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16 October 2023 | Story Leonie Bolleurs | Photo Sonia Small
Dr Grey Magaiza
Members involved in the Mountain-to-Mountain collaboration between the two institutions recently met at ASU to seek further collaboration beyond the completion of the current project. Pictured here is Dr Grey Magaiza, Lecturer and Head of the UFS Community Development Programme on the Qwaqwa Campus.

A three-year collaboration between the University of the Free State (UFS) and the Appalachian State University (ASU) in Boone, North Carolina in the United States, is coming to an end. The Mountain-to-Mountain Collaboration under the US University Partnership Initiative in South Africa is funded through the US Embassy and Consulates in South Africa.

From the start, this project had four specific objectives. It wanted to develop and offer an interdisciplinary master's degree in Mountain Studies and another in Community Development on the UFS Qwaqwa Campus. 

Furthermore, the collaboration included the installation of four climate monitoring stations in the Maloti-Drakensberg (South Africa), which will form part of a global network of climate change monitoring sites.  A further objective of the grant was to establish and offer a formal leadership mentorship programme for younger black women in academia and support services at the UFS.

According to Dr Grey Magaiza, Head of the UFS Community Development Programme (Qwaqwa), mutual synergies were identified due to the mountainous locations of both campuses (Qwaqwa and AppState), and the Mountain-to-Mountain project between the two universities was conceptualised. 

The stated objectives and more were achieved.

Grant implementation progress

Dr Magaiza says four meteorological stations have been installed in the Drakensberg and data is now streaming through for climate monitoring. 

The new master's programme in Community Development has successfully received accreditation from the South African Qualifications Authority (SAQA) and will be offered in 2024 or 2025, pending internal logistical processes. The new interdisciplinary master's degree in Mountain Studies is currently under review.

Additionally, an innovative mentorship programme was designed to support the academic and administrative development of 12 black female support and academic staff. Some have since completed their postgraduate studies, and as a result of this collaboration, an article has been accepted for publication in a book chapter. Other female colleagues have also improved their operational competencies in their workplaces. Dr Magaiza remarked, “This aspect of the project has created a network of aspiring and ambitious young female staff members seeking to expand their footprint.”

Also resulting from this initiative were two engaged scholarship initiatives with civic sector organisations in Qwaqwa. These engagements led to the formation of the Maluti-a-Phofung Sustainable Development Forum to engage on development issues in Qwaqwa.

Future steps

Dr Magaiza is excited about the future prospects created by this project. “There have been some signs of potential collaboration in the UFS Department of Geography, for example, Ethnobotany and the Centre for Appalachian Studies. All these partnerships will improve the academic profile of the UFS and enhance international collaborations,” he believes. 

He is also of the opinion that the increased internationalisation footprint brought about by this project, coupled with the much-needed partnership, will go a long way in enhancing the global standing of the UFS as a research-led institution. “The partnership will also see the entrance of the UFS into nuanced scholarly areas such as mountain studies and mountain medicinal research,” he says. 

Dr Magaiza feels a productive and impactful research agenda is critical for any university. “This partnership is supporting the UFS in achieving its strategic imperative to be a globally competitive research-led institution. The postgraduate programmes also enhance our student-centric appeal, while the mentorship programme reaffirms the institution’s ethic of care as critical to the upward mobility and support for female staff members.”

Members involved in the Mountain-to-Mountain collaboration between the two institutions recently met at ASU to seek further collaboration beyond the completion of the current project.

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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