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23 October 2024 | Story Lunga Luthuli | Photo Kaleidoscope
EDSA Awards - 2024
At the 2024 EDSA Prestige Awards (from left): Temba Hlasho, Executive Director of Student Affairs; Siphilangenkosi Dlamini, Student of the Year; and Prof Anthea Rhoda, acting Vice-Chancellor and Principal.

The 2024 Executive Director of Student Affairs (EDSA) Prestige Awards, hosted by the University of the Free State (UFS) on 12 October on South Campus, was a celebration of student excellence, leadership and holistic development. The third annual event recognised exceptional achievements across academia, sport, community engagement and innovative activities, aligning with the university’s broader Vision 130 strategy, which emphasises excellence, innovation and social impact.

Prof Anthea Rhoda, Acting Vice-Chancellor and Principal of UFS, highlighted how the awards reflect the university’s commitment to nurturing well-rounded students who are capable of excelling on the global stage. She emphasised that categories like ‘Most Innovative Fundraising Activity,’ ‘Best Undergraduate’ and ‘Best Sportsman’ embody the values of Vision 130.

“The awards encourage students to strive for excellence in several areas of their student experience, similarly to how UFS aspires to achieve excellence in various spheres where it is a role player,” she said.

The decision to host the ceremony on South Campus marked a significant step towards inclusivity across all UFS campuses. Prof Rhoda noted that this choice reiterated UFS’s identity as “one university with three campuses”. She expressed optimism for the future of South Campus, calling it a hub for academic and student activities, and signalling its potential to host even larger events in the future.

Through its Division of Student Affairs, UFS plays a pivotal role in supporting students in both academic and extracurricular pursuits. According to Prof Rhoda, the university has formulated a strategic framework that emphasises student success, well-being and development. She highlighted that students are given ample opportunities to excel, whether through academic support systems or through initiatives like entrepreneurial programmes and sports infrastructure. This well-rounded support system equips UFS students with the tools to compete globally, both academically and in extracurricular endeavours.

Among the many students honoured was Mthi Mthimkhulu, a first-year who is studying towards a Bachelor of Arts degree specialising in Language Practice. The rising 400-metre sprint star participated at the South African Under-23 Championships in Pretoria earlier this year, finishing with a time of 46 seconds, as well as in the African Athletics Championships in Douala, Cameroon, logging a time of 46.50.

On the night of the EDSA Prestige Awards, Mthimkhulu walked away with three gongs: the Club Sports Star of the Year, Kovsie National Sports Representative of the Year, and Sportsman of the Year.

The big winner on the night was Siphilangenkosi Dlamini, who took home the Student of the Year award. Dlamini, a student and research assistant at the Centre for Teaching and Learning, is also the Provincial Chairperson of the BRICS Student Commission in the Free State. Along with being named Student of the Year, he also took home a cash prize of R1 500.

“Winning the Student of the Year award is an incredible honour, both personally and professionally,” Dlamini said. “It represents the culmination of years of dedication to leadership, academic excellence and social impact.”

His leadership extends beyond UFS, with initiatives focused on decolonising education and youth entrepreneurship. Dlamini also leads the Initiative for Creative African Narratives (iCAN) project, which empowers African youth to reclaim their narratives by writing in their own languages. This initiative, which now includes 10 South African languages, exemplifies his dedication to fostering innovation and cultural pride among African youth.

The 2024 EDSA Prestige Awards not only celebrated excellence but also reinforced UFS's dedication to creating a vibrant student life that enhances leadership, personal growth and community engagement, in line with Vision 130.

Click to view documentClick here for the list of all the categories and the winners.

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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