Astronomers detect hundreds of thousands of previously unknown galaxies

A major new radio sky survey has revealed hundreds of thousands of previously undetected galaxies, shedding new light on many research areas including the physics of black holes and how clusters of galaxies evolve. An international team of more than 200 astronomers from 18 countries, including staff from the University of Manchester's Jodrell Bank Centre for Astrophysics, has published the first phase of the survey at unprecedented sensitivity using the Low Frequency Array (LOFAR) telescope.

Radio astronomy reveals processes in the Universe that we cannot see with optical instruments. In this first part of the sky survey, LOFAR observed a quarter of the northern hemisphere at low radio frequencies. Today (19th February 2019), around ten percent of that data is being made public. It maps three hundred thousand sources, almost all of which are galaxies in the distant Universe; their radio signals have travelled billions of light years before reaching Earth.

The University of Manchester team that have contributed to the results from this survey includes Dr. Neal Jackson, Prof. Anna Scaife, Dr. Alex Clarke, Dr. Rob Beswick, Dr. Eskil Varenius and Prof. Michael Garrett.

Prof. Michael Garrett, Director of Jodrell Bank Centre for Astrophysics commented that "It’s great to see LOFAR producing these huge panoramic images of the sky, and for the UK astronomical community to be so closely involved in this success. We’re looking forward to studying these new sources in much more detail and higher resolution with e-MERLIN and the European VLBI Network."

Black holes

Huub Röttgering, Leiden University (The Netherlands) says: “If we take a radio telescope and we look up at the sky, we see mainly emission from the immediate environment of massive black holes. With LOFAR we hope to answer the fascinating question: where do those black holes come from?”

Philip Best, University of Edinburgh (UK), adds: “What we do know is that black holes are pretty messy eaters. When gas falls onto them they emit jets of material that can be seen at radio wavelengths. LOFAR has a remarkable sensitivity which allows us to study black holes even in galaxies which only have jets on very small scales. We have discovered that these jets are present in all of the most massive galaxies, which means that their black holes never stop eating.” The energy output in these radio jets plays a crucial role in controlling the conversion of gas into stars in their surrounding galaxies.

Clusters of galaxies

Clusters of galaxies are ensembles of hundreds to thousands of galaxies. It has been known for decades that when two clusters of galaxies merge, they can produce radio emission spanning millions of light years. This emission is thought to come from particles that are accelerated during the merger process. New research using LOFAR is beginning to show this emission at previously undetected levels from clusters of galaxies that are not merging. This means that there are phenomena other than merger events that can trigger particle accelerations over huge scales.

High-quality images

LOFAR produces enormous amounts of data. The equivalent of ten million DVDs of data has been processed to create the low-frequency radio sky map. The survey was made possible by a mathematical breakthrough in the way we understand interferometry.

A large international team has been working to efficiently transform the massive amounts of data into high-quality images. Pre-processing of the LOFAR data within the archives in the Netherlands, Germany and Poland reduces the size of the huge LOFAR datasets before the data are transported to member institutions for the images to be made.

Most of the images for the first data release were made on the University of Hertfordshire's high-performance computing facility, supported by Science and Technology Facilities Council (STFC) funding for LOFAR-UK. "Making these images in a completely automated way has required a lot of investment in software development as well as new computer hardware," explained Martin Hardcastle, University of Hertfordshire. "But the payoff is the unprecedented quality of the data, which will allow us to study the evolution of galaxies and their activity in more detail than ever before."

LOFAR

The LOFAR telescope is unique in its capabilities to map the sky in fine detail at metre wavelengths and is considered to be the world’s leading telescope of its type. The European network of radio antennas spans
seven countries and includes the UK station at STFC RAL Space’s Chilbolton Observatory in Hampshire. The network is operated by ASTRON in The Netherlands.

Professor Chris Mutlow, Director of STFC RAL Space said: “UK scientists are at the heart of this international project to better comprehend our Universe. This new survey has already mapped thousands of galaxies, helping us understand how these galaxies and black holes evolve. The LOFAR-UK station at RAL Space’s Chilbolton Observatory will be celebrating its 10th anniversary next year, so it is timely to see such fascinating results from this radio sky survey. This is something we are extremely proud to support.”

The signals from all of the stations are combined to make the radio images. This effectively gives astronomers a much larger telescope than it is practical to build - and the bigger the telescope, the better the resolution. The first phase of the survey only processed data from the central stations located in the Netherlands, but UK astronomers are now re-processing the data with all of the international stations to provide resolution twenty times better. "We will be able to identify hidden black holes, study individual clouds of star formation in nearby galaxies, and understand what jets from black holes look like in the most distant galaxies," says Leah Morabito, University of Oxford. "This extra phase of the survey will be truly unique in the history of radio astronomy, and who knows what mysteries we'll uncover?"

The next step

A special issue of the scientific journal Astronomy & Astrophysics is dedicated to the first 26 research papers describing the survey and its first results. A quarter of the papers were led by UK scientists. The papers were completed with only the first two percent of the sky survey. “This sky map will be a wonderful scientific legacy for the future. It is a testimony to the designers of LOFAR that this telescope performs so well”, says Carole Jackson, Director General of ASTRON.

The team aims to make sensitive high-resolution images of the whole northern sky, which will reveal 15 million radio sources in total. “Just imagine some of the discoveries we may make along the way. I certainly look forward to it”, says Jackson.

The galaxy cluster Abell 1314 is located in Ursa Major at at distance of approximately 460 million light years from earth. It hosts large-scale radio emission that was caused by its merger with another cluster. Non-thermal radio emission detected with the LOFAR telescope is shown in red and pink, and thermal X-ray emission detected with the Chandra telescope is shown in gray, overlaid on an optical image.
Credit: Amanda Wilber/LOFAR Surveys Team/NASA/CXC
This image shows how the LOFAR radio telescope opens a new view of the universe. The image shows galaxy cluster Abell 1314. In shades of grey, a piece of the sky can be seen as we know it in visible light. The orange hues show the radio emitting radiation in the same part of the sky. The radio image looks completely different and changes our assumptions about how galaxies arise and develop. These objects are located at a distance of approximately 460 million light years from earth.
In the middle of every galaxy there is a black hole. When matter falls into it, an unbelievable amount of energy is released and electrons are ejected like a fountain. These accelerated electrons produce radio emission that can extend over gigantic distances and is not visible at optical wavelengths.
Credit: Rafaël Mostert/LOFAR Surveys Team/Sloan Digital Sky Survey DR13
This image shows M51, also known as the Whirlpool Galaxy. It is 15-35 million light years from Earth and around 60,000 light years in diameter. At the centre of the spiral galaxy there sits a supermassive black hole. With the LOFAR data (yellow and red hues), we can see that the spiral galaxy and its companion are interacting because there is a bridge of emission joining them.
Credit: Sean Mooney/LOFAR Surveys Team/Digitized Sky Survey

Additional Info

More images are available on the LOFAR Surveys website gallery.

Rafaël Mostert (Leiden University) has made a website where you can explore the most common shapes of the 320,000 radio objects that the LOFAR Survey has detected so far.

Further information about the survey can be found on the LOFAR Surveys team website.

Share this page

 

▲ Up to the top