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26 June 2023 | Story Valentino Ndaba | Photo Supplied
Akani Baloyi
Akani Baloyi is a Presidential Youth Employment Initiative (PYEI) Intern in the Disaster Management Training and Education Centre for Africa.

The University of the Free State (UFS) is celebrating Youth Month by showcasing the positive influence of the institution on career development. As part of this initiative, we are sharing the stories of UFS alumni who are now working at the university.

Akani Baloyi, Presidential Youth Employment Initiative (PYEI) Intern in the Disaster Management Training and Education Centre for Africa (DiMTEC), shares her UFS journey:

Q: Year of graduation from the UFS:

A: 2016, 2018, and 2023.

Q: Qualification obtained from the UFS:

A: My first qualification was a Bachelor of Social Sciences in Human Societal Dynamics, my second qualification was a Postgraduate Diploma in Disaster Management, and my third qualification was a Master of Disaster Management.

Q: Date of joining the UFS as a staff member:

A: I have had the opportunity of holding multiple positions at the UFS during my postgraduate studies. The first role I took on was in 2019 when I was a Contact Session Assistant in DiMTEC.

Q: Initial job title and current job title:

A: During my master’s studies, I had the opportunity to take on some roles that helped prepare me for the professional world. I worked as a Contact Session Assistant in DiMTEC during the postgraduate diploma and master’s contact sessions, as an Assistant Officer in Student Academic Services, and as a Research Assistant in the Centre for Environmental Management. I am currently employed as a PYEI Intern at UFS-DiMTEC.

Q: How did the UFS prepare you for the professional world?

A: The roles that I took on during my postgraduate studies at the UFS have contributed so much to my personal and professional development. In the role of Contact Session Assistant, I acquired a diverse set of skills, such as strong communication, interacting with the students, understanding their needs, and conveying information clearly. I also learned to listen actively so that I comprehend the students’ concerns, questions, and feedback in order to respond appropriately. I also developed empathy and emotional intelligence, as it is important to understand and respond to the students’ emotions and needs, to ensure that they feel supported and heard. Another important skill that I developed is organisational and time management skills, which are important for managing and handling administrative tasks, and problem-solving skills that have enabled me to address challenges that arose during the sessions.

In my role as an Assistant Officer, I developed strong communication and interpersonal skills through interactions with students and colleagues, and my customer service skills were cultivated by providing support and information to students. I also learned to pay attention to detail and confidentiality, as these skills are important when handling student records.

in the role of Research Assistant, I worked with a diverse group of people on the Summer School Project, a collaboration between the UFS, the Cape Peninsula University of Technology, and the Technical University of Dresden (Germany). I had the opportunity to be part of a great team of individuals who successfully organised and hosted an online Summer School in 2022 with the theme ‘Monitoring Surface Water Quality: General Framework, Tools and Implementing Disaster Management Aspects in Urban Areas’.

Being a student at the UFS has equipped me with specialised knowledge, critical thinking abilities, and problem-solving skills. By managing multiple responsibilities, I have learned valuable skills such as time management and organisational skills. It also provided me with networking opportunities, which have allowed me the opportunity to build connections with professionals in my field. Being a student at the UFS has facilitated my personal development, as I am now confident in myself and can easily adapt to the everyday challenges of the professional world.

Q: What are your thoughts on transitioning from a UFS alumnus to a staff member?

A: Transitioning from student to staff has been a journey filled with so many feelings. Initially, it was both exciting and scary, as I was uncertain about my new responsibilities and capabilities. However, the familiarity and comfort of the UFS brought ease to this transition. I appreciate the opportunity to continue learning and growing.

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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