Radio astronomers bypass disturbing Earth's atmosphere with new calibration technique

Published on 06 May 2024

An international team of researchers led by astronomers from Leiden University (the Netherlands) has produced the first sharp radio maps of the universe at low frequencies. Thanks to a new calibration technique, they bypassed the disturbances of the Earth's ionosphere. They used the new method to study plasmas from ancient black hole bursts. Potentially, the technique might be useful for finding exoplanets that orbit small stars. The researchers report their technique in the journal Nature Astronomy.

The technique allowed astronomers to take clear radio images of the universe at frequencies between 16 and 30 MHz for the first time. This was thought to be impossible because the ionosphere, at about 80 kilometers above the Earth, interferes with observations at these frequencies.

The researchers used the LOFAR telescope in Drenthe, the Netherlands. This is currently one of the best low-frequency radio telescopes in the world. To test their technique, they studied a number of galaxy clusters that had previously only been studied in detail at higher frequencies.

Old versus new. Left shows an image of a piece of sky observed with the hitherto best calibration technique. Right shows the same piece of sky with the new technique. More detail is visible, and what were once large, blurry patches now appear as single points. (c) LOFAR/Groeneveld et al.

Glasses

Thanks to the new images, it appears that the radio emission from these clusters is not evenly distributed across the entire cluster, but rather there is a spot pattern. "It's like putting on a pair of glasses for the first time and no longer seeing blurred," said research leader Christian Groeneveld (Leiden University, the Netherlands).

The motivation for the research was that at high frequencies, around 150 MHz, many improvements in calibration had already been made in recent years. "We hoped that we could also extend this technique to lower frequencies, below 30 MHz," says the originator of the idea, Reinout van Weeren (Leiden University). "And we succeeded."

At the moment, the researchers are processing more data in order to map the entire northern sky at the lower frequencies.

According to the researchers, the new calibration technique makes it possible to study phenomena that were previously hidden. It might be used to detect exoplanets orbiting small stars. And, Groeneveld concludes, "There is, of course, a chance that we will eventually discover something unexpected.

Scientific paper

Characterisation of the decameter sky at sub-arcminute resolution. By: C. Groeneveld, R.J. van Weeren, E. Osinga, W.L. Williams, J.R. Callingham, F. de Gasperin, A. Botteon, T. Shimwell, F. Sweijen, J. de Jong, L.F. Jansen, G.K. Miley, G. Brunetti, M. Brüggen & H.J.A. Röttgering. In Nature Astronomy, 6 May 2024. [original | preprint (pdf)]

About NOVA

The Netherlands Research School for Astronomy (NOVA) is the alliance of the astronomical institutes of the universities of Amsterdam, Groningen, Leiden, and Nijmegen. The mission of Top Research School NOVA is to carry out frontline astronomical research in the Netherlands, to train young astronomers at the highest international level, and to share its new discoveries with society. The NOVA laboratories are specialized in building state-of-the-art optical/infrared and submillimeter instrumentation for the largest telescopes on earth.