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12 December 2024 | Story Edzani Nephalela | Photo Supplied
Stefanus Scheepers
The recently dual-capped Stefanus Scheepers, Senior Admin Assistant Officer in the UFS Faculty of Education, says his success lies in mastering the art of balance.

Completing a master’s degree in record time is a remarkable achievement, but for Stefanus Scheepers, Senior Admin Assistant Officer at the University of the Free State Faculty of Education, it marked the beginning of an even more extraordinary academic journey. In a feat few could match, he earned two master’s degrees in just 20 months.

Scheepers’ first degree, a Master of Education specialising in Higher Education Studies, was conferred by the University of the Free State (UFS) on 9 December 2024. His thesis, ‘Effective Pedagogical Practices Teaching Assistants Use in Hybrid Teaching Modes: A Community of Inquiry Approach’, explored innovative teaching strategies in hybrid learning environments.

The second degree, a Master of Science by Research in Sustainable African Futures, was conferred through the Wits-Edinburgh Sustainable African Futures (WESAF) Doctoral Programme. His thesis, ‘Investigating the Perception, Adoption, and Utilization of Generative Artificial Intelligence in South African Higher Education Institutions’, examined the impact of generative artificial intelligence (GAI) on sustainable education in South Africa.

“My experience presenting workshops on GAI tools and its misuse by students sparked my research interest,” he explained. The resulting mini-dissertation shed light on the critical need for sustainable education practices in an era increasingly influenced by AI. This theme will continue as Scheepers embarks on a PhD at Wits University in 2025, exploring how to balance GAI’s benefits and risks in education.

Initially, Scheepers embarked on a part-time master’s degree in 2023 at the UFS while working full-time. “I hadn’t planned to complete two degrees,” he said, “but my supervisor’s encouragement and excellent guidance made completing the degree within a year seem possible.” Midway through, however, a nomination from the Dean and Vice-Dean of the Faculty of Education changed everything. The WESAF Doctoral Programme offered an opportunity that was too valuable to pass up, even though it added another degree to his demanding schedule.

“At first I was very hesitant, but my supervisor said that I would regret not taking it”, he said with a smile.

Time management does the trick

Balancing the demands of studying for two master’s degrees was no small feat. Scheepers chose to embrace meticulous time management, creating a schedule that integrated study and rest.

“Time management is not just about making a plan but sticking to it,” he emphasised. This structured approach allowed him to maximise productivity without burnout. “I must admit, working at night in your office did feel strange at first, but tranquil after a while.” Weekends included much-needed downtime, which helped him maintain resilience throughout.

Reflecting on this intense period, Scheepers attributes his success to cumulative skills gained over the years. “Every skill learnt in prior degrees was put to the test. The journey wasn’t easy, but intentionally applying these skills made the challenge rewarding.”

After nearly six years at higher education institutions – Scheepers’ career ambition is to transition into a lecturer role, with the hope of passing on his research and hands-on experience to a new generation of students.

When asked what he would share with prospective students at the UFS, Scheepers said, “The path to success isn’t always straightforward. I’ve experienced setbacks, even dropping out twice before finding my footing. But each challenge taught me resilience and determination. To all students: Keep going, even when the journey feels daunting. Every obstacle you overcome is a step closer to your goals. Remember, success is not about avoiding failure but learning and growing stronger with each experience. Stay focused, believe in yourself, and trust the process – you can do much more than you may realise.”

This remarkable dual graduation is not only a rare achievement in academia but also highlights Scheepers’ exceptional time management, strategic planning, and unwavering commitment to advancing the fields of education and sustainable futures.

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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