Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
12 June 2023 | Story André Damons | Photo Sonia Small
Prof Carolina Pohl-Albertyn
Prof Carlien Pohl-Albertyn, National Research Forum (NRF) SARChI Research Chair in Pathogenic Yeasts, leads the research team that is working on various research projects relating to fungi casing yeast.

Fungal infections affect more than one billion people each year, of which more than 150 million cases are severe and life-threatening, causing 1.7 million deaths a year. In South Africa it is estimated that diseases caused by fungal infections total more than three million cases a year. These figures are especially shocking given that prior to 1980, fungal infections were not a major health problem. The WHO has recently published a list of priority pathogens in which fungi are classified in critical, high- and medium- priority groups. Candida species are found in all three levels and Cryptococcus species in critical and medium groups,” says Prof Pohl-Albertyn.

It is for these reasons that researchers in the Department of Microbiology and Biochemistry at the University of the Free State (UFS) are working on various research projects investigating new treatment options beyond the established antifungals. Prof Carlien Pohl-Albertyn, National Research Forum (NRF) SARChI Research Chair in Pathogenic Yeasts, leads the team that is working on various research projects relating to fungi casing yeast.

Multidrug-resistant yeast

One of the yeasts being researched is Candida auris – a multidrug-resistant yeast that can cause severe infections in humans, particularly in people who are hospitalised or have weakened immune systems. C. auris was first identified in 2009 in Japan and has since been reported in over 49 countries.

According to Prof Pohl-Albertyn, C. auris is of concern because it is often resistant to multiple antifungal drugs, making it difficult to treat. In addition, it can survive on surfaces in healthcare settings, which can contribute to its spread between patients, causing outbreaks in hospitals. “Due to its multidrug resistance and potential for transmission, C. auris has been designated by the Centers for Disease Control and Prevention (CDC) as a serious global health threat and listed as the second most critical fungal pathogen in the World Health Organisation (WHO) fungal critical priority group.

C. auris possesses virulence factors such as increased thermotolerance, high salinity tolerance, biofilm formation, and extra cellular enzyme secretion, which are the major contributing factors to its multidrug resistance profile and virulence. Even though C. auris has a variety of virulence factors that it employs against its human host to develop an infection, its virulence mechanisms remain unclear,” says Prof Pohl-Albertyn.

Therefore, several research projects investigate this pathogenic yeast. All of them started with the development of CRISP-Cas9 gene editing tools for this yeast, in order to be able to delete specific genes in this yeast to study their roles. These tools are also constantly being improved for greater efficiency by students under the supervision of Prof Koos Albertyn. Two current projects deal with the function of specific secreted enzymes in the virulence of C. auris.

Environmental yeast

Another yeast being researched, under the supervision of Prof Olihile Sebolai, is Cryptococcus neoformans, an environmental yeast found in trees and soil contaminated with bird droppings. Moreover, it can be airborne and when inhaled it lodges in the lungs (in alveoli) and can cause primary lung infection, explains Prof Pohl-Albertyn.

Cryptococcus neoformans causes AIDS-defining illnesses in people living with HIV/AIDS. To the point, it was not surprising when the WHO declared it as the first critical fungal pathogen of concern. Dissemination to other organs has been reported where it crosses the epithelium barrier by secreting proteases (a class of enzymes that break down proteins in the host) that compromise the tight junctions between the epithelial cells.

The current projects investigate the interaction between the proteases secreted by C. neoformans and co-infecting viruses, such as SARS-CoV-2 and influenza. The SARS-CoV-2 virus is activated by proteases in the host and proteases also help the influenza virus to enter and infect the host cells. Since the host proteases are similar to those secreted by C. neoformans, these projects are focused on determining if the yeast proteases can also help the viruses to cause infection. This project is also extended to study Candida albicans proteases as this is also a common co-infecting yeast in COVID-19 patients (for more detail on C. albicans).

Another project looks at the application of plants as sources for novel drugs against C. neoformans. This is important since 75-80% of African and Asian populations still rely on traditional or complementary/alternative medicines for their primary health-care needs. Coupled to this, modern medicines have become increasingly expensive and thus inaccessible to many in developing countries. Moreover, there is a shift to more “organic” and “vegan” lifestyles as well as the use of herbal medicines to prevent or manage the development of certain diseases.

Yeast contaminated water

“Considering the severity of invasive fungal infection, it is important to study the dissemination and proliferation of various pathogenic or potentially pathogenic fungal species in our surrounding environments. It is crucial to identify major vectors that aid in the spread of pathogenic yeast to prevent infections in susceptible individuals, which mainly include immunocompromised or immunosuppressed individuals.

“Candida, Cryptococcus and Rhodotorula species are commonly found in a variety of water sources with which humans are in frequent contact through daily activities like bathing, washing of clothes and cooking. This recent information further warrants the investigation into the possibility that fungal infections may occur through contact with yeast contaminated water,” concludes Prof Pohl-Albertyn.

She says it is thus important to investigate the presence and antifungal susceptibility of yeast found in water as well as to identify ways to monitor potential fungal outbreaks, possibly through wastewater surveillance. The research aims to identify potentially pathogenic yeast species as well as to quantify levels of azole, specifically fluconazole, in wastewater. In addition, the fluconazole susceptibility of these isolates will be assessed in an attempt to link azole pollution of the environment to antifungal drug resistance development.

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