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22 October 2025 | Story Leonie Bolleurs | Photo Supplied
Giraffe Research Centre
The giraffe research programme and infrastructure facility at Amanzi Private Game Reserve marks the next phase in a research journey that has already placed the UFS at the forefront of giraffe science.

The University of the Free State (UFS) is taking wildlife research to new heights. On Wednesday 29 October 2025, the university will officially launch the giraffe research programme and infrastructure facility at the Amanzi Private Game Reserve near Brandfort – a first-of-its-kind in the world, dedicated to advancing local and international scientific collaboration in the study and conservation of giraffes.

The launch marks the next phase in a research journey that has already placed the UFS at the forefront of giraffe science. Over the past decade, a team of researchers, led by Prof Francois Deacon from the Department of Animal Science, has made significant contributions to understanding giraffe behaviour, physiology, and ecology. Building on pioneering work in reproductive technologies, endocrinology, anatomy, and disease, the new infrastructure combines on-site research laboratories with spacious, stress-free habitats. In this hands-on environment, veterinarians, scientists, and students can work closely with giraffes while promoting their welfare and supporting both local and international research projects.

Over the past seven years, his team has conducted 254 successful sedations and captures, carefully building the expertise needed for the next delicate step: the first embryo transfer in wild giraffes.

“This dedicated research facility will provide a safe and controlled environment where the world’s first giraffe embryo can develop and grow, and where we can collaborate to produce the science needed to turn the extinction of the giraffe around,” he explains. “The general public may not see the results immediately, but 20 years from now, what we are doing today will be vital in creating a biobank of viable giraffe embryos and calves that can be used in surrogate animals, supporting sustainable conservation practices for future generations.”

This programme will allow researchers to expand their understanding of the world’s tallest land mammal in ways that were not possible before. “From conducting sedation and sample collection to pioneering reproductive techniques such as semen preservation and embryo transfer, the facility provides an environment where we can study, among others, giraffe genetics, reproductive biology, and physiology; knowledge that is important for their conservation and survival,” says Prof Deacon. 

About 12 departments at the UFS are already involved in the research project in one way or another. This includes from the Department of Animal Science to the Departments of Zoology and Entomology, as well as Chemistry and even Information and Communication and Technology Services, which contributes to 3D-modelling, software, and monitoring of the animals. 

The project also offers opportunities for collaboration with conservation organisations and universities worldwide, positioning the UFS as a leading hub for giraffe and large-mammal research in Africa. Current partners who share Prof Deacon’s vision for giraffe conservation on the African continent include Save the Giraffes (a US-based NGO), Absolute Genetics, Ramsem, and the Kroonstad Animal Hospital.

Despite their towering presence on the African continent, giraffes are quietly disappearing. The International Union for Conservation of Nature (IUCN) lists them as Vulnerable, with populations declining by more than 40% over the past three decades. Today, fewer than 100 000 remain in the wild – a sobering reminder that their future is far from secure and that research excellence like this is key to ensure their survival.

“We have all the technology and all the expertise to make a change. Now is the time to bring about this change to secure the future of giraffes on this continent,” Prof Deacon concludes, emphasising the UFS’ commitment to sustainability, care, and conservation.

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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