Tuesday, September 20, 2011

Welcome to Swedish LOFAR; making LOFAR even bigger

The Swedish LOFAR station in Onsala is to be opened on Monday, joining stations all over Europe to make the International LOFAR Telescope even bigger. Below is the press release from Onsala Space Observatory.

Swedes Make World's Largest Telescope Bigger

The 192 radio antennas that make up Onsala’s Lofar station cover an area the size of a soccer pitch. Credit: Onsala Space Observatory/Leif Helldner

On Monday, Sweden’s Minister for Education and Research, Jan Björklund, will open Onsala Space Observatory’s newest telescope. Part of LOFAR, the world’s largest radio telescope, it is the biggest telescope built in Sweden in the last 35 years. LOFAR will map radio signals which have travelled across the universe for billions of years. Scientists expect LOFAR to answer questions about the nature of our universe.

LOFAR (LOw Frequency ARray) is a new kind of radio telescope. It can see radio waves with low frequencies, similar to those that give us FM radio. Rather than collecting signals from individual radio sources, LOFAR continuously monitors large swathes of sky. Lofar is more sensitive to the longest observable radio waves than any other telescope. It can see many billions of light years out into space, back to the time before the first stars formed, a few hundred million years after the Big Bang.

The 192 new radio antennas at Onsala’s LOFAR station look modest enough. But the radio signals they collect will be linked together with 47 similar stations over the whole of Europe, and sent over Internet to a central supercomputer in the Netherlands. This means huge amount of data traffic: the equivalent of over 7000 DVD films per day just from the Swedish station. The telescope creates images of the sky using a unique combination of computer power and innovative software. Together, LOFAR’s antennas form a single telescope with a diameter of 1300 kilometres.

Hans Olofsson is director of Onsala Space Observatory and professor at Chalmers.

“For astronomers like me, LOFAR means that we can see far enough to be able to study the universe’s early history. We want to discover traces of the clouds of hydrogen gas that filled the universe 13 billion years ago, and find out just why today’s universe looks the way it does,” he says.

Scientists expect LOFAR to discover hitherto unknown types of astronomical objects. It will also investigate the environments of black holes, find extreme galaxies and pulsars, and search for planets around other stars.

Onsala Space Observatory was founded in 1949 and was led for three decades by Professor Olof Rydbeck. Since its inception the observatory has contributed to the forefront of research in radio astronomy, both through interpretation of observations and developing new technology. Since 1990 the observatory is the Swedish National Facility for Radio Astronomy. It is financed by the Swedish Research Council and operated by Chalmers.

“Onsala Space Observatory has always been a prominent centre for radio astronomy research, and now it’s part of the world’s most exciting radio telescope. In the future we plan to develop the technology that makes Lofar unique when we build the next generation of radio telescopes, says René Vermeulen of Astron, the Netherlands national institute for radio astronomy, and director of the International LOFAR Telescope.

LOFAR is one of many examples of Onsala Space Observatory’s increasing involvement in international projects. Chalmers is one of three international partners in the submillimetre telescope Apex in Chile, which recently discovered hydrogen peroxide in space. Last winter Chalmers delivered sensitive new receivers to the Alma Observatory, the world’s largest astronomy project, currently being built in Chile’s Atacama desert. The observatory is also planning for the radio observatory SKA (Square Kilometre Array), to be built in Australia or South Africa, in which LOFAR’s new technology will be developed even further. SKA is expected to give answers about the origins of both the universe itself and life in space.

“Space research is also critical for our understanding of the earth and its climate, and it invariably leads to spin-off effects. International facilities like Lofar foster strong cooperation across both scientific and cultural borders,” says Karin Markides, President of Chalmers.

“I believe LOFAR in particular will have great importance for our ability to handle very large amounts of data,” she adds.

During the inauguration ceremony at Onsala Space Observatory on Monday Minister of Education and Research Jan Björklund will take some of the first ever images of the sky with the Swedish LOFAR station. He will also visit the station together with around a hundred invited guests.



For more information see here. 

Thursday, September 1, 2011

LOFAR-UK Data School in Manchester

The LOFAR-UK data school is currently in progress in Manchester. You can see the programme and download some of the talk on the school website

Data school participants pose for a photo.

Hard at work learning about long baseline interferometry.

Monday, August 22, 2011

Alan Penny - We should talk about Aliens

In an article for the Guardian Science Blog, LOFAR-UK member Dr. Alan Penny from the University of St. Andrews, argues that we should think more about what to say to aliens if we ever do detect them.

"We Need to Talk about Aliens"

Alan is leading efforts to run test SETI observations using the LOFAR-UK station in stand-alone mode (ie. not connected to the rest of the LOFAR array).

LOFAR at the BAA Radio Astronomy Group 2011 General Meeting

At the 2011 General Meeting of the British Astronomical Association's Radio Astronomy Group (to be held 12th November 2011 at the Humfrey Rooms, Castilian Terrace, Northampton), the two keynote speakers have a LOFAR-UK link. They are Professor Paul Alexander, who is Head of the Astrophysics Group at Cambridge is the project leader for the UK contribution to the Square Kilometre Array (and a member of LOFAR-UK), and Dr Ben Stappers from Jodrell Bank who is Head of the Pulsar Science Working Group for the LOFAR radio telescope (and Technical Co-ordinator for LOFAR-UK). 


For more details see the BAA Radio Group website

Wednesday, August 17, 2011

Portsmouth College Work Experience Student Makes LOFAR-UK Poster

Last week at ICG, Portsmouth we hosted a local A-level student from Portsmouth College who made the below LOFAR-UK poster. We hope to use this poster locally in Hampshire to advertise the world class radio telescope on our doorstep.


Monday, August 8, 2011

Solar and Space Weather KSP Meeting



Members of the Solar and Space Weather Key Science Project for LOFAR met for a workshop in Aberystwyth on the west coast of Wales at the end of June.  The Workshop focused on the progress achieved so far in using LOFAR to obtain images of the solar corona, using the dynamic spectrum (2D plots of time versus frequency) to identify and mitigate interference and obtain measurements of interplanetary scintillation (the scintillation of radio sources due to density variations in the solar wind).  Results so far look encouraging and compare favourably with similar measurements taken on traditional instruments but much work remains to be done.  Participants also had time to enjoy the environs of Aberystwyth and it's various pubs and restaurants!


(with thanks to Richard Fallows for this report). 

Friday, August 5, 2011

LOFAR related postdocs at CEA Saclay (near Paris)

Another job advert for two postdoc positions at CEA Saclay near Paris working on detection of radio transients - including for the LOFAR Transient Key Project.

AAS Job Register posting (copied below).


Applications are invited for two postdoctoral positions in signal processing/data analysis for an initial period of 2 years, with the UnivEarthsS LabEx program.
The astrophysics division of CEA Saclay is offering two positions to work with Professor Stéphane Corbel on radio transients in close collaboration with Jean-Luc Starck. Over the next decade, a combination of increased sensitivity, larger field of view, and algorithmic developments will open up the time domain to a wide range of astronomical fields, from stellar flares and supernovae to neutron-star and black-hole births, quakes and instabilities. Radio astronomy is leading this effort and transient science is identified as a key goal for LOFAR (Europe), ASKAP (Autralia) and MeerKAT (South Africa), the precursor instruments of the major international SKA facility to be developed for 2020+.
The applicant will work in one of these related topics:
  -Transient search in one of the affiliated key projects: TKP (LOFAR), ThunderKAT (MeerKAT), VAST (ASKAP),
  - Optimization of current methods and development of near real-time detection pipelines,
  - Characterization of transients and identification at other wavelengths,
  - Image reconstruction from undersampled Fourier measurements.
Minimum qualifications include an undergraduate degree or higher in astronomy, physics, computer science, statistics or related field. The candidate must have a strong motivation in developing statistical methods and applying them in large international projects. CEA Saclay ( http://irfu.cea.fr/Sap/en/ ) is located 25km south of Paris, near Universities and other research centers. The astrophysics division gathers more than 150 faculty and staff members, studying a large range of astrophysical problems.
The positions are initially for two years and the starting dates should be between early Fall 2011 and early 2012. Ample funding for conferences, collaborations, personal equipment and publication is available. Applicants should submit by email resume, bibliography and a brief research plans to Stéphane Corbel (stephane.corbel@cea.fr) and Jean-Luc Starck (jstarck@cea.fr) and arrange for three reference letters to be sent as well before 31 August 2011.