Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
07 January 2025 | Story Gerda-Marie van Rooyen | Photo Supplied
KovsieX
KovsieX offers a comprehensive digital experience through podcasts, video content, and social media. This initiative is set to transform the student experience, creating a strong sense of belonging and collaboration across campuses.

Optimising student experience while providing students with multimedia training using state-of-the-art equipment and aligning with Vision 130, KovsieX is set to become a great asset to the university, its students, and the community. 

This initiative, approved by the UFS Rectorate on 29 November 2023, combines various student media brands on the Bloemfontein and Qwaqwa campuses (KovsieFM, Q-Lit, KovsieTV, KovsieCAST) into a unified brand consisting of three student-driven sub-departments. This includes audio (radio and podcasts), video (long and short form), and social media (including TikTok, Instagram, WhatsApp, and YouTube). 

An all-digital approach 

Gerben van Niekerk, Head of Student Experience (KovsieX), explains: “This all-digital approach leverages digital radio, podcasts, and social media platforms to create a sense of belonging among students by reflecting on and leading student life across the campuses.” KovsieX has achieved remarkable success, reaching an audience of more than 1,2 million in the first semester alone, with multiple TikTok videos surpassing 100 000 views. 

“Recognising the evolving radio landscape, our approach integrates a comprehensive digital strategy to adapt to changing media consumption preferences and provide students with hands-on experience on emerging platforms, strengthening their market relevance. KovsieX (previously KovsieFM) moves away from traditional FM broadcasting and has enabled the students to cover a wider range of topics that affect the Kovsie community,” says Van Niekerk. He adds, “The essence of KovsieX can be summarised in our one-word slogan: IMAGINE.”  

KovsieX supports Vision 130, as it leverages emerging technologies to enrich academic and non-academic student experiences. Furthermore, it also provides students with the opportunity to gain on-the-job and leadership experience in the KovsieX executive committee (KovsieXco), comprising a small group of ‘dynamic and highly talented students’, with their first objective: to decide on a brand name and setting on KovsieX – with the ‘X’ referring to experience. 

A mobile app provides students with easier access to KovsieX’s content. This initiative is set to increase students’ experience even more, as possible partnerships are in the pipeline to deliver a year-long dialogue series on themes pertinent to students. “This initiative will engage students on key issues such as leadership, mental health, heritage, and anti-discrimination through a blend of digital content – including interviews, social media posts, and expert discussions – and live on-campus events.”  

State-of-the-art facilities 

The construction of the KovsieX Pod on the Bloemfontein Campus allows students to produce content in a state-of-the-art podcast and video studio with Apple Mac workstations and a meeting room. A similar space in the current Student Media Building on the Qwaqwa Campus, named the KovsieX Q-Pod, is on the cards, as is the integration of KovsieX across the Bloemfontein and Qwaqwa campuses. “KovsieX will be broadcast from two locations and will, therefore, allow students from both campuses to interact with one another live on air. Both radio studios will be rebuilt to allow students to stream directly on YouTube, Instagram, and TikTok from both campuses simultaneously. This is made possible by cutting edge cloud-based software – popular in Europe – but KovsieX will be the first to leverage this technology in the country,” shares Van Niekerk.

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