Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
06 December 2022 | Story André Damons | Photo Sonia Small
Dr Nicholas Pearce
Prof Nicholas Pearce has joined the Faculty of Health Sciences’ management team after being appointed Head of the School of Clinical Medicine. Prof Pearce is the former Head of the Department of Surgery at the UFS and led the Universitas Hospital’s COVID-19 Task Team.

During the height of the COVID-19 pandemic, Prof Nicholas Pearce led the COVID-19 Task Team of the Universitas Academic Hospital, ensuring that the hospital not only had enough Personal protective equipment (PPEs) and beds for patients, but also that the vaccination process ran smoothly. Now, the Best Doctor of the Year for 2022 – as named during this year’s National Annual Batho Pele Excellence Awards (NBPEA) – will lead the School of Clinical Medicine in the Faculty of Health Sciences at the University of the Free State (UFS).

Prof Pearce, former Head of the Department of Surgery at the UFS who served the faculty in multiple capacities over a long period, took up this position on 1 December 2022 – a position he is looking forward to.  

Create world-class doctors, maximise students’ full potential

“I’m excited about taking up my new position as Head of the School of Clinical Medicine. This is a role that comes with huge responsibility, and my vision is to create world-class doctors and to maximise each student’s full potential.  We, as university, are a national asset and need to grow and develop to be of service to the future of our country.  So, to lead a school with such a prestigious history is truly a privilege,” says Prof Pearce. 

According to him, the goal for the Medical School in the next five years should be determined by three main core drivers: service delivery, research, and teaching and training. He would like to be in a stronger position, with innovation that can produce world-class doctors (both undergraduate and postgraduate). 

If you look at the strategic plan of the UFS, says Prof Pearce, it is clear that, under the leadership of current Rector and Vice-Chancellor, Prof Francis Petersen, a period of regeneration and innovation is upon the university. Tied to this concept is the idea of self-evaluation and improvement. The idea of challenges and coming up with solutions excites him.  

“I think for a while, my main aim will be to bring the university, the provincial Department of Health, and the school in alignment, ensuring that we are all pulling in the same direction to achieve the same goal.”  

“At the end of the day, the goal here is to provide quality health care to the people of South Africa, while the Department of Health, the university, and society each function in different environments – coming together and understanding each other’s needs and having a common goal – excellent health care in this country for all our citizens.”

Lessons learned from surgery and running COVID-19 task teams

Prof Pearce, who was awarded the UFS Chancellor’s Medal for outstanding service during the April graduation ceremonies, says lessons learned from being both a surgeon and running COVID-19 task teams, are that strategic organisational processes need to be in place – systems strengthened, the policies and procedures adapted, and comprehensive planning taking place. 

However, he says, one must also bear in mind that we have a history of very high academic standards in the School of Clinical Medicine, so you want to improve on that rather than go backwards.

“I learned a lot from surgery and COVID-19 that will equip me in future. COVID-19 taught me about organisational management, disaster management, funding, resource management, people management skills, development, etc.  
“Running the Department of Surgery, one of the largest departments in the faculty with multiple inputs and personalities, has taught me that you are only as strong as the team behind you. I have an amazing team behind me in this new role, whether it is the dean, vice-dean, heads of department, administration, rectorate, and so forth.” 

He will continue to work at the Universitas Hospital; however, being fully employed by the university, he will only be doing some calls and working over weekends.  

“As a surgeon, theatre has always been my safe haven, my place of meditation, my place of peace, and I am sad to say goodbye to surgery and the Department of Surgery – it has been loyal, and I am grateful to everyone in the department; but I think as with all good things, there is a time to come and a time to go.”

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.

We use cookies to make interactions with our websites and services easy and meaningful. To better understand how they are used, read more about the UFS cookie policy. By continuing to use this site you are giving us your consent to do this.

Accept