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22 November 2024 | Story Lunga Luthuli | Photo Supplied
International Audit Week 2024
UFS students at Coventry University’s International Audit Week, marking a historic first for South African and Global South universities participating in this prestigious global accountancy gathering.

In a significant first for any university in South Africa and the Global South, five students from the University of the Free State (UFS) participated in Coventry University’s prestigious International Audit Week (IAW). This global gathering of top accountancy students from various countries took place from 28 to 30 October 2024 in England.

The UFS School of Accountancy earned the invitation through a Collaborative Online International Learning (COIL) project initiated earlier this year. Prof Frans Prinsloo, Vice-Dean for Learning, Teaching, Innovation, and Digitalisation in the Faculty of Economic and Management Sciences, said, “Our participation signifies a major step in our internationalisation strategy. We were the first university from the Global South to attend, showcasing our students’ exceptional skills and fostering global collaboration.”

Trailblazing students

The selected students – Charlene Black, Twisiso Mathonsi, Heike de Nysschen, Charlize Oosthuizen, and Boitumelo Radebe – are among the top performers in the Postgraduate Programmes in Chartered Accountancy (PGCA). These future chartered accountants were chosen based on their stellar mid-year results, as final marks were unavailable before the trip.

Black expressed her excitement, stating, “Being selected to represent UFS at such a prestigious event was a tremendous privilege. It reinforced my decision to pursue the CA(SA) qualification and inspired me to make impactful contributions to the profession.”

Mathonsi, equally thrilled, reflected on the significance of the experience, saying, “Attending IAW was a dream come true. It validated my hard work and gave me a unique opportunity to engage with global perspectives on auditing.”

International insights and learnings

The week’s highlights included interactive sessions and industry tours. Black found the visit to Morgan Motors particularly inspiring, noting, “Witnessing their manufacturing process and reliance on paper-based job cards was fascinating. It was a reminder of the diverse practices within industries globally.”

Mathonsi recalled the collaborative activities, particularly a group project at Shakespeare’s birthplace. “It was both fun and insightful, emphasising teamwork across cultural and linguistic differences,” he said.

The students were exposed to cutting-edge developments in auditing, including the integration of artificial intelligence. These insights deepened their understanding of global industry trends and standards, such as the IFRS Foundation Standards and International Standards of Auditing, and highlighted differences in professional qualifications and practices between South Africa and the UK.

Sponsorship and support

This historic participation was made possible by the generosity of sponsors, who contributed over R250,000. The Raubex Group led with R150,000, followed by Rain Chartered Accountants (R50,000), Core Bloemfontein (R20,000 and K-Way jackets), the South African Institute of Chartered Accountants (R20,000), and Interstate Bus Lines (R10,000).

Prof Prinsloo emphasised the importance of such collaborations: “Our visionary sponsors recognised the immense benefits of this initiative for our students. Their support underscores the value they place on nurturing future leaders.”

Global impact and future plans

The experience not only elevated the students’ aspirations but also boosted the UFS’s international reputation. “Our students’ technical competence often surpassed that of their peers, cementing UFS as a global player in accountancy education,” Prof Prinsloo noted.

Looking ahead, the School of Accountancy plans to expand its international partnerships and aims to host the International Audit Week in Bloemfontein by 2026. For Mathonsi, the advice to future students is clear: “Work hard even when no one is watching; dedication always pays off.”

The UFS delegation’s success at IAW exemplifies the university’s commitment to excellence, global engagement, and producing graduates poised to make a difference on international and local platforms.

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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