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02 January 2024 | Story Leonie Bolleurs
UFS scientists contribute to the battle against cancer
From top left, moving clockwise: Dr Nerina van der Merwe, Dr Osayande Evbuomwan, Prof Alicia Sherriff, Profs Andreas Roodt and Alice Brink.

Cancer stands as a prominent contributor to deaths worldwide, with a big impact on families and communities. Prostate cancer is one of the leading causes of mortality in the world. The recent diagnoses of cervical cancer are 10 702 annually, with 5 870 patients passing away. Female breast cancer surpassed lung cancer as the most commonly diagnosed cancer in 2020 (American Cancer Society), representing 11,7% of all cancer cases, making it the fifth leading cause of cancer mortality worldwide. Researchers at the university are doing their part in the fight against cancer.

Treating prostate cancer

In July 2021, Dr Osayande Evbuomwan, Senior Lecturer and Medical Specialist in the Department of Nuclear Medicine, along with a team of university doctors, initiated patient treatment using radioligand therapy (RLT). This targeted nuclear medicine therapy delivers high radiation levels precisely to cancer cells, minimising damage to normal organs and tissue, a benefit not typically provided by conventional therapies.

It was the first time that Lutetium 177 PSMA – a type of PRRT – has been used to treat patients with metastatic castrateresistant prostate cancer (MCRPC) in the Free State, providing hope when standard treatments and conventional therapy are not an option. This treatment generally enhances quality of life, slows disease progression, and extends overall survival, with minimal side effects.

All three patients treated with Lu 177 PSMA so far have completed at least four therapy cycles and tolerated it well. The first two patients, while initially responding well, sadly passed away due to unrelated causes. The third case stands out as the most successful, responding excellently to seven treatment cycle and remaining in good health.

Dr Evbuomwan recently also obtained a license for a more effective therapy, AC 225 PSMA, as an alternative to Lu 177 PSMA.

Precise cervical cancer therapy

Medical personnel at the Universitas Academic Hospital also became the first in Southern Africa to use interstitial brachytherapy as a method for treating cervical cancer. Prof Alicia Sherriff, Head of the Department of Oncology, explains that brachytherapy – a form of internal radiation therapy – places the radiation source near or inside the cancer. “Precise delivery of curative doses to the cancer protects surrounding organs such as the bladder, rectum, and small bowel,” she explains.

Three to five weekly brachytherapy sessions under conscious sedation usually begins after two weeks of daily external beam radiation. On brachytherapy days, external beam radiation is not administered. “The intracavitary brachytherapy applicators are placed within the cervix and uterus and deliver high doses locally, but for surrounding tissue infiltration, additional needles are inserted via the Venezia applicator, delivering high-dose radiation while sparing organs,” says Prof Sherriff.

Their work aligns with the broader goals of the university and its commitment to advancing health care in the region by ensuring the continued growth of their skills and technology, while applying these skills to improve the possibility of disease control, cure or palliation with quality of life.

Familial breast and ovarian cancer testing

Dr Nerina van der Merwe, a principal medical scientist in the Division of Human Genetics, and colleagues are engaged in breast cancer research. They are involved in translational research using new technologies that, once validated as a first-tier diagnostic test, could revolutionise genetic testing for familial breast and ovarian cancer in South Africa when used in conjunction with genetic counselling. This parallel application is ideally suited for primary hospitals and rural clinics, as it will dramatically increase accessibility and uptake of genetic testing in rural areas.

By performing first-tier genetic testing at a community clinic, patients no longer have to be transported to tertiary hospitals for testing, and more patients and related family members who are unaware of a familial predisposition will be reached. “By warning unaffected related individuals about their potential increased risk, we can play a part in the earlier detection or diagnosis of patients, improving their cancer survival rate,” states Dr Van der Merwe.

Patenting cancer research

Prof Andreas Roodt, a retired Distinguished Professor in the Department of Chemistry, and colleagues – particularly Prof Alice Brink and co-worker Prof Roger Alberto from the University of Zurich – have published widely on the chemistry of radiopharmaceutical models. Since the 2000s, the world has introduced the concept of ‘theranostics,’ which involves the use of a single compound for both cancer detection and therapy. “These compounds contain a radioisotope that provides internal radiation for cancer detection (diagnostic) and a second part for treatment,” explains Prof Roodt.

Their research enables the high-yield preparation of compounds containing multiple isotopes often present in very low concentrations. “This allows combining diagnostic isotopes such as technetium-99m (used in >80% of diagnostic patient studies worldwide) with therapeutic radioisotopes, such as rhenium-186 (used for bone cancer therapy), with ease. Many therapeutic radioisotopes do not have good diagnostic radiation; thus, by combining the two types of radioisotopes in one medicine, the oncologist can now clearly see where the therapeutic part is going and apply more effective treatment,” he says.

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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