LOFAR imaging capabilities and system sensitivity

@inproceedings{Nijboer2013LOFARIC,
  title={LOFAR imaging capabilities and system sensitivity},
  author={Ronald Nijboer and M. Pandey-Pommier and A. G. de Bruyn},
  year={2013}
}
This document describes the general astronomical capabilities of the LOw Frequency ARray (LOFAR). The frequency range covered by LOFAR is split into two bands denoted as low band (LB, 10 - 80 MHz) and high band (HB, 120 - 240 MHz). LOFAR stations are spread over a 100 km sized region in the northern part of the Netherlands. In addition to the Dutch stations there will be European stations providing baselines between 200 km and 1000 km. Most of the results in this document, however, are limited… CONTINUE READING

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