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07 July 2023 | Story Kekeletso Takang
UFS Industry VisitsUFS Industry Visits - promoting student development
Students from the University of the Free State (UFS) recently had the opportunity to visit four Bloemfontein companies as part of their learning experience in the School of Accountancy.

The University of the Free State (UFS) is committed to producing employable graduates. Being student-centred, the UFS is continuously seeking opportunities to promote the learning experience by taking a holistic approach where teaching and learning extend beyond the four walls of a lecture hall. It is to this end that the UFS School of Accountancy recently took hands with local businesses to expose students to the real world of work through industry visits.

Aimed at providing students with insights into the real world, the industry visits are the initial point of contact between students and the working industry. The approximately 280 students in the Bachelor of Accounting (final-years), Bachelor of Commerce Honours in Accounting, and Postgraduate Diploma in General Accountancy were exposed to the real world so they could see first-hand what professional accountants do, how the business world works, and how their different modules integrate.

Four of Bloemfontein’s largest companies agreed to host a group of 70 students each. Students were given the opportunity to sign up for the company they found most interesting. The companies – Raubex Infra, SA Truck Bodies, Interstate Bus Lines, which sponsored transport to and from all the companies, and Sun Windmill Casino – function in the construction, manufacturing, transportation, and entertainment sectors, respectively. Students were not only treated to talks by the directors and senior staff of all the companies who took time to address them and share insightful information about their operations, but also to tours and treats.

“The updated SAICA competency framework, which guides most of our teaching at the School of Accountancy, requires us to enhance our focus on professional values, attitudes, and acumens (PVAAs). The industrial visits specifically address business acumen, but the added benefit is that it inspires and excites students, as it exposes them to where they may be in future," says Ané Church, Lecturer in the School of Accountancy.

The industry visits were not only fun and tours, but students were also tasked with writing a reflective essay after the visit, setting out what they learnt, found interesting, and would recommend to the respective companies. This, in turn, addressed students’ writing skills and uses reflection as a means of learning.

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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