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.
Currently, there is a limited but diverse set of standard observing capabilities. 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 1 running from 15 November 2013 to 14 May 2014. Open to the worldwide community. Submission deadline: Friday 6 September 2013, 12:00 UT.
** Proposers must ensure that their justification files adhere to the instructions given the proposal call and in Northstar, repeated online here. **
Supplemental call for Director's Discretionary Time open to established Cycle 0 observers only. Submission deadline: Wednesday 31 July 2013, 12:00 UT.
Proposals should be submitted using the "NorthStar for LOFAR" proposal submission tool.A short "Walk Though" (version 18-07-2013) manual of NorthStar [PDF file].
Answers to some Frequently Asked Questions for the use of NorthStar during the "Call for Proposals"
Proposers will be able to use the online "LOFAR Data Volume Calculator"
Further questions can be addressed to the Radio Observatory Science Support Group: sciencesupport_AT_astron.nl