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UFS hosts IASIA 2024 Conference on Public Administration

24 July 2024 | Story Valentino Ndaba | Photo Born2shoot

The University of the Free State (UFS) recently hosted the esteemed International Association of Schools and Institutes of Administration (IASIA) 2024 Conference. This notable event was organised by the UFS Department of Public Administration and Management, bringing together 280 academics, researchers, students, and practitioners to delve into the theme, Alternative Service Delivery and Sustainable Societal Responsiveness.

The relevance of this theme aligns with the Global and Africa Agendas 2030 and 2063, emphasising the need for a transformative dynamic to ensure that no one is left behind. The conference addressed the roles and challenges faced by public institutions, governments at all levels, public servants, and citizens worldwide. It highlighted the importance of managing uncertainties, challenges, and expectations in an era of complex reforms.

The conference featured a diverse and distinguished line-up of speakers, including Dr Najat Zarrouk, President of IASIA; Dr Sofiane Sahraoui, Director General of IASIA; Dr Ra’ed Benshams, President of the International Institute of Administrative Sciences (IIAS); Prof Francis Petersen, UFS Vice-Chancellor and Principal; and Geraldine Fraser-Moleketi, former Minister of Public Service and Administration of South Africa.

Advancing excellence

IASIA is dedicated to strengthening administrative capacity worldwide, advancing excellence in public administration education and training, and fostering the dissemination of innovative scholarly research and practices in governance and administration. The key objectives of the conference are to promote the exchange of knowledge on the evolution of public administration theory and practice and to facilitate comparative studies and the development of public administration theory. In addition, it aims to encourage innovation in ideas, methods, and techniques in public administration; strengthen the dialogue between academics and practitioners; as well as to develop and consolidate a community of public administration experts open to contributions from young researchers and public officials.

Sustainable solutions

“Hosting the IASIA Conference was pivotal for addressing sustainable solutions to service delivery challenges in the public sector, both globally and within the South African context. It provided a valuable platform for international exposure and networking for the UFS Department of Public Administration and Management, the broader UFS community, the Free State Provincial Government, and the South African as well as the global public administration and management fraternity,” said Prof Liezel Lues, UFS Professor of Public Administration and Management and rapporteur of the IASIA conference.

“It also included practitioners from South African universities and various public sector stakeholders, aligning with Vision 130's goal of making a significant social impact by fostering collaboration, knowledge sharing, and innovative solutions to local and global challenges,” she added.

Exploring the future of public service

A significant focus of the conference was exploring alternative service delivery models aimed at enhancing efficiency, responsiveness, inclusiveness, collaboration, co-production, and accountability. Public institutions and governments worldwide are grappling with numerous complex challenges, including the aftermath of the COVID-19 pandemic, geopolitical tensions, rapid urbanisation, climate change, inequality, youth disorientation, migration, and the digital revolution. These challenges have led to a critical lack of trust in public institutions and growing dissatisfaction with government performance.

Embracing alternative service delivery

Traditional government models have often struggled to meet citizens' needs and address these multifaceted issues. The conference highlighted the emergence of alternative service delivery models, emphasising the need to open public services to other actors and stakeholders, including the private sector, civil society organisations, and community groups. This approach seeks to enhance public service delivery through collaboration and innovation, ultimately striving to build a more responsive and sustainable society.

Click to view document Please click here to scan the QR code with the IASIA app for more information about the conference.

Watch the conference highlights video

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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