The LOFAR Two-Meter Sky Survey: Deep Fields Data Release 1 I. Direction-dependent calibration and imaging

The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic surveys. It has a large field of view and is sensitive to large-scale and compact emission. It is, however, very challenging to synthesize thermal noise limited maps at full resolution, mainly because of the complex...

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Detalhes bibliográficos
Main Authors: Tasse, C, Shimwell, T, Hardcastle, MJ, O'Sullivan, SP, van Weeren, R, Best, PN, Bester, L, Hugo, B, Smirnov, O, Sabater, J, Calistro-Rivera, G, de Gasperin, F, Morabito, LK, Roettgering, H, Williams, WL, Bonato, M, Bondi, M, Botteon, A, Brueggen, M, Brunetti, G, Chyzy, KT, Garrett, MA, Guerkan, G, Jarvis, MJ, Kondapally, R, Mandal, S, Prandoni, I, Repetti, A, Retana-Montenegro, E, Schwarz, DJ, Shulevski, A, Wiaux, Y
Formato: Journal article
Idioma:English
Publicado em: EDP Sciences 2021