LOFAR: Recent imaging results & future prospects
Proceedings of the "Diffuse Relativistic Plasmas" conference, Bangalore, 1-4 March 2011
Journal of Astrophysics and Astronomy (2011)
arXiv:1106.3195
G. Heald et al. (including O. Wucknitz)
Abstract
The Low Frequency Array (LOFAR) is under construction in the Netherlands and in several surrounding European countries. In this contribution, we describe the layout and design of the telescope, with a particular emphasis on the imaging characteristics of the array when used in its "standard imaging" mode. After briefly reviewing the calibration and imaging software used for LOFAR image processing, we show some recent results from the ongoing imaging commissioning efforts. We conclude by summarizing future prospects for the use of LOFAR in observing the little-explored low frequency Universe.
On behalf of the LOFAR collaboration
Journal of Astrophysics and Astronomy (2011)
arXiv:1106.3195 (link to e-print archive)
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PDF file (706.0 kB, last change 20 Sep 2011)
10 pages, astro-ph version
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Script last modified on 7 Sep 2010
Last change to this data base entry on 20 Sep 2011