An international team of astronomers, including Marta Burgay, Delphine Perrodin and Andrea Possenti from the Italian National Institute for Astrophysics (INAF), identified for the first time the place of origin of a Fast Radio Burst (FRB), enigmatic radio signals lasting just a few milliseconds, which appear without warning in the sky. The discovery was made thanks to observations done with optical telescopes and radio telescopes and allowed to confirm the current cosmological model describing the distribution of matter in the universe.

It all starts on April 18th, 2015, when the typical signal of a FRB is detected by the Commonwealth Scientific and Industrial Research Organisation (CSIRO)’s 64-m Parkes radio telescope in Australia. "In a matter of hours - says Evan Keane, Project Scientist at the Square Kilometre Array Organisation, first author of the paper describing the discovery, published in the latest issue of the journal Nature - it has been issued an international alert and various telescopes around the world were involved in the search for the ‘result’ of that signal".

The INAF’s Sardinia Radio Telescope (SRT) was among them. "In April 2015, SRT was not in operation at 100% as it is today. Thanks to the great work of the INAF team for scientific validation of the radio telescope, SRT has, however, been able to attend promptly to the international campaign" explains Marta Burgay. "The SRT observations, combined with those of other radio telescopes single disc, have ruled out that the FRB is associated with a repetitive cosmic phenomenon".

Thanks to the ATCA's six 22-m dishes and their combined resolution, the team was able to pinpoint the location of the signal with much greater accuracy than has been possible in the past and detected a radio afterglow that lasted for around 6 days before fading away. This afterglow enabled them to pinpoint the location of the FRB about 1000 times more precisely than for previous events.

The team then used the National Astronomical Observatory of Japan (NAOJ)’s 8.2-m Subaru optical telescope in Hawaii to look at where the signal came from, and identified an elliptical galaxy some 6 billion light years away. "8 years after the identification of the first radio burst - explains Andrea Possenti - has finally been possible to establish the ‘place of birth’ of one of these events. Thanks to this, the identikit of the probable ‘parents’ may be limited to catastrophic events, highly energetic and not repetitive. "

The radio bursts are recorded prior to the higher frequencies of observation and only later to the lower ones: this phenomenon, a frequency-dependent dispersion, is caused by how much material it has gone through. "Until now, the dispersion measure is all we had. By also having a distance we can now measure how dense the material is between the point of origin and Earth, and compare that with the current model of the distribution of matter in the Universe" explains Dr Simon Johnston, co-author of the study, from CSIRO’s Astronomy and Space Science division. “Essentially this lets us weigh the Universe, or at least the normal matter it contains.”

In the current model, the Universe is believed to be made of 70% dark energy, 25% dark matter and 5% ‘ordinary’ matter, the matter that makes everything we see. However, through observations of stars, galaxies and hydrogen, astronomers have only been able to account for about half of the ordinary matter, the rest could not be seen directly and so has been referred to as ‘missing’.

"The good news is that our observations are consistent with the theoretical model: we found the missing matter" says Evan Keane. "It's the first time that a flash radio is used to conduct a measure cosmological." "The confirmation that at least a fraction of FRBs comes from very far distances - adds Andrea Possenti - certifies the opening of a new era in observational cosmology, in which the FRBs can play a complementary role to that of other cosmological indicators such as supernovae."

Looking forward, the Square Kilometre Array, with its extreme sensitivity, resolution and wide field of view is expected to be able to detect hundreds of FRBs and to pinpoint their host galaxies. A much larger sample will enable precision measurements of cosmological parameters such as the distribution of matter in the Universe, and provide a refined understanding of dark energy.

Original paper:

“The host galaxy of a fast radio burst”, E. F. Keane, S. Johnston, S. Bhandari, E. Barr, N. D. R. Bhat, M. Burgay, M. Caleb, C. Flynn, A. Jameson, M. Kramer, E. Petroff, A. Possenti, W. van Straten, M. Bailes, S. Burke-Spolaor, R. P. Eatough, B. Stappers, T. Totani, M. Honma, H. Furusawa, T. Hattori, T. Morokuma, Y. Niino, H. Sugai, T. Terai, N. Tominaga, S. Yamasaki, N. Yasuda, R. Allen, J. Cooke, J. Jencson, M. M. Kasliwal, D. L. Kaplan, S. J. Tingay, A. Williams, R. Wayth, P. Chandra, D. Perrodin, M. Berezina, M. Mickaliger & C. Bassa. Published in Nature on 25 February 2016.