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18 June 2024 | Story André Damons | Photo Suplied
SADoCoL
Betsie Human and Elandré Williams, analysts at the South African Doping Control Laboratory (SADoCoL) at the University of the Free State (UFS), will be involved in sample preparation, analysis and data processing at the upcoming Olympic and Paralympic Games in Paris, France.

Two staff members from the South African Doping Control Laboratory (SADoCoL) which is housed at the University of the Free State (UFS), have been selected to work at the upcoming Olympic and Paralympic Games, in Paris, France.

Elandré Williams and Betsie Human will support the Paris laboratory during both games. The Olympic Games will take place from 26 July to 11 August 2024 and the Paralympic Games from 28 August to 8 September 2024.

Williams will be involved in steroid profile analysis, which includes sample preparation, analysis and data processing by Gas Chromatography (GC) and Isotope Ratio Mass Spectrometry (GC-C-IRMS).

Part of the fight against doping 

“I am excited, optimistic and privileged to have been given this opportunity, but I have to say that I am also quite nervous as this is most probably the biggest sporting event of the year. Being a part of the fight against doping in sport remains a great responsibility as what we do directly impacts the athletes,” says Williams.

She says is looking forward to the entire experience, from doing what she loves on an international level, meeting other analysts in the field and being part of the fight against doping in sport on an Olympic level.

This is her first big international sporting event.

“I am also looking forward to learning from other experts in the field who have more experience and to witness the procedures and the manner in which the laboratory operates at this time where the sample numbers are extremely high with the added pressure to finalise results in short turn-around times. This is a great opportunity for growth, both individually and in my field of expertise, in the scientific and the doping control field.

“It will definitely be an advantage for me as an analyst to get exposure to how the entire analytical procedure is executed in another laboratory, as well as insight into possible new techniques and advancements that I will be able to apply back at SADoCoL. I also think this is a great way to improve my ideas, perspectives and level of expertise as I will be working and witnessing other scientific experts in the doping control field.”

Managing workflow and logistics at the Games

Human, who was an analyst at the 2010 Soccer World Cup in South Africa, says she is both nervous and excited for this experience. 

“I was a junior analyst at SADoCoL during the 2010 Soccer World Cup, but you cannot compare a single-sport discipline with a multisport discipline like the Olympic Games – The Games will be exponentially bigger.

“In the past 14 years doping control as a whole has grown significantly. New technologies, updated requirements, more sensitive testing methods have emerged – this will be a new experience,” says Human.

She will also be involved with sample preparation/analysis/data processing and says she is looking forward to seeing how the work-flow and logistics associated with the Games (massive amounts of samples/tight deadlines etc) is managed in a high through-put laboratory.

“I am of course also looking forward to meeting analysts from other labs – we are a bit secluded here at the southern tip of Africa. Collaboration between labs is tricky when your closest neighbour is in Europe.

“It is always eye-opening to see how other labs manage similar situations (even though an Olympics is quite different from normal routine days) – exposure to new techniques and alternative thinking has a way of elevating your own thought processes and it promotes growth – both as an individual and as a doping control analyst.”

Immensely proud

Hanno du Preez, Director of SADoCoL, says the laboratory personnel are immensely proud that two of their staff members were chosen to participate in this international event, which for many scientists is the peak of their career. Similarly, this provides acknowledgement to the staff members for the area in which they have been working.

“It is only a select few who are requested to provide service at the Olympic Games. The work conducted in an Olympic laboratory provides experience which cannot be gained elsewhere. The workload and fast-paced analysis is something which the personnel are used to, but the Olympics will bring a different dimension to the processes. 

“We are excited to see what Betsie and Elandré bring back, with regards to new viewpoints on processes which are similar in all anti-doping laboratories. Individual experiences uplift everyone in a regulated business unit such as SADoCoL and also ensures improved relationships between laboratories, as other anti-doping laboratories will be represented at the Games as well. We wish them all the best for the experience, and we thank them for being dedicated ambassadors for SADoCoL and the UFS.”

News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

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