Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
13 December 2020 | Story Eugene Seegers and South Campus contributors | Photo Johan Roux
Dr Joleen Hamilton - Johan Roux JRX December 2019
Dr Joleen Hamilton is one of the faces behind the short learning programmes hosted on the UFS South Campus. Joleen obtained her PhD in December 2019.

 

This year may have been one of the most challenging since the higher-education industry started, but the UFS South Campus in Bloemfontein has not rested on its laurels when it came to putting its technology and expertise to use in supporting not only tertiary but also basic education. Here are three examples of a large array of short-learning and other courses or interventions hosted on this always-innovating campus.

Online and short learning
Since the South Campus is the university’s online, distance-learning, and e-Education (ODeL) hub, it was in the ideal position to take certain courses and convert them to online short-learning programmes (SLP). These included a Euclidean Geometry programme arranged with the Free State Department of Education (FSDoE). Study guides were printed and couriered to the teachers who participated, and WhatsApp groups were used as the primary communication tool. Participants could submit their assignments via email or WhatsApp. An online forms platform was used to facilitate registration, as well as for pre- and post-tests and evaluation of the SLP.

Another two courses were Harnessing Social Media (five weeks) and TeachOnline (sixteen weeks): these SLPs were developed during the lockdown. The goal of both was to equip teachers with the skills needed to use technology as a mode of instruction during times like lockdown. Harnessing Social Media is a basic course that focuses on social-media platforms such as WhatsApp as a teaching tool. TeachOnline is a more advanced SLP that shows you how to use Google Classroom effectively. All the assignments were also completed and uploaded on Google Classroom. A total of 150 teachers were accommodated in the above three SLPs.

IDEAS Lab lends a hand
The IDEAS Lab’s studios, which would usually host the Internet Broadcast Project, were made available to the FSDoE, and technical assistance was provided to record the trimmed Annual Teaching Plan (ATP). The IDEAS Lab furthermore designed and published a YouTube channel where their IBP videos could be uploaded; the IBP’s recording time and subjects were also increased. Computer hard drives were used to distribute videos to schools.

Community Engagement project in Sterkspruit
Despite the pandemic and national lockdown, there was no concern that the South Campus would be prevented from displaying a meaningful 67-minute act of love. The tight-knit family on this campus reached out to an early childhood development (ECD) centre in need close to Sterkspruit which has 15 learners. Being aware of their extremely limited resources, and how cold the winters get in that area, staff members under the inspiration of Nelia Oosthuizen and Prof Lynette Jacobs, have since September 2019 been knitting squares that are then sewn together to form blankets. Knitting was certainly also a form of therapy for the staff members involved, and when lockdown eased and we could give them the gifts of love, the young learners at this ECD centre knew that somebody in a place far from theirs took the trouble to make a colourful, comfy blanket stitch by stitch to keep them warm.

Gauteng teachers empowered
The South Campus is dedicated to delivering quality distance education to sectors of society that would not necessarily have access to higher education. Its flagship programme, the Advanced Certificate in Teaching (ACT), has been delivered across six provinces of South Africa to more than four thousand semi-qualified teachers over the past four years, thereby ensuring that qualified teachers deliver quality education in some of the country’s remotest areas.

The South Campus Formal Programmes division, in collaboration with the Gauteng Department of Basic Education, has identified teachers within that province who would benefit from additional training. Funding for the students’ tuition and ICT training was secured from ETDP-SETA through the Campus Principal, Dr Maria Madiope. In 2020, a total of 563 Gauteng students were funded at a comprehensive value of more than ten million rands.

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