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17 February 2023 | Story Valentino Ndaba | Photo UFS Photo Archive
The UFS Protest Protocol offers the university community safety guidelines during protests, including dos and don’ts for staff and students who are not demonstrating; acceptable and unacceptable behaviour during protests, and how to handle protests in accordance with standard operating procedures

The University of the Free State (UFS) recognises the right of students and staff members to peacefully assemble, picket, and protest in a way that does not interfere with the rights of other members of the university community. At the same time, the safety of all UFS staff and students is one of our top priorities.

The UFS Protest Protocol offers the university community safety guidelines during protests, including dos and don’ts for staff and students who are not demonstrating; acceptable and unacceptable behaviour during protests, and how to handle protests in accordance with standard operating procedures.

As a university, we continuously strive to create an inclusive environment where opposing views are accommodated, and the constitutional right to protest is respected. According to the UFS’s Vision 130 strategy, one of the key principles that drive the institution is social justice: “The university recognises that diversity goes together with a commitment to inclusivity, equity, and social justice. We therefore also commit to creating a culture of care and a vibrant space for, and acceptance of, constructive and critical engagement; where a diversity of often contested ideas and perspectives is not just tolerated, but also fostered through discussion and subsequent implementation.”

What should one do if a protest occurs?

1. Communicate: The university must be informed if it is to respond appropriately to protest action. If you are aware of ongoing or impending protest action, immediately inform the relevant 24/7 Protection Services operational centre.

2. Be informed: In order to respond appropriately to protest action (for your own protection and the protection of others), you need to know about impending or ongoing protests and stay informed on how it unfolds, via official UFS communication platforms and ConnectYard. The latter provides as-it-happens crisis alert notifications via WhatsApp.

3. Keep away: If at all possible, keep away from the area of the protest action. Try to keep others for whom you are responsible away as well.

4. Help others: If someone appears to be in danger or distress, intervene only if you are sure that it is safe for you to do so, and proceed calmly, without provoking protesters. Seek treatment for injuries. Should you or someone else suffer injuries of any kind during protest action, seek treatment from emergency services or Kovsie Health. Contact the Protection Services operational centres for any medical emergencies, so that they can activate the ambulance services according to available protocols.

5. Report: Report all incidents and damages to Protection Services at the numbers provided. It is important that non-protesting staff and students submit statements to the UFS investigating officers for the internal disciplinary process, to prevent similar occurrences in future. Be specific when providing a statement, to enable the investigating team to identify those involved in violent disruptions. Culprits cannot be brought to book if no evidence is available to link them to specific incidents. All reasonable steps will be taken to protect non-protesting staff and students testifying in disciplinary proceedings.

For advice on what to do and what not to do, read the UFS Protest Guidelines booklet. You can also watch the video below for more information:

 

Bloemfontein Campus
Protection Services: +27 51 401 2911 | +27 51 401 2634 | 0800 204 682
Ambulance: +27 80 005 1051 | 10177
Social worker: +27 73 182 3048
Kovsie Health: +27 51 401 2603

Qwaqwa Campus     
Protection Services: +27 58 718 5460 | +27 58 718 5175 | +27 58 718 5360
Ambulance: 10177
Social Worker: +27 58 718 5090 | +27 58 718 5091
Kovsie Health:   +27 58 718 5210                          

South Campus
Protection Services: +27 51 505 1217
Ambulance: +27 80 005 1051 | 10177
Social worker: +27 73 182 3048
Kovsie Health: +27 51 401 2603

 

 

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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