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06 November 2018 Photo Sonia Small
Matrics 2018 a shift from access to success urgently needed in higher education
According to UFS Rector and Vice-Chancellor, Prof Francis Petersen, we should ask ourselves how learners successfully exit institutions of higher learning – within the minimum time and with an appropriate qualification that will enable them to start earning an income and contribute to the economy.

Opinion article by Prof Francis Petersen

 

With Grade 12 learners from across the county in the full throes of writing their matric examination, one inevitably wonders about 2019 and where those who pass successfully, will find themselves.
 
The announcement of subsidised free education last year has increased learners’ access to higher education.
 
However, the question we should ask is no longer how these learners enter institutions of higher learning, but how they exit successfully – within the minimum time and with an appropriate qualification that will enable them to start earning an income and contribute to the economy.
 
Universities getting involved in schools

I believe universities have a critical role to play in ensuring their own students’ success. It often involves taking a step back and getting actively involved in the schools that supply us with a new cohort of first-year students annually. We should not wait until they reach our campuses to identify academic obstacles; we should be proactive and do what we can to help improve our school systems.

At the University of the Free State, we have established Social Responsibility Enterprises (SRE) on our South Campus in Bloemfontein, which focus on the mentoring of teachers in order to make a sustainable impact. A total of 78 schools in the Free State, Mpumalanga, and the Eastern Cape benefit from this programme. SRE mentors are assisting school principals with school management, while teachers in Mathematics, Physical Science, Accounting, and English as language of learning are assisted in mastering curriculum content, pedagogy, and classroom management. 

Mentors visit schools and share knowledge, extra material, and technology to improve the standard of teaching. The impact has been significant. Matric results, Mathematics pass rates, and Physical Science pass rates have improved dramatically in these schools. We also identify learners with the potential to get access to university (i.e. first-generation students) and assist them through extra classes and in applying for tertiary education and bursaries.

Using technology to reach learners

Another important initiative is the Internet Broadcast Project (IBP), established on our South Campus seven years ago. Our aim is to take quality education to all learners across the Free State, regardless of their socio-economic backgrounds and the standard of education at their schools. Schools are equipped with internet broadcasting devices, and lessons by top-qualified presenters in a studio are transmitted live to learners. They also have an opportunity to interact with these presenters.  Currently, the departments of Education in three provinces (including the Western Cape) are also considering the implementation of the IBP as part of their interventions in schools.
 
A total of 71 000 learners in 83 different schools are currently reached through this project every week – and the impact is far-reaching. The Free State has delivered the best matric results in the country for the past two years. Last year, the Free State MEC for Education, Tate Makgoe, made special mention of the IBP for the profound role it played in this achievement.
 
Understanding students’ needs

However, preparing learners for access to higher education is not enough; the crucial factor is how they exit successfully. The university’s Centre for Teaching and Learning (CTL) is continuously developing data analytics to better understand our students and to help them navigate their studies. Making use of international funding, CTL is playing a leading role nationally to develop academic advising (using predictive data analytics) that helps students match their studies with their career and life goals.

One of the main factors that has been found to inhibit student performance, is food insecurity. Research has shown this to be a challenge faced by universities across the world. In South Africa, our institutions of higher learning have risen to this challenge, responding with efforts in various forms. At the University of the Free State, the No Student Hungry initiative (NSH) was launched in 2011. A research study conducted by our Department of Nutrition and Dietetics indicated that 59% of the student population suffer from food insecurity. Many of these students eventually drop out of higher education because of the need to earn an income. The NHS provides our students in need with modest food allowances and daily access to one balanced meal. Students are selected in terms of financial need, academic performance, participation in student life, and a commitment to giving back to the community. The programme allows students to focus on their studies without worrying about their next meal, thus increasing their chances to excel academically and ultimately obtain their degrees.  Since its inception, close to a thousand students have been assisted by this initiative and have given back nearly 37 000 community hours to South African communities.
 
Currently, the NSH programme is enhanced through the development of an institutional endowment fund aimed at raising capital from business, industry, and the private sector. This provides an opportunity for these sectors to become involved and support the challenge of food security among students, thereby supplementing the efforts of the university and government. 

Teamwork needed to progress from access to success

Teamwork such as this is needed on all levels to transform the educational landscape in our country. As institutions of higher learning, we need to increasingly find innovative ways to become involved in the broader communities we serve – beyond our academic curricula.
 
In this way, we will finally be able to move beyond the question of access that has been dominating discourse and demonstration for so long and focus more specifically on ensuring that our students successfully exit the post-school system.

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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