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17 April 2019 | Story Mamosa Makaya
National Lotteries Commission
Front row from the left: Dr MA Madzivhandila (board member), Prof YN Gordhan (board member), Ms Charlotte Mampane (Commissioner), Prof D Coetzee (South Campus Principal), Ms Bish B Ramahlele (Director: Community Engagement) Back row from the left T Mandyu (Provincial Manager), Prof NA Nevhutanda (Chairman of the Board), Mr F Van Der Wat (Deputy Director: KovsieSport)
The University of the Free State (UFS) has over many years embarked on developmental projects to improve and upgrade its sports facilities, sports research, medical research, arts and cultural programmes and community focused programmes. These projects were made possible with the financial support of the National Lotteries Commission (NLC) which has provided funding through grants to the UFS since 2006. The UFS office of Institutional Advancement (IA) hosted the NLC on the Bloemfontein Campus on 5 April 2019, where a presentation on the success of projects was made. The role of the IA office is to ensure that the university complies with reporting requirements set out in the grant agreements and that the university maintains good relations with the NLC over the long term.

Funding fortifies UFS projects
Feedback on the success and impact of various projects was presented, such as the visual arts project. This includes the public sculpture project funded with over R3 million in 2009, which brought about the creation of outdoor sculptures that can be seen on the university grounds produced by local and regional sculptors. Feedback was provided by Ms Angela de Jesus, Curator, UFS Arts Collection and Assistant Director: Johannes Stegmann Gallery.  

In 2010 the NLC funded the upgrading of the UFS swimming pool for more than R2 million. The pool was rebuilt to bring it up to Olympic standards, allowing UFS students to have a facility at which to train for international swimming competitions. Feedback on the project was provided by Mr Frans van der Wat, Deputy Director: KovsieSport. Other funded projects are the Khoisan early learning centre, which teaches young learners on the history and culture of the “first people” of South Africa, and the Arts in Schools Project, which were both funded in 2009 for more than R6 million combined. More funded projects include the upgrading of the Johannes Stegmann Gallery in 2017, research into swimming in the Free State, and equipment for the South African Doping Control Laboratory (SADOCol), which is the only laboratory of its kind in Africa, which were funded between 2010 and 2012, totalling R4.8million.

Community development and engaged scholarship
After the change in the mandate of the Provincial Arts Council of the Free State (PACOFS) after 1996, many local dramatic arts professionals in the province were faced with dwindling work opportunities. The UFS, through the Department of Drama and Theatre Arts, stepped in to create arts programmes that would help develop and retain the skills of local performers and playwrights and an opportunity for them to be trained and directed by UFS and industry-based professional directors. 

Prof Nico Luwes, from the UFS Department of Drama and Theatre Arts, said: “I initiated the formation of the Free State Theatre Acts (FACTS) as a section 21 Company with committee members from UFS staff and local actors, with the aim of creating work for professional actors in the greater Bloemfontein area.” A combination of grants from the NLC and the UFS Department of Drama, between 2006 and 2010 resulted in 19 professional plays and four professional musicals, performed by Free State professional artists including community players from Heidedal, Botshabelo and drama students, using English, Afrikaans and Sesotho. These initiatives brought together students and artists from different linguistic and cultural backgrounds, who worked together to perform at local and national arts festivals. Although the NLC will not be funding arts and culture projects at universities in the 2019-2020 financial year, the university is hopeful to be considered in the future.

The UFS and NLC have had a successful working relationship and the feedback session aimed to strengthen the ties between them. Members of the board of the NLC expressed pride at how the UFS has developed not only its own projects, but the Free State community as well. The team was treated to an art exhibition of the work of Cape Town-based artist Ieshaan Adams at the Johannes Stegmann gallery.

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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