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UFS implements interventions to increase diversity of researchers

03 January 2022 | Story André Damons | Photo Supplied

Seven supported academics from the Afromontane Research Unit (ARU) on the Qwaqwa Campus saw an increase in their H-indices (Google Scholar) during 2020.

Over the past few years, the university has implemented special interventions to increase the diversity of UFS researchers, including targeted appointments and focused research capacity development and support. Strategic interventions relating to National Research Foundation (NRF) rating resulted in the UFS having a well-established cohort of rated researchers.

According to the recent internal research report, the UFS has 144 researchers in the A, B and C categories (established according to NRF criteria), and 57 researchers under the age of 40 who are considered emerging researchers in the P and Y categories. This brings the total to 201 rated researchers in 2021, compared to 188 in 2020, and 164 in 2019. The university also has 57 Y-rated researchers.

Furthermore, the university submitted 51 applications to the NRF under the 2020 rating call, including 21 first-time applications (of which four were unsuccessful) and 26 who were invited to reapply to keep their ratings active (of which all were successful).

Prof Corli Witthuhn, Vice-Rector: Research and Internationalisation, says the UFS has been able to appoint outstanding young researchers over the past eight years. “Not only did these exceptional individuals contribute to our scholarship and research productivity, but they also increased our diversity. The increase in the diversity of our NRF-rated academics is an aspect of the research portfolio that I am most proud of,” says Prof Witthuhn.

Highlighted trends regarding NRF-rated researchers

• There has been a constant growth in the number of rated researchers, from 127 in 2016 to 202 in 2021.
• The majority of NRF-rated researchers (186 in 2021) are from the Bloemfontein Campus. The number of rated researchers from the Qwaqwa Campus increased from 4 in 2016 to 13 in 2021. The South Campus increased its number of rated researchers by two in 2021, with a current total of three rated researchers.
• The Faculty of Natural and Agricultural Sciences has the highest percentage of rated researchers (45%) in 2021, followed by the Faculty of the Humanities (29%).
• The percentage of rated white researchers declined from 92% in 2016 to 78% in 2021, and the rated black researchers increased from 6% in 2016 to 17% in 2021.
• The percentage of rated female researchers increased from 27% in 2016 to 34% in 2021.
• Rated researchers in the C2 and C3 rating categories declined slightly, from 52% in 2019 to 47% in 2021. There is still positive growth in the number of young (Y1/Y2) rated researchers – from 14% in 2016 to 27% in 2021.

Ratings and promotions

The university hosts a total of six South African Research Chairs (SARChI) funded by the NRF / Department of Science and Innovation (DSI), of which four are held by women. Three chairs are appointed in the Faculty of Natural and Agricultural Sciences and the Faculty of Education, while the faculties of Economic and Management Sciences and Health Sciences appointed one chair each. Two research chairs have been renewed for 2021-2025.

Seven supported academics from the Afromontane Research Unit (ARU) on the Qwaqwa Campus saw an increase in their H-indices (Google Scholar) during 2020, while one new Y1 NRF rating was awarded and another was increased to C2 level. Two ARU-supported academics achieved professorial status in the same year.

Twenty-five young academics on the cusp of NRF rating and promotion to the rank of Associate Professor are participating in the Future Professoriate Mentoring Programme, while the 25 participants of the ESAP group have completed their doctorates over the past three years and are working towards obtaining a Y-rating. As a result of the outstanding progress of the first cohort of the mentoring programme during 2020, a second cohort of ESAP scholars was selected in March 2021. More than 80% of the 75 group members are younger than 40 years.

Drs Frans Kruger and Lodewyk Sutton also received NRF Y-ratings in November 2020. The ESAP programme currently has three recipients of the FirstRand NRF Black African Advancement Fellowship Programme: Dr Eugene Baron (Practical Theology), Dr Mirriam Moleko (School of Mathematics and Science Education), and Dr Neo Pule (Psychology). Dr Lizemari Hugo from the School of Nursing also received a FAIMER (Foundation for Advancement of International Medical Education and Research) fellowship. Dr Mikateko Höppener (Centre for Development Support) has been selected to participate in the national DHET Future Professoriate Programme.

Publication output units show significant increase

The publication output units (books, conference proceedings, and journal articles) by UFS researchers, as measured and reported to the Department of Higher Education and Training (DHET), show consistent growth from 2016 to 2020. The output units increased significantly in 2019 and 2020 after a slight decrease in 2017.

There has also been a notable increase in books/chapters since 2018. Journal articles also showed constant growth from 2017 onwards, especially from 2019 to 2020, with a 20% growth in journal outputs visible; however, conference proceedings declined last year.

Main contributors

The faculties of Natural and Agricultural Sciences, the Humanities, and Theology and Religion remain the main contributors to the university’s publication output. Four faculties (Economic and Management Sciences, Education, Health Sciences, and Theology and Religion) increased their share of units in 2020 compared to the 2016-2019 period.

The journal output units generated from scholarly articles published in internationally indexed journals remained more than 80% (82% in 2017, 85% in 2018, 81% in 2019, and 85% in 2020). Only 15% of journal articles were published in South African indexed (DHET) journals (compared to 24% in 2016). Since 2016, there has been a clear shift towards publications in internationally indexed journals.

The following nine in-house journals are being administered by the UFS:

Acta Academica (editor: Henning Melber), Acta Structilia (editor: K Kajimo-Shakantu), Acta Theologica (editor: Jan-Albert van den Berg), Communitas (editor: Willemien Marais), Journal for Juridical Science (editor: Bradley Smith), Journal for Translation Studies in Africa (editor: Kobus Marais), Perspectives in Education (editor: Jan Nieuwenhuis), Southern Journal for Contemporary History (editor: Neil Roos), and Town and Regional Planning (editor: Maléne Campbell).

All are DHET-accredited, except for the Journal for Translation Studies in Africa, a new KovsieJournals title.

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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