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08 April 2025 | Story Precious Shamase | Photo Supplied
Sifiso Banda
Sifiso Banda balances library duties and academic goals, showcasing innovation and resilience at the UFS Qwaqwa Campus.

In the heart of the University of the Free State Qwaqwa Campus, Sifiso Banda's story is one of ambition, and the seamless fusion of seemingly disparate worlds. Balancing his role as Senior Assistant Officer: Circulations and TK Mopeli Makerspace in the library with the rigorous demands of a BSc Honours Degree in Computer Science, Banda has not only excelled but also inspired.

 

Overcoming challenges fuelled by dreams

"Computer Science is my primary passion," Banda explains, his voice resonating with determination. "Being in academia allows me to interact with ever-evolving technologies. I love problem-solving and creating new ideas to help my community. “However, the path was far from easy. Juggling a demanding job with intense academic pressure led to sleepless nights and near-burnout. "It required immense professionalism in time planning and management," he confesses. "I almost gave up, but the unwavering support of my colleagues and supervisors kept me going."

Banda's journey is a testament to the power of perseverance, fuelled by a deep sense of responsibility and gratitude. "I had to remind myself daily who I was doing this for," he says, his voice filled with emotion. "My late mother used her last savings to register me for university, giving me an opportunity she never had. That memory pushed me through the pain."

 

From theory to practice: Innovating library technology

His unique position within the library has provided an unexpected synergy with his Computer Science studies. "I saw a gap to bridge theory with practical application," Banda explains. "I want to use my tech skills to innovate and make education engaging, developing systems and apps that simplify student life."

He discovered that library science extends far beyond traditional book management. "It's not just borrowing and cataloguing," he says. "There are diverse career paths for a computer scientist, such as systems librarian."

Banda's practical application of his computer science knowledge is evident in his daily work. He plays a key role in managing and configuring the library's technology, including RFID self-check machines and automated chutes. Notably, a YouTube demonstration he created showcases his ability to bridge the digital divide for library users.

The most daunting challenge was his mini-dissertation. "It demanded immense time, often encroaching on my work hours," he recalls. "Balancing coding, documentation, and assisting patrons was incredibly difficult."

 

Evolving technology and support

His fascination with computer science stems from its dynamic nature. "Technology evolves daily," he says. "I'm particularly drawn to artificial intelligence and machine learning, as I envision a future where everything is digitised. My childhood dream was to build robots that could assist in households."

Banda credits several mentors for their profound impact on his academic journey. Prof Richard Ocaya, Prof Lehlohonolo Koao, Dr Andronicus Akinyelu, and Adebola Musa all provided crucial guidance and support. He also acknowledges the invaluable emotional support from Nonhlanhla Moleleki, a counsellor, and Khethiwe Bhiyo, his academic adviser. "The community at large played a vital role," he emphasises.

His advice to students working while studying is simple yet powerful: "Everything is possible with consistency, persistence, determination, and dedication. Keep focused, no matter how long it takes."

His research project, an online dining hall purchasing system, exemplifies his commitment to community-driven innovation. "It has reduced wait times and queues across our campuses," he says proudly.

Looking ahead, Banda plans to pursue a master's degree, aiming to combine his library experience with his technical expertise. "I envision libraries becoming increasingly digitised, and I want to be part of that evolution," he states.

The skills he gained – time management, multitasking, collaboration, and the courage to seek help – will be invaluable in his future endeavours. "Most importantly, believe in yourself," he concluded.

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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