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31 October 2021 | Story Rulanzen Martin | Photo Stephen Collett
Stegmann Gallery - Stephen Collett
The Johannes Stegmann Gallery.

Digital and online art exhibitions are no novelty. However, for the Art Gallery at the University of the Free State (UFS), it was a way of keeping the art scene alive, as many promising young artists and students depend on the exhibition opportunities UFS Art Galleries offer to debut and exhibit their works.

“The situation surrounding COVID-19 necessitated a very rapid migration into the virtual space,” says Angela de Jesus, Curator of the UFS Art Gallery. In 2020, the gallery presented its first virtual exhibition tour, creating an opportunity to reach a global audience. The exhibition hosted by the Johannes Stegmann Gallery was Leeto: a Sam Nhlengethwa Print Retrospective. (It was the second virtual exhibition for the Sam Nhlengethwa collection.)

The UFS Art Galleries comprise the Johannes Stegmann Gallery in the UFS Sasol Library on the Bloemfontein Campus and the Centenary Complex, boasting an art gallery that hosts the UFS permanent collection of about 1 000 artworks, including paintings, sculptural works, murals, prints, and ceramic works.

“The situation surrounding COVID-19
necessitated a very rapid migration
into the virtual space.”
—Angela de Jesus

Challenging times called for an adaptive attitude

In 2021, the gallery approached a hybrid model with a blended approach of an in-person and virtual exhibition being launched simultaneously. “The virtual tours allow audiences to digitally navigate (‘walk through’) the gallery space as they would in real space,” says De Jesus.

The Liminality: Student Exhibition, which saw works from first-, second, - and third-year students from 2019 and 2020 exhibited, and the Folds & Faults: An Exhibition of African Women Artists Examining Identity, Culture, and Heritage , and The Annual Final-Year Student Exhibition of the Department of Fine Arts exhibitions were just some of the 2021 exhibitions using the hybrid model.

“Every project is different, and each one comes with its own challenges and difficulties, but we learn new ways through its complexities,” says De Jesus. However, she is optimistic that the gallery will soon be able to host its signature opening events and welcome back large crowds.

 The limitation on in-person gatherings meant that traditional exhibitions were in a hiatus. The value and quality of the arts programme had to be maintained, using creative arts to navigate the pandemic. “Projects have been reimagined into the digital space through virtual tours or through the activation of social media platforms, Zoom, app development, webinars and dedicated project websites,” De Jesus says. New and exciting projects in response to the pandemic and feelings of “isolation, uncertainty, violence, and the digital overload” were initiated.

Although viewing art virtually cannot replace the experience of engaging with the art first-hand; the shift to the digital space presented the opportunity for a wider audience beyond the UFS to access the Art Gallery and its projects.

PIAD projects rejuvenate artistic creativity

Through the Programme for Innovation in Artform Development (PIAD) and funding from the Andrew W. Mellon Foundation, a number of digital artistic projects consisting of short stories, a theatrical performance, and a satirical e-commerce website, amongst others, were made possible.

The projects are still accessible and are available to view here:

Stories in die Wind, a short film animation web series about a young girl finding her purpose, based on the Nama story |!hûni //gāres |(The Rain Flower) Die reën blom: /Nanub !Khas.

WATCH THE ANIMATED SERIES HERE: https://www.storiesindiewind.co.za/

Digi-Cleanse, a satirical artwork disguised as an e-commerce website that mimics and critiques the contemporary wellness industry and its reliance on marketing and advertising.

SEE DIGI-CLEANSE HERE: https://digicleanse.co.za/

My Internal Oppression, a musical theatrical performance of emotionally content dedicated women who have toiled with internal oppression as a result of the psychological and emotional trauma of Gender-Based Violence caused by intimate partners.

SEE PERFORMANCE HERE: https://vimeo.com/468883494/376f3573d4

Sonic Re-Dress is a collaborative meeting point between music, visual art, science and art therapy, the project specifically acknowledges the insecurity, fragility and discord within our current global pandemic context by working with ‘universal’ human emotions.

SEE PROJECT HERE: https://www.sonic-redress.com/

Imaginary Futures is an experimental project of live and participatory experiences with over 40 creative practitioners, consisting of sound and film mixing, drawing, animation, puppetry and performance.

SEE PROJECT HERE: https://imaginaryfutures.org/

I am woman
I am woman
Megan Johns, "Battleground", Tobacco, charcoal dust, plaster of paris and resin, 93,5 x 50 x 7,5 cm
Megan Johns, "Battleground", Tobacco, charcoal dust, plaster of paris and resin, 93,5 x 50 x 7,5 cm
Poloko Mohanoe, "Prayer for rain", Gouache on Fabriano, 66 x 72,8 cm
Poloko Mohanoe, "Prayer for rain", Gouache on Fabriano, 66 x 72,8 cm

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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