believe that a paradigm shift to new software, technology and methods that exploit the power of visual perception, will play an increasingly important role in bridging the gap between statistical metrics and new discovery.
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies
no code implementations • 10 Dec 2020 • J. Delhaize, I. Heywood, M. Prescott, M. J. Jarvis, I. Delvecchio, I. H. Whittam, S. V. White, M. J. Hardcastle, C. L. Hale, J. Afonso, Y. Ao, M. Brienza, M. Brueggen, J. D. Collier, E. Daddi, M. Glowacki, N. Maddox, L. K. Morabito, I. Prandoni, Z. Randriamanakoto, S. Sekhar, FangXia An, N. J. Adams, S. Blyth, R. A. A. Bowler, L. Leeuw, L. Marchetti, S. M. Randriamampandry, K. Thorat, N. Seymour, O. Smirnov, A. R. Taylor, C. Tasse, M. Vaccari
However, the excellent sensitivity and uv coverage of the new MeerKAT telescope allowed this diffuse emission to be detected.
Astrophysics of Galaxies