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17 March 2021 | Story University Estates | Photo UFS Photo Archive
The UFS is committed to providing inclusive and accessible living, teaching, and learning spaces that are welcoming to all.

In accordance with its vision to be a university that is recognised across the world for excellence in academic achievement and human reconciliation, the University of the Free State (UFS) is committed to providing a universally accessible environment for all students, staff, and visitors on all three of its campuses. 

A sense of belonging and togetherness

Creating an accessible environment that is conducive and welcoming to everybody on the campuses – which were not designed with accessibility in mind – is not an easy task. When the principles of universal design and access are applied, the environment and spaces can be enjoyed by all users alike, creating a sense of belonging and togetherness. The common perception that accessibility only provides equitable access and opportunities for persons in wheelchairs is refuted by universal access, stating that it is to the advantage and for the use of everybody. Parents with infants in strollers, delivery persons with trolleys or carrying heavy material, library patrons carrying an armful of books, academic staff with wheeled (rolling) laptop bags, and older people all benefit from the availability of a ramp, elevator, or automated door. 

The current accessibility project of the UFS was initiated in 2009, evaluating the accessibility status of the UFS at the time. Priority inaccessible areas and spaces were identified and listed to be converted and improved over a period of five years, revising the list every year. The focus of the project was primarily on areas and spaces where most student activities take place, where specific needs and challenges have been identified, and where specific departments/divisions of the UFS have requested the improvement of access. The project does not only include access to buildings, but also accessible bathrooms, sufficient accessible parking spaces, accessible walkways, and accessibility within the classroom. The emphasis of the project is not only on wheelchair users and persons with mobility impairments, but also on creating an environment that can easily be navigated and used by everybody. 

All new infrastructure incorporates accessibility measures

University Estates updated the accessibility reports mid-2020 and identified project priorities up to 2024. Among other things, the key focus areas were to make all walkways wheelchair-friendly, to create ablution facilities for persons with disabilities, to install lifts in buildings, and to install ramps. All new infrastructure by default incorporates accessibility measures in the planning stage.

On the South Campus, ramps were installed around the campus and pathways were made wheelchair-friendly. Entrances to existing lecture halls and other buildings have also been made more user-friendly for persons with disabilities. Additional to the above-mentioned initiatives, the institution has also embarked on a project that seeks to assist the visually impaired to better navigate the campus.

For our Qwaqwa Campus, immediate critical interventions that are in the planning stage and that should be done within the next year, are the creation of accessible ablution facilities in the Administration Building, library, and the Humanities and Education buildings.

WATCH video below: 


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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