June 1st, 2010 - Written by Nancy Atkinson
Radio images of the quasar 3C 196 at 4 - 10 m wavelength (30 - 80 MHz frequency). Left: Data from LOFAR stations in the Netherlands only. The resolution is not sufficient to identify any substructure. Right: Blow-up produced with data from the German stations included. The resolution of this image is about ten times better and allows for the first time to distinguish fine details in this wavelength range. The colours are chosen to resemble what the human eye would see if it were sensitive to radiation at a wavelength ten million times larger than visible light. Image: Olaf Wucknitz, Bonn University (Click to enlarge image).
Just eight of the eventual forty-four antenna stations for the LOw Frequency ARray (LOFAR) were combined to produce the first high-resolution image of a distant quasar at meter radio wavelengths. The first image shows fine details of the quasar 3C 196, a strong radio source several billion light years away, observed at wavelengths between 4 and 10 m. "We chose this object for the first tests, because we know its structure very well from observations at shorter wavelengths," said Olaf Wucknitz from Bonn University. "The goal was not to find something new but to see the same or similar structures also at very long wavelengths to confirm that the new instrument really works. Without the German stations, we only saw a fuzzy blob, no sub-structure. Once we included the long baselines, all the details showed up."
Five stations in the Netherlands were connected with three stations in Germany. To make detailed observations at such low frequencies, the telescopes have to be spaced far apart. When complete, the LOFAR array span across a large part of Europe.
Observations at wavelengths covered by LOFAR are not new. In fact, the pioneers of radio astronomy started their work in the same range. However, they were only able to produce very rough maps of the sky and to measure just the positions and intensities of objects.
"We are now returning to this long neglected wavelength range", says Michael Garrett, general director of ASTRON, in The Netherlands, the institution that leads the international LOFAR project. "But this time we are able to see much fainter objects and, even more important, to image very fine details. This offers entirely new opportunities for astrophysical research."
"The high resolution and sensitivity of LOFAR mean that we are really entering uncharted territory, and the analysis of the data was correspondingly intricate", adds Olaf Wucknitz. "We had to develop completely new techniques. Nevertheless, producing the images went surprisingly smoothly in the end. The quality of the data is stunning." The next step for Wucknitz is to use LOFAR to study so-called gravitational lenses, where the light from distant objects is distorted by large mass concentrations. High resolution is required to see the interesting structures of these objects. This research would be impossible without the international stations.
IS-DE1: Some of the 96 low-band dipole antennas, Effelsberg LOFAR station (foreground); high-band array (background) (Credit: James Anderson, MPIfR)
LOFAR will consist of at least 36 stations in the Netherlands and eight stations in Germany, France, the United Kingdom and Sweden. Currently 22 stations are operational and more are being set up. Each station consists of hundreds of dipole antennas that are connected electronically to form a huge radio telescope that will cover half of Europe. With the novel techniques introduced by LOFAR, it is no longer necessary to point the radio antennas at specific objects of interest. Instead it will be possible to observe several regions of the sky simultaneously.
The resolution of an array of radio telescopes depends directly on the separation between the telescopes. The larger these baselines are relative to the observed wavelength, the better the achieved resolution. Currently the German stations provide the first long baselines of the array and improve the resolution by a factor of ten over just using the Dutch stations. ASTRON officials say the imaging quality will improve significantly as more stations come online.
"We want to use LOFAR to search for signals from very early epochs of the Universe,, said Benedetta Ciardi from the Max-Planck-Institut für Astrophysik (MPA) in Garching. "Having a completely theoretical background myself, I never had thought that I would get excited over a radio image, but this result is really fascinating."
Source: Max-Planck-Institut für Astrophysik
http://www.universetoday.com/2010/06/01 ... far-array/
The International LOFAR telescope (ILT) is being primarily built by ASTRON, the Netherlands Institute for Radio Astronomy, in collaboration with a number of international partners. The LOFAR station at Effelsberg is operated by MPIfR, the one in Unterweilenbach by MPA and the Tautenburg station by Thüringer Landessternwarte. The German LOFAR partners form GLOW, the German LOng Wavelength consortium.
In its final stages, the international LOFAR array will consist of at least 36 stations in the Netherlands and eight stations in Germany, France, the United Kingdom and Sweden. Currently 22 stations are operational and more are being set up in Bornim near Potsdam (Germany), Chilbolton (UK), Onsala (Sweden) and Nançay (France). Each station consists of hundreds of dipole antennas that are connected electronically to form a huge radio telescope that will cover half of Europe. With the novel techniques introduced by LOFAR, it is no longer necessary to point the radio antennas at specific objects of interest. Instead it will be possible to observe several regions of the sky simultaneously.
The data from all LOFAR stations are transfered via powerful fibre optic cables in research networks to the computing centre in Groningen in the north of the Netherlands. There they are combined and preprocessed for the final analysis which can be performed either there or at any of the participating institutes, in this case at the Argelander-Institute for Astronomy in Bonn.
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