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04 July 2024 | Story Jacky Tshokwe | Photo Supplied
Launch of the Artists in Residency  2024
Prof Francis Petersen, Vice-Chancellor and Principal of the University of the Free State (UFS), joined in celebrating the power of art and its limitless potential for the university.

The University of the Free State (UFS) is thrilled to announce the successful launch of its groundbreaking Artist in Residency Programme. This momentous event, held on 27 June 2024, marked the beginning of an inspiring new chapter in the university's commitment to fostering creativity, innovation, and the arts within its academic community.

The event was graced by esteemed guests, including the Vice-Chancellor and Principal, Prof Francis Petersen; Deputy Vice-Chancellor, Prof Vasu Reddy; Dean of the Faculty of The Humanities, Prof Mogomme Masoga; and our inaugural artist in residence, Mike van Graan. Their presence underscored the significance of this occasion and the vital role the arts play in enriching our academic environment.

Prof Petersen's welcome address highlighted the vision behind this initiative, emphasising the university's commitment to broadening its impact beyond academia and fostering relationships that span various disciplines, including developments from STEM to STEAM (Science, Technology, Engineering, the Arts, and Mathematics). He lauded the programme as a beacon of creativity and innovation, set to thrive within the UFS community.

“This launch marks the beginning of a vibrant and enriching journey for the UFS Artist in Residency Programme. We eagerly anticipate the collaboration and the creation of a space where creativity thrives, ideas flourish, and imaginations soar. With artists like Mike van Graan leading the way, we are confident that this programme will serve as a bridge between academia and the arts, fostering dialogue and creativity that transcend traditional boundaries,” Prof Petersen expressed his gratitude.

The highlight of the event was undoubtedly the introduction of Mike van Graan, a distinguished independent artist and playwright. Van Graan, with an impressive career spanning 36 plays and extensive contributions to cultural policy and artist network development, has been a pivotal figure in the cultural landscape of South Africa and beyond. His dedication to cultural activism and artistic creation is widely recognised, and his insights during the event provided a profound perspective on the importance of supporting the arts, particularly theatre.

Van Graan shared his vision for the future of theatre and drama in South Africa, emphasising the need for a supportive and recognising arts minister. He expressed hope for a future where talent and policy merge to create a thriving cultural sector. His thoughts on the relevance and impact of the residency programme on both the industry and the academic environment resonated deeply with the audience.

The programme director, Prof Anthea van Jaarsveld, guided the event seamlessly, introducing the staged readings that showcased the incredible talent nurtured during the residency. The first reading, an excerpt from The Good White, delved into contemporary issues such as race, social justice, and the complexities of human relationships against the backdrop of the 2015/16 student protests. The second reading, Return of the Ancestors, paid homage to the satirical South African political play, Woza Albert, exploring themes of democracy and sacrifice through the return of figures such as Steve Biko and Neil Aggett.

As the event drew to a close, heartfelt gratitude was extended to all who contributed to the success of this launch. Special thanks were extended to the UFS leadership, the Dean of the Faculty of The Humanities, the office of the Deputy Vice-Chancellor, the Department of Communication and Marketing’s staff, the staff in the office of the Vice-Chancellor, and the various outsourced companies for their presence and contributions.

“Thank you to everyone who joined us in celebrating the power of art and the limitless potential it holds for our university and beyond. Together, we will continue to create spaces for dialogue, understanding, and inspiration through the transformative power of art,” Prof Van Jaarsveld said in closing the ceremony. 

#UFSArts #ArtistInResidency #MikeVanGraan #Creativity #Innovation #STEAM

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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