Gamma-ray bursts (GRBs) are the most luminous explosions in the cosmos. These explosive events last several seconds and during that time they they release in 10 seconds in gamma rays as much energy as the sun will emit in its 10-bilion year life. Such extreme amounts of energy can only be released during catastrophic events like the death of a very massive star, or the merging of two compact stars, and are accompanied by an afterglow of light over a broad range of wavelengths (or equivalently energies), that fades with time.
While it has been decades since the discovery of the first GRB, some of their fundamental traits remain a puzzle. An international team of more than 300 researchers, including IDIA researchers, Prof Patrick Woudt from the University of Cape Town and IDIA-funded MSc student Mr Reikantseone Diretse, has gained further insight into the physical processes at work during these events. They accomplished this through the observation of a GRB with an afterglow featuring the highest energy photons ever detected in these events: photons a trillion times more energetic than visible light.
On January 14, 2019, researchers detected GRB 190114C. GRB 190114C is unique in that researchers were able to observe for the first time in its afterglow emission photons with teraelectronvolt (TeV) energies, using the MAGIC telescope in the Canary Islands. This emission of TeV photons was 100 times more intense than the brightest known steady source at TeV energies, the Crab Nebula. As expected, the very high energy emission faded quickly in about half an hour after the event onset, while the afterglow emission in other parts of the spectrum persisted for much longer.
The discovery triggered an extensive campaign of observations across the electromagnetic spectrum, mobilising more than 20 observatories and instruments around the world. This collaborative effort allowed researchers to gather the most information ever collected about a GRB, capturing the evolution of the GRB afterglow emission across 17 orders of magnitude in energy.
Prof Woudt and Mr Diretse were part of a team responsible for tracking the emission of radio waves in the afterglow of GRB 190114C. The team used the new MeerKAT radio telescope in South Africa to record the emission. Whilst gamma rays are very high energy photons, radio waves are found at the other energy end of the electromagnetic spectrum. “The rapid response of the MeerKAT telescope to observe this extreme stellar explosion, combined with its excellent sensitivity, has allowed us to detect the radio afterglow within 24 hours of the explosion.” Prof Woudt explained.
Mr Reikantseone Diretse continues to monitor the radio afterglow of this event using MeerKAT. Mr Diretse says: “The recording of TeV energies for GRB190114C and its continued monitoring with radio telescopes such as MeerKAT helps us to untangle the high energy astrophysics of these exciting transient events. Being part of such a discovery was ecstatic and highly motivating.”
Reikantseone’s study is supported by a postgraduate scholarship from the Inter-University Institute for Data Intensive Astronomy (IDIA). The research cloud computing infrastructure of IDIA contributed towards the fast analysis of the MeerKAT observations of GRB190114C. Prof Russ Taylor, Director of IDIA, says: “This amazing scientific achievement underscores the importance of the ability of South African researchers to rapidly analyze large MeerKAT data sets with the data intensive research cloud developed at IDIA.”
Rob Adam, Managing Director of the South African Radio Astronomy Observatory (SARAO) said: “Once again we see the potential of the MeerKAT telescope in finding interesting and possibly new astrophysical phenomena, as well as the power of the multi-wavelength approach to the analysis of observations.
A collaborator on the MeerKAT team, Prof. Kouveliotou of George Washington University in the USA, concludes, “MAGIC (the TeV photon detector) opened up a new window on GRB research, and we are looking forward to understanding their physics and true energy release with more detections in the future”.
The findings were announced in the study, “Inverse Compton emission revealed by multi-wavelength observations of a gamma-ray burst,” published today (21 November 2019) in the journal Nature.
Photo: Mr Reikantseone Diretse in front of the MeerKAT observation of GRB190114C (encircled) in the IDIA Visualisation Lab. (credit: Siphelo Funani).
Prof Patrick Woudt
Head of Department: Astronomy
Mr Reikantseone Diretse
Department of Astronomy & Inter-University Institute for Data-Intensive Astronomy