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26 November 2021 | Story Lacea Loader | Photo Sonia Small (Kaleidoscope Studios)
Prof Philippe Burger
Prof Philippe Burger.

The Council of the University of the Free State (UFS) approved the appointment of Prof Philippe Burger as Dean of the Faculty of Economic and Management Sciences for a five-year term during its quarterly virtual meeting on 26 November 2021. 

He is Pro-Vice-Chancellor: Poverty, Inequality and Economic Development, as well as Vice-Dean (Strategic Projects) of the Faculty of Economic and Management Sciences, and Professor of Economics at the UFS. 

Extensive experience

Prof Burger was a 2016/17 Fulbright exchange scholar at the Center for Sustainable Development, Earth Institute, Columbia University in the United States, with Prof Jeffrey Sachs as his Fulbright host, where he wrote a book titled Getting it right: a new economy for South Africa. The book was launched, with presentations at the International Monetary Fund (IMF), World Bank, and RAND Corporation in Washington DC, among others. In addition, he is a member of the Fiscal Policy and Financial Markets Task Team of the Lancet Commission on COVID-19. Co-chaired by the Head of the IMF’s Department of Fiscal Affairs and a former Minister of Finance of Chile, the task team of 11 members comprises economists from across the world, including two Nobel prize winners. 

From September 2012 to October 2014, Prof Burger was President of the Economic Society of South Africa. His publications include three more books and numerous academic articles on fiscal rules and fiscal sustainability, public-private partnerships, and macroeconomic and economic development policy. Together with IMF staff, he co-authored two IMF working papers. In 2009, the IMF invited him to spend a month at the IMF as a visiting scholar in the Fiscal Affairs Department (FAD), researching public-private partnerships and the Global Financial Crisis. For two months each in 2007, 2010, and 2012, he was seconded to the Organisation for Economic Co-operation and Development (OECD) in Paris, France, to work on public-private partnerships and capital budgeting, while in October 2011 he joined an OECD mission to Indonesia to conduct a regulatory review of Indonesia. 

Prof Burger was a member of the Panel of Experts of the South African National Treasury, in which capacity he co-authored a 20-year review of South African fiscal policy since 1994. From 2013 to 2018, he was a member of the South African Statistics Council, which oversees the work of Statistics South Africa. From 1 February 2018 to 31 January 2019, he acted as dean of the Faculty of Economic and Management Sciences at the UFS, and from 2002 to 2019 he was Head of the UFS Department of Economics. 

“With more than 27 years of experience in the higher-education sector, Prof Burger will bring a wealth of expertise, extensive networks, and partnerships, nationally and abroad, to the Faculty of Economic and Management Sciences and the UFS. His experience in the positions held at the university, as well as his extensive knowledge and understanding of the South African and global economy, places him in good standing to lead the faculty to be a formidable and impactful academic force nationally and abroad,” said Prof Francis Petersen, UFS Rector and Vice-Chancellor. 

“Prof Burger has the competencies required as dean of the Faculty of Economic and Management Sciences, leading it to exploit opportunities and deal with the challenges that the rapidly changing world presents to the UFS,” said Prof Petersen.  

Vision for the faculty

In response to his appointment, Prof Burger said, “I am humbled by this appointment and look forward to taking on this wonderful challenge. The faculty has a strong team of academics and administrative staff. With this team, I know we will create wonderful pathways for our students into the future and into the complex world of work. I also look forward to strengthening our research position and building the faculty as a nationally and internationally recognised research-strong faculty, as well as a faculty with a very strong Global South presence.”

Prof Burger succeeds the current Dean, Prof Hendri Kroukamp, who will be retiring at the end of February 2022.  

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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