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21 August 2025 | Story Tshepo Tsotetsi | Photo Tshepo Tsotetsi
EMS Womens Function
From the left: Prof Brownhilder Neneh, Vice-Dean of the Faculty of Economic and Management Sciences; Prof Hester C. Klopper, Vice-Chancellor and Principal of the UFS; Simone Williams, Faculty Manager; and Dr Celeste Campher, Senior Lecturer in the Faculty of Economic and Management Sciences, at the Women’s Function held on the Bloemfontein Campus on 18 August.

The University of the Free State’s (UFS) Faculty of Economic and Management Sciences recently hosted a Women’s Function on the UFS Bloemfontein Campus – an event that paid tribute to women’s leadership in academia during Women’s Month. The gathering, held on 18 August 2025, was marked by a historic conversation with Prof Hester C. Klopper, UFS Vice-Chancellor and Principal, who earlier this year became the first woman to lead the university in its 121-year history.

The function brought together women academics and professional staff in an atmosphere of connection and reflection to converse on breaking barriers, building futures, and empowering women in higher education. In conversation with colleagues, Prof Klopper shared her personal journey in higher education, her leadership philosophy, and the values that have guided her career. The occasion created a meaningful platform for colleagues to reflect on the role of women in shaping the future of the faculty and the university.

 

Breaking barriers, building futures

Prof Klopper described her appointment as both humbling and historic: “It is an extraordinary honour to be entrusted with this responsibility. This milestone is not just a personal achievement, but also a reflection of the progress we have made as a university and as a society in recognising and valuing diversity in leadership. I stand on the shoulders of many trailblazers who paved the way, and I hope my appointment inspires women to believe that there are no limits to what they can achieve.”

She shared pivotal moments across her career journey – from transitioning into academia to international leadership experiences that shaped her vision. “You become aware of a growing, burning desire to plough back what you have learned; to pay forward in some way after receiving so many opportunities for growth, so much exposure to great role models, and such incredible learning experiences,” she said.

Acknowledging the challenges women still face in higher education, Prof Klopper reflected: “Academia has traditionally been male-dominated. In order to overcome stereotyping and bias, I drew on the values instilled by my parents – hard work, believing in yourself, non-discrimination, fairness, and care. These have been incredibly valuable in my journey.” She also highlighted the importance of supportive partnerships when balancing professional and family responsibilities.

Prof Brownhilder Neneh, Vice-Dean: Research, Engagement and Internationalisation in the Faculty, said these reflections captured the very purpose of the gathering. “With Prof Klopper serving as the first female Vice-Chancellor and Principal of the UFS, it was important to create a platform for her to inspire and empower women academics,” she said. “By sharing her career journey and insights, she demonstrated how barriers can be overcome in higher education leadership.” 

She added that the conversation reinforced an important message: “Women, too, can achieve whatever they aspire to become. Prof Klopper reminded us that one must be clear about the message they want to communicate, know what they stand for, and remain consistent, authentic and honest. She emphasised the importance of always considering what you bring to the table – your expertise and knowledge – which ultimately opens doors. She also reminded us that women need to create their own values and live them, be intentional, and show up. There is no single recipe – each person must find their own rhythm and pursue it deliberately.”

Prof Klopper echoed with a message of encouragement to young women: “Have the courage to embrace your own authentic leadership style. Do not allow others to define who you are – believe in your own abilities. Knowledge without action is incomplete. Lead with heart, take intellectual risks, and remember that talent exists everywhere, but you have the power to create opportunity.”

Prof Neneh added that the event was not only a celebration but also a call to action: “Women play a vital role in enriching the academic project by bringing diverse experiences, perspectives, and leadership approaches. I hope colleagues left encouraged to pursue their aspirations with confidence and inspired to embrace mentorship, sponsorship, and solidarity among women academics.”

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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