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23 July 2024 | Story Teboho Mositi | Photo Yonela Vimba
Academic Advising Office 2024
Bongumusa Zwane, one of the academic advisers, giving advice to students.

The Academic Advising Office in the Centre for Teaching and Learning (CTL) on the University of the Free State (UFS) Qwaqwa Campus hosted an Academic Advising activation under the theme: Unombuzo? Tloho o tlo botsa adviser ya hao for undergraduate students on 12 July 2024 in preparation for the second semester.

The event was aimed at assisting students to reach their full potential and strive for academic success. It marked the starting point for students to prepare for the second semester of their academic year in stride.

Increase student use of academic advising services

CTL aims to advance evidence-based innovation that promotes excellence in learning and teaching for student access with success.

The objective of the activation was to increase the visibility of academic advising on the Qwaqwa Campus. The goal was also to increase students’ use of the various general academic advising services. The Advising Office noticed that not many students attended general advising sessions in the last semester, which inspired the activation as well as the introduction of the newly appointed transition advisers.

The Advising Office urges students to attend time management and study strategy sessions. The office also assists students in collaboration with the faculties, Student Counselling and Development, residences, the No Student Hungry office, Career Services, and other stakeholders at the university.

Success of the event

The event was a great success, as 120 students showed up and had the opportunity to speak face to face to the advisers. Alongside the advisers, a curriculum adviser from the Faculty of The Humanities, representatives from University Estates, the CTL office, and Transition Development and Success were in attendance.

The advising team was able to introduce advising to students, listen to their concerns, and provide short general advising opportunities. Students were treated to some goodies at the event and were given a chance to enter a competition through a survey, which will result in four lucky students winning exciting prizes.  Students had a great time, taking pictures, videos, and dancing to the music at the venue.

If students missed this opportunity, there will be more opportunities to meet the team through advising pop-ups:

• 26 July 2024 – Dining Hall
• 2 August 2024 – UFS Taxi Rank
• 16 August – Outside Fulufhelo Residence

• 13 September – Notice boards near the Intsika Building

Where to find your advisers

• Intsika Building, Ground Floor, Offices: 0030, 0043, 0044

• Email address: AdvisingQQ@ufs.ac.za

The activation’s objectives were to

• increase the visibility of academic advising on campus;
• increase student use of academic advising services;
• make students aware of the services offered by Academic Advising; and
• share different ways with students to connect with the advising team and how to set up appointments with their advisers.

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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