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06 February 2020 | Story Michelle Nöthling | Photo Johan Roux
Symposium bridges the gap between students, staff, and management
Students from the UFS, UCLA and VUA shared on their collective experience within higher education at the colloquium.

The Unit for Institutional Change and Social Justice at the University of the Free State (UFS) united with the University of California, Los Angeles (UCLA), and the Vrije Universiteit Amsterdam (VUA) on the Bloemfontein Campus in a symposium discussing ‘Fragility and Resilience: Facets, Features and (Trans)Formations in Higher Education’. “It is really the only conference that brings together support staff, academic staff, students, and upper administration management, which includes vice-chancellors, rectors, presidents, and provosts,” said Dr Dionne van Reenen, Senior Researcher in the Unit for Institutional Change and Social Justice, and convener of the event.

Dr Van Reenen further explained that, when it comes to matters such as policy changes, contact between these various groups at a university is crucial. In general, upper management has very little contact with students. Students would rather approach academic staff. In turn, academic staff members are often reluctant to approach support staff, since support staff are already burdened with administrative tasks. But, Dr Van Reenen continued, all these stakeholders actually need to move closer to each other, since the Academic Project goal is the same: delivering excellent-quality graduates and producing new knowledge. With this in mind, the symposium programme specifically included panel presentations and discussions by academic as well as support staff and students. What emanated from these discussions was a rich variety of topics speaking to various aspects of fragility and resilience. The following are only a few excerpts from these engaging dialogues. 

Using counter-stories to narrate fragilities and resilience in higher education institutions in South Africa

Dr Fumane Khanare, Dr Ntombizandile Gcelu, and Pearl Larey – all three academic staff members in the UFS School of Education Studies, and Lihle Ndlovu, Head of Department for Business Studies at the uMfolozi TVET College – use narratives to interrogate fragility and resilience among black women in higher education. They wanted to go beyond surface conversations about how each was doing and decided to use critical race theory to question even their own stories through collaborative learning. They share, listen, question, and reflect, and as a result, create new narratives through counter-stories. “We are trying to explore our narratives,” Dr Khanare said, “not only as the outsiders, but as the insiders as well. From our background, we cannot ignore that we came here full of potential, but full of fragilities as well.” 

The ambiguity of change: The stories that South African student narratives tell 
Continuing the exploration of narratives, Dr Frans Kamsteeg from the Department of Sciences at VUA shared his research among students of the UFS who were part of the Leadership for Change programme. The programme, that came to an end in 2016, took UFS students through a process of leadership courses and training and included a trip to one of the external participating foreign universities. Dr Kamsteeg subsequently received several groups at the VUA and became interested in how these students engage in transformation processes at the UFS. Presenting seven vignettes of students’ narratives, Dr Kamsteeg revealed a tapestry of multivocality and fragility, and a meandering path of self-identity and transformation. “They learned a lot about academic citizenship and becoming responsible citizens,” Dr Kamsteeg added.

Keeping up with changing times: Student leaders, resilience, fragility, and professional development

Dr Marguerite Muller, Pulane Malefane, and Liezl Dick were all residence heads at the UFS. During the #FeesMustFall period, they realised that the role of student leaders had begun to change. They saw how these roles evolved and became interested in how student leaders became stakeholders and decision makers at the UFS. An interesting outcome from the arts-based research was that in the individual drawing exercise – in which students had to represent their lives as a winding river – fragility did not feature at all. Instead, the student leaders chose to depict sources of challenges and support, and how these factors built resilience. However, in the group exercise where students had to stage a puppet show, the stories revealed clear areas of fragility. Essentially, the students were willing to show fragility as long as they were fragile with others. “What we learned was that it is really important for student leaders to understand the complexity of their roles. Student leaders also need to learn and understand that it is okay to fail, that you need to grow and need to change, and that fragility in this sense is not necessarily a weakness,” Dr Muller 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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