Progress with the LOFAR Imaging Pipeline

Open Access
Authors
  • G. Heald
  • J. McKean
  • R. Pizzo
  • G. van Diepen
  • J.E. van Zwieten
  • R.J. van Weeren
  • D. Rafferty
  • S. van der Tol
  • L. Birzan
  • A. Shulevski ORCID logo
  • J. Swinbank
  • E. OrrĂ¹
  • F. de Gasperin
  • L. Ker
  • A. Bonafede
  • G. Macario
  • C. Ferrari
Publication date 2010
Journal Proceedings of Science
Event International SKA Forum 2010 (ISKAF2010), Nooitgedacht, the Netherlands
Article number 057
Volume | Issue number 112
Number of pages 12
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
One of the science drivers of the new Low Frequency Array (LOFAR) is large-area surveys of the low-frequency radio sky. Realizing this goal requires automated processing of the interferometric data, such that fully calibrated images are produced by the system during survey operations. The LOFAR Imaging Pipeline is the tool intended for this purpose, and is now undergoing significant commissioning work. The pipeline is now functional as an automated processing chain. Here we present several recent LOFAR images that have been produced during the still ongoing commissioning period. These early LOFAR images are representative of some of the science goals of the commissioning team members.
Document type Article
Note Proceedings title: ISKAF2010 science meeting: June 10-14 2010, Assen, The Netherlands Publisher: SISSA Place of publication: Trieste
Language English
Published at https://arxiv.org/abs/1008.4693 http://pos.sissa.it/archive/conferences/112/057/ISKAF2010_057.pdf
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336412.pdf (Final published version)
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