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09 May 2024 | Story Valentino Ndaba | Photo Supplied
Disability Conference 2024
Empowering change: Advocates and experts unite at the UFS Conference on Disability Rights to foster inclusion and equality for all.

The Faculty of Law at the University of the Free State (UFS) through its Free State Centre for Human Rights, in collaboration with the Centre for Universal Access and Disability Support (CUADS) and Counterpart International, recently hosted the International Conference on Disability Rights from 24-26 April 2024. This significant event not only convened experts and advocates but also marked the launch of the Disability Rights Unit within the Faculty of Law.

Themed “Embracing Inclusion and Equality: A Perspective on Disability Rights Transformation", the conference served as a platform for insightful discussions and presentations aimed at fostering a more inclusive society.

Prof Serges Kamga, Dean of the Faculty of Law, emphasised the importance of the newly established Disability Rights Unit, stating, “The Disability Rights Unit will pave the way for promotion and protection of disability rights in our society.”

Martie Miranda, Head of CUADS, echoed this sentiment, underscoring the crucial role of such initiatives in advancing disability rights. “While CUADS provides holistic student support to students with disabilities, the Disability Rights Unit will provide for leverage in terms of access as their fundamental human right to optimally participate equally to their peers.”

Lessons from Mozambican disability legislation

Felisberto Elija Nhanenge and Jytte Nhanenge from Mozambique shed light on community inclusion through an examination of Mozambican disability legislation. Despite strides in policy, challenges persist in ensuring full societal participation for people with disabilities. The presentation highlighted the systemic barriers hindering access to education, healthcare, transportation, and employment. Moreover, it drew attention to the underlying influence of Western paradigms, emphasising the need for a holistic worldview to address entrenched biases and promote inclusivity.

Barriers to inclusion: The case of “unsound mind” provisions

Dr Dianah Msipa from the University of Pretoria delved into the legal hurdles faced by individuals with intellectual and psychosocial disabilities due to “unsound mind” provisions in African legislation. These provisions, found in several countries, restrict fundamental rights such as voting, property ownership, and personal liberty based solely on disability. Dr Msipa highlighted the urgent need for African states to align with international standards, advocating for universal legal capacity to ensure the full inclusion of persons with disabilities.

Visibility of disability: Data collection challenges

Bianca van der Schyff, representing the National and Provincial Women's Representative for DeafBlind in South Africa, addressed the critical issue of data collection regarding dual sensory impairments. She stressed the inadequacies in existing legislation which fails to capture the unique challenges faced by DeafBlind individuals, particularly concerning domestic violence. Van der Schyff put emphasis on the necessity of specialised research and comprehensive data collection to inform targeted interventions and support services for this marginalised group.

Advocating for dual-sensory impairments

The presentation underscored the importance of advocacy and empowerment for DeafBlind individuals, urging for a nuanced understanding of their needs and rights within broader disability discourse. Advocacy organisations play a vital role in raising awareness and promoting inclusive support services, yet there remains a pressing need for greater recognition of the complexities inherent in dual-sensory impairments.

In conclusion, the UFS International Conference on Disability Rights served as a catalyst for dialogue and action, reaffirming the university’s commitment to fostering an inclusive society that upholds the rights and dignity of all individuals, regardless of ability, as stipulated in Vision 130 – the strategic intent of the UFS to reposition itself for its 130th anniversary in 2034. As discussions continue and initiatives take shape, the conference represents a pivotal step towards realising the transformative potential of disability rights advocacy.

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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