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14 February 2025 | Story Charlene Stanley | Photo Kaleidoscope Studios
Prof Hester Klopper
Prof Hester Klopper, newly appointed Vice-Chancellor and Principal of the University of the Free State.

Re-discovering Our Institutional Heart was the theme of the official opening address of the University of the Free State (UFS) presented by newly appointed UFS Vice-Chancellor and Principal, Prof Hester Klopper, as she addressed UFS staff members in the Odeion Auditorium on the Bloemfontein Campus.

Prof Klopper sketched the current global, national, and local contexts that have affected higher education in general, and the UFS in particular, giving an overview of where the institution has come from, where it currently is, and where it is going. She emphasised the need to focus on the qualities and research areas for which the university has become well known, and to stay true to the values and principles set out in its Vision 130.

“Vision 130 illuminates our way into the future – expounding how we want to establish ourselves as a top-tier university that is continually extending its influence and impact locally, regionally, and globally,” she said.

 

The institutional heart

Prof Klopper referred to the image of a heart that is reflected in the UFS marketing logo, encouraging staff to rediscover what lies at the heart of the institution, and what sets it apart.

“A university such as ours inevitably forms and moulds the lives and characters of the people associated with it; and in turn, it too is shaped and transformed by those who have graced its campuses over the decades. It too has a character. And it certainly has a heart.”

She elaborated on the metaphorical meanings locked up within the concept of a heart, touching on how it symbolised vitality, flow, and energy, interconnectedness, and a sense of belonging. She also highlighted its significance as a beacon of resilience.

“It is associated with courage and steadfastness. Over the past 120 years, the University of the Free State has prevailed despite adversity and has managed to constantly reinvent itself in order to remain relevant, without losing sight of the values in which it is anchored,” she said.

 

Priorities for tenure

One of the broad focus areas that Prof Klopper identified as a priority during her term was establishing the UFS as an innovation and entrepreneurial ecosystem. “This includes advancing transdisciplinary research, moving towards identifying two to three core research themes that address local, regional, and global challenges, and strengthening our unique offering,” she said.

Another focus area will be working towards systemic sustainability, which will include a disciplined approach towards financial management, as well as revision and optimisation of the academic model. She also indicated that internationalisation will be a core theme during her tenure, as will the establishment of the UFS as a first-choice employer and a magnet for talent. To this end, she announced the establishment of a VC Strategic Personnel Fund to grow and attract the best academic talent.

 

Innovation through connection

Prof Klopper concluded that the heartbeat of the UFS lies in innovation through connection.

For her, innovation is expressed in the university’s cutting-edge programme content, its focus on creating a culture of entrepreneurship, optimisation of the academic model, and finding new ways to diversify income streams. On the other hand, connection is reflected in heightened internationalisation, expansive collaborative networks, and a renewed focus on transdisciplinary research and real societal impact through engaged scholarship.

“My sincere wish is that each one of you will rediscover this heartbeat and that it will inspire you this year to take our great institution to even greater heights,” she said.

 

Click to view document Click here for the official opening speech.

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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