Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
04 September 2025 | Story Lilitha Dingwayo | Photo Lunga Luthuli
Bibi Essop
Bibi Essop, newly elected Universal Access Officer of the Bloemfontein Campus CSRC, celebrates her election as a representative of CUADS and students living with disabilities at the UFS.

The University of the Free State (UFS) community proudly celebrates the appointment of Bibi Essop as the newly elected Campus Student Representative Council Universal Access Officer on the Bloemfontein Campus – a role of immense importance for inclusivity, representation, and student advocacy.

Living with brittle bone syndrome, Essop brings both personal insight and leadership to her portfolio, representing the Centre for Universal Access and Disability Support (CUADS). Her election is not only a personal milestone but also a testament to the university’s growing recognition of the importance of visible leadership by students with disabilities.

By stepping into this position, Essop embodies the empowerment of students who navigate both academic life and unique personal challenges. “This is the pinnacle of my achievements this year, as I have been working towards this for the past three to four years,” she says.

She emphasises that her first priority was to understand the needs of the community she represents. “I had to make sure I know the people I represent, which gave me the opportunity to learn about the other four cohorts on our campus: students with visual impairment, hearing impairment, and learning difficulties, since I am a part of the mobility impairment cohort,” she explains.

The role of Universal Access Officer is vital in ensuring that the needs of students with disabilities remain central to discussions about inclusivity, campus infrastructure, and academic support. Essop is determined to challenge misconceptions about the position. 

“Many people assume my portfolio is restricted to CUADS students only, whereas it is so diverse that it needs to be incorporated in every other portfolio. Accessibility at every event is essential for students living with disabilities,” she says. “Many students do not attend events because they presume that they will not be accommodated.” 

Looking beyond academics, Essop hopes to work closely with fellow CSRC members to ensure inclusivity across all aspects of student life. One initiative she is particularly excited about is Casual Day on 5 September 2025 - a celebration of different disabilities aimed at fostering awareness, education, and integration among all students. 

“The CSRC has reach and influence across all three campuses. By partnering with them, CUADS can amplify its work, ensure consistent messaging, and create opportunities for engagement that are student-driven. This collaboration allows us to step outside of formal support channels and become part of broader campus conversations, events, and initiatives,” says Mosa Moerane who is the liaison, advocacy and awareness officer for CUADS. 

Moerane explains that there are differences in challenges faced by students with disabilities on three campuses. “Bloemfontein, being the largest campus, often presents challenges around scale- serving a higher number of students with diverse needs. South Campus has its own dynamics, with many first-year students who may still be navigating disclosure and adjustment. Qwaqwa students face unique geographical and infrastructural challenges. CUADS responds by tailoring support through assistive technology, academic accommodations, or advocacy for improved accessibility while keeping the student’s lived experience at the centre,” said Moerane.

“The aim is always to make students in Qwaqwa and South Campuses feel as included as those in Bloemfontein. Also having offices at South Campus and Qwaqwa Campus with CUADS Coordinators assists in ensuring that our students are supported similarly to those on Bloemfontein Campus,” she added.

As UFS continues its journey towards greater inclusivity, Essop’s appointment serves as a reminder of the importance of representation across all student cohorts. It affirms that every voice, regardless of background or circumstance, deserves to be heard.

The university congratulates Bibi Essop on this well-deserved achievement. Her leadership represents a step towards ensuring that universal access is not just a policy, but a lived reality for all UFS students. 

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.

We use cookies to make interactions with our websites and services easy and meaningful. To better understand how they are used, read more about the UFS cookie policy. By continuing to use this site you are giving us your consent to do this.

Accept