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30 August 2022 | Story Edzani Nephalela | Photo Lethabo Machabaphala
From the left; Dr Marinkie Madiope, UFS South Campus Principal and founder of the UFS Women's Forum; Advocate Nthabiseng Sepanya-Mogale, Commissioner for Gender Equality: Free State province and Advocate at Oxford Chambers; Dr Molapo Qhobela, UFS Vice-Rector: Institutional Change, Strategic Partnerships, and Societal Impact, Pinky Kekana, Deputy Minister in the Presidency, and Zola Thamae, Acting Head of the Free State Department of Sport, Arts, Culture and Recreation.

“Most people believe that Women's Month celebrations are primarily for women, because issues discussed during these events are related to women. However, have you considered including men in these discussions to achieve gender equality? Do men understand how women want to be treated and cared for?” Pinky Kekana, Deputy Minister in the Presidency, spoke during the Women’s Month commemoration at the University of the Free State (UFS) South Campus on 16 August 2022.

This was the first gender-inclusive event, following the collaboration between the UFS Women's Forum, South African Women in Dialogue (SAWID), and Grootvlei Correctional Services

Some of the delegates who attended this prestigious event, included Dr Marinkie Madiope, UFS South Campus Principal and founder of the UFS Women's Forum; Advocate Nthabiseng Sepanya-Mogale, Commissioner for Gender Equality: Free State province and Advocate at Oxford Chambers; Zola Thamae, Acting Head of the Free State Department of Sport, Arts, Culture and Recreation; and Commissioner Jacky Reid-Moses, Correctional Services Area Commissioner for the Free State and Northern Cape regions.

Following the welcome by Dr Molapo Qhobela, UFS Vice-Rector: Institutional Change, Strategic Partnerships, and Societal Impact, Thandeka Mosholi, Assistant Director: School of Open Learning, deliberated the significance of women. She emphasised that women do more than bear children; they are also specialists in their fields and should be regarded for various managerial roles. 

“There are many opportunities for women, and men should not feel threatened when women occupy them; rather, they should support and encourage them, as they strive to be the best they can be. Generational equality should be used as a catalyst for us to drive gender equality. We need to be innovative and guarantee that boys and girls participate in things like domestic duties from a young age,” Mosholi stressed.

However, gender-based violence (GBV), sexual harassment, and murder are still significant issues, with various organisations trying to address and curb these socio-economic ills. Advocate Sepanya-Mogale said that it has become increasingly challenging to feel safe even in our own comfortable spaces. “If there are pastors and teachers out there who are taking advantage of our children, then we will continue to look over our shoulders. What happened to churches being our place of refuge and old generation teachers being faces of the community?” said Advocate Sepanya-Mogale. 

All the speakers encouraged women to take a position in the community, solidify their relationships, assimilate into the world of innovation and 4IR, and invite males into conversations that serve women's interests.

(From Left: Thandeka Mosholi, Assistant Director: School of Open Learning UFS; Dr Marinkie Madiope; Advocate Nthabiseng Sepanya-Mogale; Dr Molapo Qhobela; Pinky Kekana; Zola Thamae, and Spa Kabane, Director at the Free State Office of the Premier. Photo: Lethabo Machabaphala)

Educational session and future endeavours 

In addition to the commemoration, this event was concluded with an educational session dialogue. This session was divided into four groups, including both males and females, tapping into real-life experiences. It addressed issues of peace and security, facilitated by SAWID; rehabilitation and integration of inmates into communities, by the Grootvlei Correctional Management Unit; financial management, by Standard Bank; and GBV, enabled by the UFS Women’s Forum.

The perspectives and experiences shared by the attendees will be collated by the facilitators and handed over to the Deputy Minister in the Presidency to guide her strategy and plan.
 

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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