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SPACE SCIENCES


        Ultra-sensitive radio images reveal




        thousands of star-forming galaxies




        in early Universe









          An international team of astronomers has published the most sensitive images of the Universe ever
          taken at low radio frequencies, using the International Low Frequency Array (LOFAR).







             he software needed to do this, specifically that which   “The combination of the high sensitivity of LOFAR and the
             handles the direction-dependent effects that would   wide area of sky covered by our survey – about 300 times
        Totherwise contaminate the images, goes back to the    the size of the full moon – has enabled us to detect tens of
        work of a former Rhodes University Postdoc Dr Cyril Tasse,   thousands of galaxies like the Milky Way, far out into the distant
        who remains an honorary research associate of the university,   Universe. The light from these galaxies has been travelling for
        and Prof. Oleg Smirnov, SKA (Square Kilometre Array) chair   billions of years to reach the Earth; this means that we see the
        in Radio Astronomy Techniques and Technologies at Rhodes   galaxies as they were billions of years ago, back when they
        University and head of the Radio Astronomy Research Group   were forming most of their stars.”
        at SARAO.
           By observing the same regions of sky over and over again
        and combining the data to make a single, very long exposure
        image, the international team has detected the faint radio glow
        of stars exploding as supernovae, in tens of thousands of
        galaxies, out to the most distant parts of the Universe. A special
        issue of the scientific journal Astronomy & Astrophysics is
        dedicated to 14 research papers describing these images and
        the first scientific results.
           “At LOFAR frequencies, observing the sky is like lying on
        the bottom of a swimming pool looking up, trying to make out
        patterns on the ceiling through the choppy water (the “water”
        being the ionosphere). Some very clever software was required
        to achieve this,” said Prof. Smirnov.
           A collaboration between the two academics led to a paper
        describing the maths (Smirnov & Tasse 2015, MNRAS), and
        to the DDFacet/killMS software packages that Dr Tasse had
        helped develop over the years. These packages are now at the
        heart of LOFAR data processing.
           “We quickly realised the same software can also be used to
        make MeerKAT images better, and several young researchers
        from Rhodes University and SARAO also became involved in
        this project with Dr Tasse,” explained Prof. Smirnov.
           Prof. Philip Best from the University of Edinburgh, UK, who   The image shows the deepest LOFAR image ever made, in the
        led the deep survey, said: “When we look at the sky with a   region of sky known as ‘Elais-N1’, which is one of the three fields
                                                               studied as part of this deep radio survey. The image arises from
        radio telescope, the brightest objects we see are produced by   a single LOFAR pointing observed repeatedly for a total of 164
        massive black holes at the centre of galaxies. However, our   hours. Over 80,000 radio sources are detected; this includes
        images are so deep that most of the objects in it are galaxies   some spectacular large-scale emission arising from massive
        like our own Milky Way, which emit faint radio waves that trace   black holes, but most sources are distant galaxies like the Milky
        their ongoing star formation.”                         Way, forming their stars.



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