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12 July 2023 | Story Dr Anchen Froneman | Photo Supplied
Odeion
Odeion School of Music (OSM) at the University of the Free State (UFS) will offer two new qualifications, namely the Advanced Diploma in Opera Studies and the Postgraduate Diploma in Music Performance from next year.

Over the past decade, the Odeion School of Music (OSM) at the University of the Free State (UFS) has been active in designing new qualifications and restructuring current offerings. The OSM introduced the Higher Certificate in Music Performance (in 2017) and a restructured Diploma in Music in 2018 to admit students without the necessary admission requirements for degree studies and develop the necessary skills in that regard. The purpose of these qualifications was to promote inclusivity in providing access to tertiary studies to students who developed musical skills at a more mature age for the first time. 

From next year, OSM will offer two new qualifications, namely the Advanced Diploma in Opera Studies and the Postgraduate Diploma in Music Performance. Applications are currently open and will close on 30 September. Classes will commence in February 2024. 

Dr Anchen Froneman, Programme Director and Senior Lecturer at OSM, says since the commencement of the Higher Certificate in Music Performance (in 2017) and the restructured Diploma in Music, the student intake included a high number of talented vocalists or late-developing instrumentalists. Many students in these programmes were already in their 20s, but through these programmes could develop their inherent talents and passions. Upon finishing the Diploma in Music, the students could then enter a degree qualification in music studies.

“However, the degree programmes are academically oriented while the Higher Certificate in Music Performance and Diploma in Music are vocational in nature. This disjunction led to the design of the Advanced Diploma in Opera Studies to provide a programme through which the students can access a NQF 7 level qualification in a shorter time than the current existing route through the degree programmes that requires another three or four years of study,” says Dr Froneman. 

The Advanced Diploma in Opera Studies

According to her, the Advanced Diploma in Opera Studies aims to prepare students completing the Diploma of Music for professional practice within a single academic year. This specialisation option attempts to enable students with the skillset to partake in Opera productions both locally and internationally as well as to develop an understanding of operatic activities within local communities and specifically to continuously develop young talent for future operatic careers. The modules in the programme include Performance Studies, Vocal Ensemble, Stage Craft and Language for Singers. To serve the teaching duties which are often carried out simultaneously with an operatic career, the modules of Repertoire and Method and Keyboard Skills are included. The Arts Management module serves the management of a professional opera and/or teaching career. The Introduction to Research Skills develops research and academic writing skills in view of possible further postgraduate studies. 

The Postgraduate Diploma in Music Performance

The Postgraduate Diploma in Music Performance, explains Dr Froneman, is a one-year qualification but has dual aims. Firstly, the programme will add to the offerings of the UFS that aims to widen access to tertiary education, especially considering the linear progression within vertical articulation possibilities from the Higher Certificate in Music Performance to the Diploma in Music, followed by the Advanced Diploma in Opera Studies that can eventually lead to the PGDip (Music Performance). Secondly, this qualification is partly directed at individuals with active careers in the music industry (both public and private sectors) who wish to advance performance skills and research ability. The qualification is designed to make a positive contribution towards expanding existing career opportunities for individuals completing the qualification. 

The ability to present two public concerts of high quality as a soloist or chamber musician will be developed using two recital modules. The Main Recital comprises of an approved programme 35 to 45 minutes (for vocalists and brass instruments) or 60 to 70 minutes (for all other instruments) as well as a Short Recital comprising an approved programme approximately 20 minutes (for vocalists and brass instruments) or 30 minutes (for all other instruments). Performance experts oversee and guide the preparation for these public concerts. The Viva Voce module will develop and evaluate a student’s ability to critically reflect upon and discuss musical works presented during the Main Recital.

The expert musician supervising the recital modules oversees this process in which understanding is fostered through practical experience, research, and application. The Structure Research Essay develops the student’s ability to contribute to performance-related scholarship by applying appropriate research methods and writing skills to reflect upon performance practices in, amongst others, historical, analytical, cultural, social or pedagogical aspects.

For more information on these qualifications and applications, please contact: 

Dr Anchen Froneman 
Programme Director and Senior Lecturer: Odeion School of Music 
Faculty: The Humanities
+27 51 401 2526

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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