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18 November 2024 | Story Leonie Bolleurs | Photo Tania Allen
Business School Partnership 2024
Prof Per Assmo from University West, Sweden and Prof Anthea Rhoda from the UFS signed a Memorandum of Understanding that will develop academic cooperation across fields such as research, student and academic exchanges, and collaborative projects.

The University of the Free State (UFS) has signed a Memorandum of Understanding (MOU) with University West, Sweden. Held at the UFS Business School on the Bloemfontein Campus, the event saw the signing of the agreement by Prof Anthea Rhoda, acting UFS Vice-Chancellor and Principal, and Prof Per Assmo, Deputy Vice-Chancellor for Internationalisation at University West. The partnership aims to develop academic cooperation across fields such as research, student and academic exchanges, and collaborative projects.

This MOU opens the door to a wide range of collaborative initiatives, including academic and researcher exchanges for the purposes of teaching, conducting lectures, conducting research, and exchanging expertise. Additionally, the MOU includes student exchange programmes, joint research projects, and the shared hosting of seminars and conferences.

Prof Rhoda shared her enthusiasm to incorporate work-integrated learning (WIL) more widely at the UFS. “We are looking at work-integrated learning as an extension of engaged scholarship. It is something that we're looking forward to expanding,” she said.

Building a connected community

Prof Assmo explained that their institution, though small, has a unique approach that focuses on both production technology and work-integrated learning – a teaching model that goes beyond internships to provide students with practical, hands-on experience. "For us, WIL is a research field and academic discipline in its own right," he said.

University West is also the only university in the world to offer a PhD specifically in WIL, a programme it spent 20 years developing.

“We want to collaborate with South Africa as a strategic partner,” he said. The University West is already actively working with several South African universities, including the UFS, the Central University of Technology, the University of the Western Cape, and Tshwane University of Technology. “This would be the core for us, where we collaborate and find different forms within research and education, not restricted to any faculty or field as such.”

His vision also includes forming a larger ‘Nordic hub’ of connections across Sweden, Norway, and the European Union, along with a ‘regional hub’ in Bloemfontein. This way, universities can share ideas and resources to build a stronger, more connected community for the future.

A need for work-integrated learning

A working example of this partnership between University West and the UFS is the collaborative focus on integrated learning between Prof Liezel Massyn, Associate Professor in the UFS Business School, and Prof Kristina Areskoug Josefsson, Professor in Work-integrated Learning and Health Science from University West. They have a mutual commitment to improve educational practices through international partnerships and to advance integrated learning strategies. Together, they have already co-authored a research article and presented their findings at five conferences this year.

Prof Massyn said she realised that there is a need for work-integrated learning, specifically in the UFS Business School. “Initially, I thought our students were working, so they didn't need the work-integrated learning component. I then realised it could actually add a lot more value.”

Prof Nicolene Barkhuizen, Director of the UFS Business School, highlighted how this venture aligns with the university’s Vision 130, which aims to expand the UFS’ global footprint. “This partnership is an optimisation of the collaboration to contribute to Vision 130, expanding our reach globally while bringing practical value locally. We are looking forward to a very fruitful collaboration,” she said.

Speaking on behalf of the Faculty of Economic and Management Sciences, acting Dean Prof Frans Prinsloo discussed the potential for future projects. “Now that we have this collaboration agreement, there are many opportunities we can explore further,” he stated.

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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