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Tomographic Mapping of Cosmic Structure Growth with HIRAX and Rubin-LSST
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Kavilan
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University of KwaZulu-Natal (UKZN)
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(UKZN)
|
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Modelling high-energy gamma rays from theVela pulsar: curvature vs. synchro-curvature emission.
|
Monica
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North-West University (NWU)
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(NWU)
|
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Using MeerKAT HI data to establish the distances to the low surface brightness galaxies (LSBG) projected near the Fornax galaxy cluster
|
Chandreyee
|
North-West University (NWU)
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(NWU)
|
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Physical Properties of the Brightest Radio Galaxies in the MeerKAT-Herschel Protocluster Fields
|
Lerothodi
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University of the Western Cape (UWC)
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(UCT)
|
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Pulse decay time analysis of Fermi GBM gamma-ray bursts and magnetar giant flares
|
Dimakatso
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North-West University (NWU)
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(NWU)
|
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Galaxy Cluster Environments Traced by HI
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Mpati
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Rhodes University (RU)
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(UCT)
(UKZN)
(NWU)
|
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Automated follow-up of Transient Alerts with SAAO’s “Intelligent Observatory” program
|
Nicolas
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South African Astronomical Observatory (SAAO)
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(UCT)
(NWU)
|
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Peas in my Cosmic Fruit Salad? Investigating Young Galaxies from the Early Universe.
|
Nicolas
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South African Astronomical Observatory (SAAO)
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(UCT)
(NWU)
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