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26 November 2024 | Story Leonie Bolleurs | Photo Supplied
SARIMA presentations 2024
The UFS DRD team that attended and presented at the 2024 SARIMA conference in Maputo, Mozambique.

The Directorate Research Development (DRD) team from the University of the Free State (UFS) joined research management professionals from across the globe at the 2024 Southern African Research and Innovation Management Association (SARIMA) Conference held in September this year. This year's conference, hosted for the first time in Mozambique, focused on the theme, It Takes a Village to Raise a Child, highlighting the collective effort needed in research and innovation.

The UFS delegation participated in workshops on navigating change, unlocking research impact potential, tools and techniques for research and innovation project management, reviewing research-related contracts, and assessing associated risks. The Bill and Melinda Gates Foundation also led a training session, while other workshops explored strengthening global research partnerships and advancing competencies in research management.

Opportunity to share and learn about best practices

Boemo Segoje, Officer for RIMS, Ethics and Creative Outputs, reflected on the conference’s collaborative atmosphere, noting the opportunity to share and learn about best practices. Segoje, alongside Maricel van Rooyen, Senior Officer: Project Manager, RIMS and Ethics, presented a poster titled, Empower the Village with an Effective Research Management System, showcasing the university’s InfoEd Research Information Management System (RIMS). “Our audience was particularly impressed with how RIMS consolidates various research functions into one platform,” said Segoje.

Another UFS poster by Mpho Mashamba, Officer: RIMS Development and Maintenance, and Ethics and Katleho Nyaile from the Centre for Graduate Support (CGS) focused on Breaking Down Silos: Enhancing Interdepartmental Communication in Research Administration. They highlighted the need for collaboration within the university, emphasising how interdepartmental communication enhances research outcomes. “We referred to the importance of collaborating with other units, keeping a line of communication open, as well as engaging various stakeholders. This is especially important for a team like ours whose work impacts every faculty member,” said Mashamba.

Mandy Jampies, Senior Officer Postdoctoral Fellows presented on It Takes a Village: Fostering Collaborative Networks for Postdoctoral Fellow Management. This talk focused on building a ‘village’ for postdoctoral fellows by streamlining visa processes and establishing partnerships with other institutions, such as the University of Johannesburg. "The audience showed great interest in our initiatives, particularly the visa partnership with the Department of Home Affairs," Jampies remarked.

Jampies’s commitment to supporting postdoctoral fellows extended beyond her presentation. In addition to discussing ways to build a supportive ‘village’ through streamlined visa processes and collaborative partnerships, she also played a role in the science communication pre-conference workshop. Reflecting on this workshop, Jampies noted it as a standout moment. “Boemo Segoje and I had the chance to present on the university’s initiatives to boost research visibility through newsletters, social media and webinars,” she shared.

Sugan Moodley, Director of Research Development Finance, remarked that it was interesting to see the Research Management progression made by universities and to compare similarities, differences, strengths and weaknesses between the UFS and other universities.

AI, here to stay

Mashamba found inspiration in a session by the University of Ghana, where he drew parallels between Ghana’s research fund and the UFS Central Research Fund. “Learning from their experience will help enhance our processes here at the university,” he shared. A big fan of lifelong learning, he saw the conference as a great opportunity to pick up new ideas. He said, "I really made the most of every moment. For me, a few key things stood out. First off, having clear policies and standard operating procedures (SOPs) is important for making things run smoothly and getting more done.”

He continued, “As for AI, it’s definitely here to stay. I’m excited about the potential AI has to help streamline our work. Once it’s ready to be used effectively in the workplace, I’d love to bring it into our systems and even use it to improve what we’re already doing." Additionally, Dr Glen Taylor, the Director of Research Development at the UFS, expressed similar enthusiasm for the AI presentation, finding it an interesting insight into the future of research processes.

For Segoje, the conference also highlighted the importance of leadership in research management, referring to a session by the University of Pretoria on Ubuntu leadership. “The emphasis on Ubuntu aligns with the UFS’s values, emphasising the importance of sharing knowledge and empowering others,” she said.

Reflecting on the conference, Jampies concluded, “SARIMA 2024 was one of the best conferences I have attended, providing a wealth of practical knowledge that I can apply to improve my work portfolio.”

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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