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23 May 2025 | Story Lilitha Dingwayo | Photo Lunga Luthuli
Mock Interview
UFS students shine with confidence at the 2025 Mock Interview Day, ready for career success.

To get senior and postgraduate students ready for the world of work, the University of the Free State (UFS) Division of Career Services’ Placement Preparation Day, which was initiated in 2023, has grown into an annual workshop – Mock Interview Day – with this year’s event taking place in the Callie Human Centre on the Bloemfontein Campus.   

Held on 14 and 15 May 2025, this UFS initiative – aimed at addressing employability – has evolved through the implementation of several educational subdivisions tasked with the responsibility of assisting all registered students understand the professional environment. One of these divisions is the Centre for Teaching and Learning’s (CTL) ‘Graduate Attributes’ – an initiative that seeks to assess a student’s development of valuable attributes during lectures.

According to Belinda Janeke, Assistant Director of Career Services, “Feedback indicates that most students have no interview experience – a critical factor. It is through these mock interviews that students’ confidence is built and their transition from student to employee is smoothened.” 

With the assistance of staff members and employees in conducting the interviews, the two-day initiative has seen evident success in both attendance and reach. “Yesterday we had about 90 students come in for the mock interviews and all of them stated that it was their first time being interviewed,” said Janeke. “Even though our office is situated on the Bloemfontein Campus, we also visit the South and Qwaqwa campuses to ensure accessibility across all three UFS campuses,” Janeke added. Emphasising results, she shared that in the 12 years she has been working in this division, student engagement has grown due to improvements in technology. 

Career Services sends out letters and emails on the 11th of each month to recognise the achievements of students who have used their services. In collaboration with the UFS’ Vision 130, more directions are being explored across the three campuses, starting with the cross-campus Shoe Camp project.

This initiative targets all UFS students, prioritising senior individuals on the cusp of job hunting. “As a postgraduate student, I am looking into getting a job next year and I have never been interviewed before, so I needed the trial run to get more information on accurate interview etiquette,” said Aphiwe Mbutuma, an Administration honours student. Mbutuma said the support she received from the staff was crucial in boosting her confidence for her next interview. She further described the experience as an eye-opener, adding that students should seize these opportunities to understand what is expected of them. Zukile Daki, a second-year student in the Faculty of Law, said: “I once bombed an interview, so I came here to improve, and it went well.”

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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