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19 October 2022 | Story Leonie Bolleurs
Dr Pieter du Toit
Dr Pieter du Toit, President of the Convocation, recently addressed more than 200 Convocation members at the Annual General Meeting.

What if you knew there was a body whose endeavours sought to be dynamic and engaging, promote excellence, welcome inclusion, and serve its alma mater?

One of the aims of the UFS Convocation – a body of more than 40 000 members – is to pay close attention to and engage on matters pertaining to governance, administration, and academic affairs at the University of the Free State (UFS).

This entity seeks to ensure that the research outputs of the university are communicated in a positive light, and that feedback is provided to ensure that the current academic programmes are adequate to enhance graduate employability. Among their goals is to provide a forum for unemployed graduates to share their skills, expertise, and abilities.

Furthermore, this body attempts to establish dialogue around social issues and ongoing transformation.

 

Fostering a spirit of belonging

According to Dr Pieter du Toit, President of the UFS Convocation, it is important for this structure that it stays relevant to its members and society and that it fosters a spirit of belonging. He recently addressed members on the UFS Bloemfontein Campus at the Annual General Meeting, the first to be held in the past two years. Besides the in-person attendance, the meeting was also attended by more than 200 members via livestream.

Dr Du Toit explained to members – which, according to legislation, include all persons who have obtained a formal qualification from the UFS, as well as all permanent academic staff members that the Convocation strives to promote a positive image of the UFS, advancing and safeguarding its reputation.

Also speaking at the AGM was the UFS Rector and Vice-Chancellor, Prof Francis Petersen. He reflected on the state of the UFS, talking about the past five years to date. He touched on matters pertaining to the core functions of the university, including teaching and learning, research and internationalisation, and engaged scholarship.

As stated in its vision, the UFS strives to be a research-led, student-centred, and regionally engaged university in Bloemfontein, the Free State, South Africa, and the continent.

In the past five years, the UFS’ framework of guidance has been the Integrated Transformation Plan, which endeavoured to emphasise social justice; the UFS Strategic Plan, the focus of which was to enhance the scope of transformation by following a holistic approach; and the Vice-Chancellor’s Strategic projects, aimed at creating a high-performance institution. “To be able to do what you need to do, you have to be at the top of your game,” said Prof Petersen.

In addition, the UFS has also been guided by the University Risk Management Committee and the Institutional Multi-stakeholder Group, which is a safe space that impacts the progression of an inclusive culture of belonging at the UFS.

Prof Petersen also referred to the 2020/2021 period during the COVID-19 pandemic. “There were three imperatives to which the UFS was committed during this period – the health and safety of staff and students, ensuring that no staff member or student was left behind, and successfully completing the 2020/2021 academic year,” stated Prof Petersen.

According to him, the university has engaged in different strategies to ensure that students were not left behind academically, and that committed staff did not overextend themselves. “We have dealt with it in such a way that our success rate for undergraduate studies has improved, which indicates the resilience of our students and the commitment of our staff,” he said.

The UFS is one of the nation's top universities for student success.

 

Optimising our research capacity

Two of the research successes of this year were an increase in research outputs and in the number of postgraduate students. The university is also working towards increasing the number of academic staff with PhDs, as well as its number of postdoctoral fellows. “We are looking at optimising our research capacity,” stated Prof Petersen.

Regarding engaged scholarship, Prof Petersen believes that if you cannot positively impact society through teaching and learning and research, you should ask why you exist as a university.

“We as a university is in a good place and I think you can be very proud of your alma mater,” he said.

For the way forward, the university is working on Vision130 (a strategy spanning over 12 years). “The vision will be quite bold, including goals for 75% of academic staff to have obtained their PhDs, a bigger focus on the postgraduate programme, and to be one of the top-five institutions in the country and one of the top-600 in the world. We will also reduce our student numbers to around 35 000, because we believe this is the number that we should be focusing on,” stated Prof Petersen.

“As members of the Convocation, I ask you to find a place in Vision130, to see how you can contribute to make this university a better institution than it is today,” he added.

Concluding his presentation, Prof Petersen told members of the Convocation, “You are immensely important to us as a university – you are the continuity between the past and the present as well as the future.”

Full-time UFS staff and alumni are welcome to contact the President of the Convocation with suggestions at convocation@ufs.ac.za

 

 

What is the Convocation?

  • It is important for the Convocation that it stays relevant to its members and society and that it fosters a spirit of belonging for alumni by keeping the communication channels with members open.
  • The Convocation strives to promote a positive image of the UFS, advancing and safeguarding its reputation.
  • The Convocation seeks to ensure that the research outputs of the university are communicated in a positive light, and that feedback is provided to ensure that the current academic programmes are adequate to enhance graduate employability.
  • Furthermore, this body attempts to establish dialogue around social issues and ongoing transformation.
  • In addition to promoting the institution's business and community interests, this structure aims to instil respect for the UFS.
  • Its goal is to instil in alumni a sense of responsibility, obligation, and accountability towards the community in general and to their alma mater in particular.

 Who is part of the Convocation?

  • All persons who have obtained a formal qualification from the UFS, as well as all permanent academic staff members.

 How often does the Convocation meet?

  • The Convocation sees to it that members meet at least once every two years.


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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