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
1 code implementation • 19 Nov 2018 • S. Mooney, J. Quinn, J. R. Callingham, R. Morganti, K. Duncan, L. K. Morabito, P. N. Best, G. Gürkan, M. J. Hardcastle, I. Prandoni, H. J. A. Röttgering, J. Sabater, T. W. Shimwell, A. Shulevski, C. Tasse, W. L. Williams
We used the LOFAR Two-Metre Sky Survey (LoTSS) first data release value-added catalogue (LDR1) to study blazars in the low-frequency regime with unprecedented sensitivity and resolution.
High Energy Astrophysical Phenomena
1 code implementation • 6 Dec 2017 • C. Tasse, B. Hugo, M. Mirmont, O. Smirnov, M. Atemkeng, L. Bester, M. J. Hardcastle, R. Lakhoo, S. Perkins, T. Shimwell
In this paper we discuss and implement a wide-band wide-field spectral deconvolution framework (DDFacet) based on image plane faceting, that takes into account generic direction-dependent effects.
Instrumentation and Methods for Astrophysics
