Low Frequency Array

 

LOFAR, the Low Frequency Array, is a new radio telescope under construction by ASTRON in the Netherlands and is operating in the largely unexplored frequency range between 10 and 240 MHz. LOFAR leads the way for a new generation of radio telescopes, like the planned  Square Kilometre Array (SKA), consisting of a multitude of small and cheap antennas. At present, LOFAR consists of 38 stations in the Netherlands, 5 in Germany, 3 in Poland and one each in France, Sweden, and the UK. Each station consists of two parts, one for the low band (LBA) between frequencies of 10 and 80 MHz and one for the high band between 110 and 240 MHz. Both parts are made of many dipole (192 for LBA and 3072 for the HBA in international stations) that are combined electronically. The signals are sent to the central computing facilities in Groningen (NL), where they are correlated in realtime and converted to images, spectra and time series for pulsar studies. LOFAR has many flexible observing modes that can be used to simultaneously point at several directions on the sky. Other modes allow monitoring of the entire visible radio sky continuously. The international baselines for the first time provide sub-arcsec resolutions in this frequency range.

The first international station (text  in German) next to the 100-m Effelsberg radio telescope was completed in 2009 and is run by the MPIfR in collaboration with ASTRON. The MPIfR is member of the German Long Wavelength Consortium (GLOW), which coordinates the collaboration with the other German LOFAR sites in Jülich, Norderstedt, Potsdam, Tautenburg and Unterweilenbach.

In addition to taking part in observations with the full array (International LOFAR Telescope, ILT) for various projects, including high-resolution studies of radio sources and pulsar surveys, the group is using the Effelsberg LOFAR station to image the Milky Way, study pulsars in detail, and for system tests and development.

The group founded the international LOFAR Key Science Project on Cosmic Magnetism. At low frequencies, weak extended synchrotron emission in the Milky Way, around galaxies and in galaxy clusters should become observable. This allows us to measure magnetic fields in intergalactic space. We are also involved in the  LOFAR Key Science Project on Transients and Pulsars and the Key Science Project on Surveys.

The first international LOFAR station in Effelsberg. In the foreground, the LBA antennas for 10–80 MHz are visible, in the background, the HBA antenna tiles for 110–240 MHz are hidden in styrofoam boxes covered with foil. The container to the right between the fields hosts the electronics where the signals from all individual antennas are digitised, calibrated and combined. Zoom Image
The first international LOFAR station in Effelsberg. In the foreground, the LBA antennas for 10–80 MHz are visible, in the background, the HBA antenna tiles for 110–240 MHz are hidden in styrofoam boxes covered with foil. The container to the right between the fields hosts the electronics where the signals from all individual antennas are digitised, calibrated and combined.
Winter 2012/2013 Zoom Image
Winter 2012/2013
 
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