The International LOFAR Telescope (ILT) is a powerful next-generation radio telescope for frequencies below 240 MHz that offers revolutionary new observing capabilities thanks to its phased-array technology with digital beam-forming.
LOFAR delivers correlated visibility data for synthesis imaging, plus in/coherently added single and multiple station data (several beam-formed modes) as well as transient buffer read-out, for example for studies of pulsars, transients, and cosmic rays.
Cycle 12 will run from 1 June – 30 November 2019. Submission deadline: 6 March 2019.
**Proposers must ensure that their justification files adhere to the instructions given in the proposal call and in Northstar, repeated online here. **