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30 March 2021 | Story Dikgapane Makgetha | Photo Supplied
Social Work students at the UFS are working with the relevant stakeholders in an Engaged Teaching and Learning service-learning project to promote and respect children’s rights.

The protection of children’s rights is the principal achievement on the Sustainable Development Goals (SDGs) 2030 Agenda. Emphasis has always been on the promotion and respect of children’s rights. Since the SDGs are grounded in a child rights-based approach, the University of the Free State (UFS) Social Work students – by engaging in a multi-disciplinary methodology – involve all the relevant stakeholders in their Engaged Teaching and Learning service-learning module project. 

The social partners, which included the South African Police Service (Child Protection Unit), the Department of Social Development, the Department of Home Affairs, the Department of Health, faith-based organisations, and other children’s advocacy agents, were involved from inception until the apex launch of the project. 

Access to basic human rights

In their exit level, fourth-year Social Work students participate in community work practicums, which incorporates the theoretical development process in adherence to the objectives of their community work. The initial phase of the project involved the situation analysis exercise, which the students implemented through collaboration with the Rekgonne Primary School action committee. 

The outcome of the survey indicated that some learners were exposed to physical and sexual abuse. It was also found that they did not have access to basic human rights such as education, health care, and social grants due to the absence of the required legal documents. From the interactive discussions that took place during the launch, it emerged that some children do not have birth certificates required for school registration and access to social grants. 

Through the students’ community project, a platform was created where important skills and information could be shared among all important role players (who are in different professions and guardians of children’s human rights). It is believed that since learners are spending more hours in school, educators would be the primary detectors to notice signs of negligence and potentially adverse circumstances among their learners.

Role players collaborate to make a difference

Through the scholarship of engagement, students succeeded in engaging with the community to attend to societal challenges (violated children’s rights). In order to realise the outcome of the project, continuous collaboration among all role players must be sustained. All parties adopted a resolution to create safe environments both at school and at home by supporting families and caregivers.

Government partners that participated were determined to strengthen protection systems and improve child welfare, reinforcing the implementation of the Children’s Act 38 of 2005.  Educators were empowered and supported in the mandate of the Quality Learning and Teaching Campaign (QLTC). This is an initiative that involves stakeholders in improving the quality of education for all children and addresses issues of safety and well-being for all children. 

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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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