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21 July 2022 | Story Leonie Bolleurs | Photo Supplied
Riaz-Seedat
Prof Riaz Seedat, who enrolled for a PhD through the USDP, wishes to create ear, nose, and throat knowledge through his research that is more relevant to the South African setting.

Prof Riaz Seedat is Professor and Head of the Department of Otorhinolaryngology at the University of the Free State (UFS) and in the Free State Department of Health at the Universitas Academic Hospital. It is in this position where he has the opportunity to treat patients, teach students, and conduct research.

As one of the ten academics enrolled in the University Staff Development Programme (USDP), Prof Seedat forms part of the University Capacity Development Programme (UCDP), which seeks to transform academic expertise in the field of global health.

The UFS Office for International Affairs administers the programme, which offers an enriching journey for the group of academics from the University of the Free State (UFS) and the University of Venda (Univen).

In an interview, he revealed the importance of research focused on ENT cases in developing countries. 

How has your background shaped the life and academic path you have chosen? 

During my internship, I had the opportunity to work in ENT. The field sparked great interest in me, so I decided to specialise in it. 

During my training, it became apparent to me that much of the information in the literature was based on research and practices in developed countries and did not reflect the situation in developing countries, where there is a high burden of infectious diseases and presentation of patients with pathology at an advanced stage. My research has been focused on providing a developing country perspective of otorhinolaryngology, particularly with regard to infectious diseases and allergy in the field, creating ENT knowledge that is more relevant to the South African setting. 

What drew you to the USDP project’s call? 

The USDP provides me with the chance to complete my doctorate on recurrent respiratory papillomatosis, a disease that is characterised by recurrent wart-like growths on the surface of the vocal cords or tissue around the vocal cords.

In our context, this affects mostly children and there is a relatively high prevalence of this condition here in the Free State. Research through this PhD will expand knowledge on the diagnosis and management of the condition. 

Please tell us more about your research. 

I have identified that in South Africa, recurrent respiratory papillomatosis, which is caused by the human papillomavirus, occurs more commonly in children than in Europe, where mostly adults are affected. In future, I would like my research to find factors that can help to identify which patients with recurrent respiratory papillomatosis will develop more severe disease, in order to better treat them. 

I have also done work on infectious diseases such as HIV and ENT, describing the impact of HIV in the different ENT conditions we see. 

With regard to allergic rhinitis, we have studied the impact of the condition on patients’ quality of life and are identifying the most frequent allergens present in our setting here in the Free State.

Did the pandemic impact your research?

Yes, it did. Being a full-time clinician for the Free State Department of Health meant that we had to dedicate more time towards managing the pandemic. This has affected patient care and the research we do on the patients. Many patients could not access healthcare facilities because of the lockdown, impacting their treatment, as well as research being carried out. 

Global health is one of the critical issues for the future of the human species, especially in Africa, where both infectious and non-communicable diseases threaten development. What will your project contribute to the field? 

Many of the conditions I am researching are as a result of infectious diseases. Unfortunately, these are conditions that are often neglected as they occur mainly in developing countries. The research will positively impact society through the care and treatment of patients with the condition. 

What are your future career plans? How will a PhD qualification assist you in reaching these goals?

A PhD will help me obtain a better understanding of research content and methodologies. I believe that a PhD will also equip me with the knowledge to better supervise individuals who wish to further their academic careers and do their own PhDs. 

What is your advice for aspiring PhD candidates?

I would advise someone who wishes to complete a PhD to work on a topic that they have a great interest in, because it is a task that will take much of your time. 

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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