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31 July 2023 | Story Valentino Ndaba
GEAD Infographic

The Gender Equality and Anti-Discrimination Office (GEADO) is an integral part of the University of the Free State’s (UFS) Unit for Institutional Change and Social Justice. Its primary focus is to create a safe and inclusive environment for students and staff. The office plays a crucial role in shaping the student experience and in fostering inclusivity in student accommodation and residence environments.

The GEADO takes proactive steps to achieve this, including implementing guidelines and policies to address and prevent gender-based violence and sexual misconduct. It also conducts conscientisation workshops to raise awareness, challenge biases, and promote empathy among stakeholders.

“As an integral component of our initiatives, the GEADO implements proactive measures to foster safe spaces for students, through the establishment of its Sexual Offence Response Team (SORT) and sexual harassment guidelines,” said Dr Lentsu Nchabeleng, Deputy Director of the Gender Equality and Anti-Discrimination Office. She further emphasised, “These frameworks are formulated to tackle and prevent occurrences of gender-based violence and sexual misconduct, ensuring a secure, healthy, and conducive environment for both students and staff to flourish and develop as individuals and as a community.” The GEADO is currently reviewing the UFS Sexual Harassment, Sexual Misconduct, and Sexual Violence Policy to strengthen its commitment to a zero-tolerance stance on gender-based violence and sexual misconduct.

Beyond addressing specific incidents, the GEADO aims to cultivate an inclusive and socially just atmosphere across the UFS’s campuses. It closely monitors the environment, identifies trends, and stays updated on global and local interventions to positively impact its work.

The office is a driving force behind fostering a safe, inclusive, and socially just campus culture that embraces gender equality and combats discrimination. It partners with LGBTIAQ+ (lesbian, gay, bisexual, transgender, intersex, asexual, queer, and others) organisations like Free State Rainbow Seeds to further support its mission. Some of the programmes championed by the office include safety zone training, sexuality sensitisation, and diversity training.

Safe zone training

The Safe Zones@UFS project is modelled after a similar programme in the USA, specifically the Safe Zones Project at San Diego State University. Its purpose is to create a supportive and safe environment for individuals who identify as LGBTIAQ+.

Dr Nchabeleng said the project encompasses the training of faculty members and students to become Safe Zones allies, offering support to students, staff, as well as families and friends of individuals identifying as LGBTIAQ+. She emphasised that the role of Safe Zone allies involves providing assistance to LGBTIAQ+ students and staff during their coming-out process, serving as an informative resource for LGBTIAQ+ matters, advocating for LGBTIAQ+ rights, and acting as a referral point for other essential services, including medical and counselling support.

Sexuality sensitisation

Gender and sexuality sensitisation is crucial for fostering inclusive and respectful environments in educational institutions, workplaces, and communities. It involves raising awareness about consent, sexual minorities, and diverse gender identities, while addressing gender-based violence, sexual harassment, and misconduct. The approach includes consent education, understanding sexual minorities, exploring gender identities, combating gender-based violence and harassment, promoting safe spaces, challenging stereotypes, encouraging allyship, and promoting positive masculinity and femininity. Overall, these efforts create a more understanding and supportive community in which individuals of all genders and sexual orientations can thrive.

Diversity Training

The Diversity Training programme focuses on increasing awareness and understanding of diverse backgrounds and experiences. It includes workshops and training to address unconscious bias, promoting a fair and equitable environment. The goal is to create a sense of belonging, where everyone feels accepted and valued. The programme is flexible and can be customised for organisations or communities, and it can be delivered through various formats. Embracing diversity and inclusion can lead to better outcomes, improved teamwork, and the attracting of diverse talent. Overall, it fosters a culture of inclusivity and appreciation for diverse perspectives, benefitting both individuals and organisations.

Important contact information

Bloemfontein Campus: +27 51 401 3982

South Campus: +27 51 401 7544

Qwaqwa Campus: +27 58 718 5431

Toll-free number +27 80 020 4682

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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