LOFAR takes the pulse of the radio sky
14 April 2011
The unique construction of LOFAR means that it can look in many different directions at the same time. This image shows the pulse profiles of five pulsars which were observed simultaneously using LOFAR at a frequency of just 50 MHz. Their positions are shown superimposed on a radio image of the sky at 408 MHz. The pointing directions of the two outermost beams were separated by over 65 degrees.
Image Credit: LOFAR / University of Manchester
The LOFAR 'superterp', part of the core of the extended telescope located in the Netherlands.
Image Credit: LOFAR / ASTRON.
A powerful new telescope is allowing an international team lead by University of Manchester scientists to have their "best-ever look" at pulsars: rapidly rotating neutron stars, created when massive stars die.
In the first refereed scientific results from the new European telescope LOFAR (Low Frequency Array) soon to appear in Astronomy & Astrophysics, the scientists present the most sensitive low-frequency observations of pulsars ever made.
The International LOFAR Telescope is the first in a new generation of massive radio telescopes, designed to study the sky at the lowest radio frequencies accessible from the surface of the Earth with unprecedented resolution. Deep observations of pulsars is one of its key science goals.
Dr Benjamin Stappers, from the University of Manchester's Jodrell Bank centre for Astrophysics who co-leads one of the Key Science Projects of LOFAR and is the lead author on the paper, said:
"We are returning to the frequencies where pulsars were first discovered, but now with a telescope of a sophistication that could not have been imagined back in the 1960s."
The chance detection of the first pulsar in 1967 is considered one of the great discoveries in astronomy. Astronomers got their first glimpse of pulsars by using a radio telescope sensitive to frequencies of 81MHz (roughly the same frequency as a commercial FM radio station).
With LOFAR, astronomers have gone back to some of the same techniques used in the first pulsar observations, but have used modern computing and optical fibre connections to increase many times over the power of their telescope. This will allow LOFAR to analyse regular pulses of radio emission and probe such things as the physics of gravity and the properties of the material that pervades our Galaxy.
Dr Stappers said:
"Even though these are just the first test results they are already showing spectacular promise."
LOFAR works by connecting thousands of small antennas spread right across Europe using high speed internet and a massive supercomputer near its central core at ASTRON in the Netherlands.
The LOFAR telescope has no moving parts, instead relying on adding digital time delays to to "point" the telescope in a particular direction. This approach offers a much-greater level of flexibility in the way astronomers can analyse the data. For instance, unlike a conventional radio telescope, it is possible to point in multiple directions simultaneously simply by having the computer crunch more data.
For astronomers who want to search for new pulsars, this means they can scan the sky much more quickly.
Dr Jason Hessels from ASTRON in the Netherlands said:
"A traditional radio telescope is limited to viewing a very small fraction of the sky at any one time. LOFAR casts a much broader net, which is going to help us discover new pulsars and detect explosions that were too rare to catch with past telescopes."
Dr Aris Karastergiou of the Univesrity of Oxford says:
"Pulsars are brightest at wavelengths observed by LOFAR and show a variety of puzzling emission features. We are very excited about using the centre of LOFAR in the Netherlands, and the international stations such as Chilbolton in the UK in a new approach to understanding these exotic objects."
The team's next step is to harness LOFAR's capabilities to address some of the long-standing mysteries about how pulsars shine and also to discover nearby pulsars that were missed by past telescopes.
"LOFAR has the potential to find all the undiscovered pulsars in the neighbourhood of the Sun and to reveal rare explosions in our Galaxy and beyond. We're very excited to see what's out there."says Tom Hassall, a Manchester University PhD student working on the project.
LOFAR is capable of detecting radio waves over a very large range of frequencies, all the way from 10MHz to 240MHz. As well as searching for pulsars, LOFAR will be used for making deep images, cosmology, to monitor the Sun's activity and study planets. LOFAR will also contribute to UK and European preparations for the planned global next generation radio telescope, the Square Kilometre Array (SKA).
Notes for Editors
The paper, "Observing Pulsars and fast transients with LOFAR", is available on request from the Press Office, and as an electronic preprint on the ArXiV.
Dr Stappers is available for interview on request.
For media enquiries please contact:
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The University of Manchester
0161 275 8387
The International LOFAR Telescope (ILT) is a Pan-European collaborative project led by ASTRON (the Netherlands Institute for Radio Astronomy). Combining thousands of simple dipole receivers with powerful digital signal processing and high-performance computing, LOFAR can rapidly survey wide areas of the sky, looking in multiple directions simultaneously and relatively unexplored low frequencies, opening open up a new window for astronomers.
LOFAR will focus on six areas of research:
- The Epoch of Reionisation - understanding how the first stars and black holes made the universe hot.
- Extragalactic surveys - what is the history of star formation and black hole growth over cosmological time?
- Transients and Pulsars - probing the extreme astrophysical environments that lead to transient bright bursts in the radio sky.
- Cosmic rays - what is the origin of the most energetic particles in the universe?
- Solar and space environment - mapping the structure of the solar wind, how it relates to solar bursts, and how it interacts with the Earth.
- Cosmic Magnetism - what is the origin of the large-scale magnetic fields that pervade the universe?
A pulsar is a neutron star, which is the collapsed core of a massive star that has ended its life in a supernova explosion. Weighing more than our Sun, yet only 20 kilometres across, these incredibly dense objects produce a beam of radio waves which sweeps around the sky like a lighthouse, often hundreds of times a second. Radio telescopes receive a regular train of pulses as the beam repeatedly crosses the Earth so the object is observed as a pulsating radio signal.
LOFAR-UK (the UK contribution to LOFAR)
The LOFAR station at the STFC Chilbolton Observatory in Hampshire was opened by Professor Jocelyn Bell-Burnell on the 20th September 2010. Like all the other stations, it is linked back to a central supercomputing facility at Groningen in the Netherlands using a high-speed network connection, the equivalent of 5000 standard domestic broadband connections combined into one.
LOFAR-UK is funded through a collaboration of UK universities with the SEPnet consortium and the UK Science and Technologies Facilities Council which includes RAL Space at STFC's Rutherford Appleton Laboratory, STFC's UK Astronomy Technology Centre and STFC's Chilbolton Observatory.The LOFAR-UK consortium represents 22 British universities, making it the largest radio astronomy consortium in the country. Over 70 leading UK astronomers are directly involved in the project. The universities involved include Aberystwyth, Birmingham, Cambridge, Cardiff, Durham, Edinburgh, Glasgow, Hertfordshire, Leicester, Liverpool John Moores, Kent, Manchester, Newcastle, Nottingham, Open University, Oxford, Portsmouth, Queen Mary University of London, Sheffield, Southampton, Sussex, and University College London.