This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: Using the Low Frequency Array (LOFAR), an international team led by Leiden University has produced the sharpest and most sensitive radio image of the sky ever made at low radio frequencies. The image reveals almost 63,000 radio sources, such as active galactic nuclei and star-forming galaxies, across a patch of sky about 25 times the area of the full moon.
The results have been accepted for publication in Astronomy & Astrophysics. The paper is currently available on the arXiv preprint server. The researchers have observed ELAIS-N1, a well-studied patch of the northern sky that contains many faint and distant galaxies.
The image is 20 times sharper than the previous most sensitive LOFAR image of this area of sky. For comparison, the resolution of the image is high enough to pick out a coin from about 10 kilometers (6 miles) away. At this resolution, the full image contains 8 billion pixels.
The data for the image were collected over 200 hours and amounted to 400 terabytes. For years, processing that much data for a single 8-billion-pixel image with radio telescopes at such high resolution was impossible, but improved calibration and data-reduction methods developed by the team and collaborators have cut the cost by more than a factor of 10 in the past few years. "The entire data set could be processed on Spider, the high-performance data-processing platform hosted at SURF in the Netherlands, in just a few months," says Jurjen de Jong, who led this work and is a postdoctoral researcher at Leiden Observatory and ASTRON.
The data have been made publicly available for the astronomical community, as much of the scientific value of the new data set will come from combining these observations with images of the same patch of sky taken by other telescopes at other wavelengths, like optical, infrared and X-ray observations. With this, astronomers can derive properties such as the distance and mass of each radio source detected in the new image. One of the dominant populations in the new LOFAR image is active galactic nuclei: the compact luminous centers of galaxies, powered by matter spiraling onto a supermassive black hole.
These can drive powerful jetlike outflows, which radio telescopes like LOFAR are especially well suited to detect due to the telescope's sensitivity to extended faint radio emission. On low-resolution images, distant galaxies and these black hole-driven radio jets are featureless blobs, and it's often hard to tell whether they consist of multiple galaxies or components. It's also hard to tell if this radio emission comes from a jet or from star formation across the galaxy.
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