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29 March 2019 | Story Lacea Loader

No deregistration of students at the University of the Free State (UFS) will be effected until after the Financial Appeals Committee has concluded its process on 5 April 2019.

During a meeting between the university management and the Institutional Student Representative Council (ISRC) today, the following agreement was reached:

  1. The date for the submission of appeals has been extended to Tuesday 2 April 2019 at 12:00. No further extension will be given. The application form for the Financial Appeals Committee has previously been sent to the ufs4life email addresses of all provisionally registered students.
  2. Students who have appealed their National Student Financial Aid Scheme (NSFAS) outcomes will not be deregistered while awaiting the result of the outcome of their appeal.
  3. Verified final-year students who are provisionally registered will not be deregistered. This will be subject to verification by the Financial Appeals Committee. These students must also submit an appeal.
  4. All other categories of students must submit their appeals to the Financial Appeals Committee.

NB: The documentation mentioned above must be submitted to the Student Finance Office as indicated on the financial appeals form sent to students via their ufs4life email address.

The UFS has taken a pro-poor approach to assist students who are academically deserving. With this approach, the university’s fee structure is much less than that of many public institutions of higher learning in the country. Senior students are also supported through a provisional registration process that grants them the opportunity to pay a reduced amount in order to register, enabling them to fully participate in all activities while extension is provided to secure the necessary funding for their studies.

The university has made a number of concessions to ensure that students are not financially excluded during the 2019 academic year. Many of these concessions were raised by the ISRC on behalf of students and was agreed upon by the university management.  

These concessions include:

  1. Students who have confirmed NSFAS funding for 2019 with historic debt, are to secure registration. This has taken place before the announcement on 24 March 2019 by the Minister of Higher Education and Training, Naledi Pandor, that the historic debt of NSFAS students will be settled by the department.

     

  2. Students in the missing middle who received a gap grant in 2018, have been assisted to pay a lesser amount to register fully for 2019.

     

  3. Students with historic debt who are not receiving the gap grant have also been assisted to register for 2019. Acceptable payment plans for these students have been agreed upon with the university’s Student Finance Office.

     

  4. First-time entering students were assisted with a reduced first payment to enable them to register for 2019.

     

  5. Final-year students with historic debt of less than R20 000 who could not have been assisted in any of the above concessions explained above were allowed to register.

     

  6. Students who are provisionally registered and who could not find the necessary financial means, had the opportunity to submit appeals to the Financial Appeals Committee by 29 March 2019 to secure their registration. This committee comprises representatives of the university management, as well as members of the ISRC. This committee is scheduled to meet on 5 April 2019.

The above is evidence of the multi-layered efforts by the university to support academic deserving students as far as it is practically possible in order to avoid financial exclusion. Additionally, the university’s Student Finance Office has since the beginning of the academic year communicated extensively on the process with students who are at risk of being deregistered.  

Historically, less than 0,5% of registered students at the UFS are not able to find the necessary means to secure their registration.

To support students in their academic efforts, all matters pertaining to registration should be concluded by the end of the first term. A cut-off date is set by which all registration processes – including concessions – are to be concluded. This date – 31 March 2019 – has already been set in 2018, which is the result of consultation with all relevant stakeholders, including the IRSC.

This cut-off date has now been extended to Tuesday 2 April 2019 at 12:00.

Released by:

Lacea Loader (Director: Communication and Marketing)
Telephone: +27 51 401 2584 | +27 83 645 2454
Email: news@ufs.ac.za | loaderl@ufs.ac.za
Fax: +27 51 444 6393



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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