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10 October 2022 | Story Edzani Nephalela | Photo Supplied
UFS CTL Teaching and Learning Conference
The University of the Free State (UFS) recently held its annual Teaching and Learning Conference. The theme of this year’s conference was Celebrating excellence in learning and teaching, coinciding with the Centre for Teaching and Learning’s (CTL) 10-year celebrations.

The University of the Free State (UFS) recently held its annual Teaching and Learning Conference which began with three pre-conference workshops on the Bloemfontein Campus on 12 and 13 September and ended with a virtual conference hosted from 14 to16 September 2022.

The aim of the UFS Learning and Teaching Conference is to provide academics and academic support staff the opportunity to showcase their innovative learning and teaching practices within different disciplines, as well as to advance the scholarship of teaching and learning at the institution. The theme of this year’s conference was Celebrating excellence in learning and teaching, coinciding with the Centre for Teaching and Learning’s (CTL) 10-year celebrations. During the pre-conference workshops, the focus was on blended learning, curriculum development, and student engagement. 

Dr Engela van Staden, Vice-Rector: Academic, opened the virtual conference on 14 September. She highlighted that universities contribute to the country’s economy through the type of graduates they produce. Therefore, the lecturers are vital; they must use various learning and teaching strategies and diligently perform their jobs to prepare students for the world of work. 

“We must stay current and grasp new advancements in our discipline and teaching methods. These techniques should also recognise students' diversity and multilingualism. With the new Language Policy, we should ensure that our dominant languages are used in academia in years to come. We are here to assist students in becoming employable graduates, and one of the elements that CTL has embarked on is the support we are receiving from them through various programmes, such as Enterprising your Degree: ePortfolio Development (EDED), which provides our students with platforms to market themselves in many professional fields,” Dr Van Staden said. 

Furthermore, Dr Van Staden emphasised the importance of research in enabling and empowering students to remain relevant. COVID-19 has also demonstrated the importance of the teaching approach and tested its efficacy in the classroom. This has resulted in the UFS moving towards becoming a digitalised institution. She stated that the institution has an agreement with the Free State Department of Health to conduct robotic surgery. She further explained that this is not about replacing academics, but about improving teaching and learning. 

In his welcoming address on the second day of the virtual conference, Prof Francis Petersen, Rector and Vice-Chancellor of the UFS, said that the reduction of the achievement gaps between a diverse group of people over the past decade demonstrates that the UFS is not just talking about innovation, equity, quality, and success, but about walking the talk – practically implementing what they profess, to make a real difference in the lives of the students, and to ensure the relevance of the institution.

“During the COVID-19 pandemic, the effective use of advanced data analytics was one of the contributing factors that enabled us to transition to an online learning and teaching environment successfully. It has allowed us to identify a lack of participation in online tuition, to reach out to individual students at risk, and respond with appropriate support mechanisms – thereby ensuring student success,” Prof Peterson added.

He further explained that Vision 130 commemorates 130 years of the UFS’ existence and is also a strategy to reposition the university for 2034 to ensure stability and clarity for planning and decision-making, while leaving scope for adaptation and agility. This vision will, among other things, promote 
• academic excellence, quality, and impact;
• maximum societal impact with sustainable relationships; and
• a diverse, inclusive, and equitable university.

Sizofunda Ngenkani: The Politics and Voice and Merit Principles in Higher Education

Prof Pearl Sithole, Vice-Principal: Academic and Research on the Qwaqwa Campus – one of the keynote speakers – asked, “What impact does our education have on the world? Consider our social enterprise. This demonstrates that there are stumbling blocks that prevent us from learning. We understand that education is a two-way street – capabilities and quality of access. Much has been done to demonstrate that education is more than a classroom endeavour, yet something must explain why education has failed to have the intended influence in societies. This is targeted at the interaction between society and education, and as academics, we are up to the task to ensure that these issues are solved through various programmes.”

Building future excellence through scholarship, collaboration, and action for impact

In his keynote address, Prof Francois Strydom, Senior Director: CTL, presented some of the strategies that have contributed to CTL’s success since its inception in 2012, despite some of the challenges that institutions of higher learning encountered. 

“Scholarships, collaboration, and action have always been instilled in us. We have integrated higher education research, organisational development, and management literature, considering international and national institutional viewpoints and settings. We acknowledge and promote faculty contributions and the dedication of teaching and learning managers who are supported by deans and academics to enhance the quality of teaching and learning,” said Prof Strydom.
He also emphasised the different programmes and research that contributed to this result. There are 223 national and 52 international conference papers, 288 research reports, two books, 93 articles/book chapters/peer-reviewed conference publications, and 35 postgraduate student supervisions.

Following the conference, the centre will be hosting its annual teaching and learning awards event on 12 October 2022 to recognise and award the excellent work done in learning and teaching at the UFS. 

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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