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23 September 2022 | Story Jani de Lange | Photo Rulanzen Martin
Jani de Lange
Jani de Lange is a Sign Language academic and researcher and a campaigner for South African Sign Language and greater inclusion for South Africa’s Deaf community. She is currently busy with her PhD at the UFS.

Opinion by Jani de Lange, Lecturer and PhD candidate at the Department of South African Sign Language and Deaf Studies, University of the Free State. 

September is designated as the National Month of Deaf People in South Africa. This includes the International Week of Deaf People (19-25 September) and the United Nations-recognised International Day of Sign Languages (23 September). This month commemorates the first World Deaf Congress, held in Italy in September 1951, at which the World Federation of the Deaf (WFD) was established. The purpose of this month is to raise public awareness about Deaf people’s concerns and successes, about hearing loss, deafness, Deaf culture, as well as sign languages – in our case, South African Sign Language (SASL). The WFD, as the international Deaf organisation, allocates a theme every year to guide Deaf awareness campaigns. This year’s is ‘Building Inclusive Communities for All’. Considering the recent proposed amendment to include SASL as South Africa’s 12th official language, and our yearly celebrations of our diverse heritage on 24 September, this theme is applicable to all South Africans, not only the Deaf. But how much do we really know about this minority group?


To me, the success of this group is evident in their fight for the recognition of SASL, especially with regards to access to quality education. The Deaf community of South Africa has been fighting for the recognition of SASL for many years. The pre-1994 policy of racial segregation was extended to children’s hearing status, which resulted in small pockets of Deaf school communities away from their hearing peers. The education system at the time promoted the use of oralism (teaching Deaf children to lip-read and denying the use of SASL), and many Deaf children did not go to school. Despite this, SASL continued to develop among the different communities. This resulted in different dialects of SASL, a language with its own vocabulary and grammar rules. This language is an integral part of any Deaf person’s identity, and functions as a marker of cultural membership. 

SASL needs more recognition as a Home Language 

The Schools Act of 1996 recognises sign language (not specifically referring to SASL) as “official” for the purposes of teaching and learning in Deaf Schools. Unfortunately, this stipulation did not necessarily change the educational prospects for this group. While SASL was used as a medium of instruction, it was not accepted as an exit-level Home Language subject. According to an article published in the ‘African Disability Rights Yearbook’ in 2016, this led to many dropping out of school at Grade 7. Some learners were able to attend hearing schools by making use of residual hearing or assistive devices, but they either dropped out, or completed Grade 12 with poor results. Only a small group finished with an endorsed certificate. In all these scenarios, the prospects for tertiary education and employment are limited. A step towards improving educational opportunities for the Deaf was achieved in 2009: A family wanted their child to eventually attend a tertiary institution. Given the drawbacks of attending a hearing school, they did not want to risk their child’s chances, so they took the Department of Basic Education to court. After the case was settled out of court, SASL was implemented as an exit-level Home Language subject in Deaf schools in 2013.

This year, the draft Constitution Eighteenth Amendment Bill was published to give the Deaf community what they have been fighting for over so many years – official recognition of SASL. But will this recognition contribute to the inclusion of the South African Deaf community in the mainly hearing world? Currently, the legal protection of the Deaf in South Africa is under the umbrella of disability. This view is vested in the pathological perception of deafness, which is the prevailing understanding of the hearing world. To build an inclusive society, it is necessary to look beyond the medical aspect of ‘disabled’ and see the use of SASL as a marker of another culture, a view propagated by the socio-cultural approach to deafness. There is a lot that hearing people do not know or understand about the Deaf community and their experiences. However, we can acknowledge this group of people as part of our already diverse country by being open to learning more and celebrating their successes. 

As individuals, we can take time to determine how we ourselves could change to promote inclusion, rather than expecting people to change to fit into our own view of society.

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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