MSc AND PhD SCHOLARSHIPS FOR 2024 CENTRE FOR RADIO COSMOLOGY UNIVERSITY OF THE WESTERN CAPE
Download MSc AND PhD SCHOLARSHIPS FOR 2024 AT THE UNIVERSITY OF THE WESTERN CAPE Advert (pdf)
DEADLINE: 5 June 2023
The Centre for Radio Cosmology (CRC) at UWC is internationally recognised for its research in cosmology and galaxy evolution with MeerKAT, the Square Kilometre Array (SKA) and other telescopes (see astro.uwc.ac.za for further details). In 2023, the CRC research team includes 24 PhD/ MSc students and 11 postdoctoral fellows. Postgraduate students at the CRC work in a friendly and highly active research environment, with support from postdoctoral researchers.
The CRC is offering MSc and PhD scholarships for 2024. Successful applicants will be supervised by the team of CRC staff – Prof Ed Elson, Prof Lerothodi Leeuw, Dr Michelle Lochner, Prof Roy Maartens, Dr Siyambonga Matshawule, Prof Mario Santos, Prof Russ Taylor – on cutting-edge projects described briefly below. The available topics cover the Key Science goals of the SKA in cosmology and galaxy evolution – which are closely linked to the science goals of the major upcoming optical/ infrared surveys, such as DESI, Rubin/LSST and Euclid.
Students also have the possibility to be co-supervised by visiting professors Romeel Davé and Alkistis Pourtsidou (University of Edinburgh), Andrew Baker (Rutgers University), Matt Jarvis (Oxford University), Chris Clarkson (Queen Mary University of London), Stefano Camera (University of Turin), Phil Bull (University of Manchester) and Jingying Wang (Shanghai AO).
Students have opportunities to spend time in institutions abroad, in particular the ones just mentioned. Our research depends critically on data science and CRC students have access to the resources of our partner IDIA (Inter-University Institute for Data Intensive Astronomy) at UWC (www.idia.ac.za).
Applicants should email a single PDF document containing the following:
● Your CV.
● Transcripts of all university-level results.
● A brief statement of research interests (1 page). Please include all previous research experience, with details of the research project and supervisor. Please indicate which of the projects listed below you are interested in.
Applicants should also arrange for 2 reference letters to be sent directly to us by the same closing date.
Deadline: 5 June 2023
Preference will be given to students who fit into the demographic guidelines provided by the NRF and SARAO (South African Radio Astronomy Observatory).
Applicants should be South African citizens or permanent residents or citizens of Botswana, Ghana, Kenya, Madagascar, Mauritius, Mozambique, Namibia, Zambia.
Please check NRF rules for further eligibility requirements.
CRC scholarships are governed by SARAO. The 2024 levels for Full Cost of Study are:
MSc: 2 years at R189,158 per year
+ travel grant (up to R34k/year) + equipment grant (up to R32k for 2 years)
PhD: 3 years at R196,196 per year
+ travel grant (up to R41k/year) + equipment grant (up to R46k for 3 years)
Scholarships are granted on a year by year basis – i.e. continuing into the next year depends on satisfactory progress.
We offer a range of topics that tackle some of the big questions at the forefront of international cosmology and galaxy evolution. Research students in South Africa have a historic opportunity provided by MeerKAT (sarao.ac.za/science/meerkat/) and the future SKA (skatelescope.org/). In each topic below, there is a focus on the South African-based radio arrays MeerKAT, SKA, HERA (reionization.org) and HIRAX (hirax.ukzn.ac.za/). Some topics also look at the synergy of radio surveys with optical/ infrared galaxy surveys such as LSST, DESI and Euclid.
Training in cutting-edge theory, computation, simulations and data science will be provided.
1. Measuring neutral hydrogen (HI) across cosmic time with MeerKAT
We will use MeerKAT observations to make statistical detections of neutral hydrogen intensity on cosmological scales. There are several projects, from more technical data analysis to simulations of the signal. These include the measurement of the power spectrum and detection of the elusive Baryon Acoustic Oscillations (BAO) that can constrain Dark Matter and Dark Energy. The data analysis techniques use state of the art statistical methods including machine learning algorithms.
2. Unveiling the properties of HI galaxies
Using existing multi-wavelength observations and upcoming MeerKAT data, we will investigate the properties of HI in galaxies, giving new information on the HI and dark matter content of such systems. Projects may be focused on the dynamical modelling of galaxies, the statistical study of galaxies lying below the detection threshold, and methods of automated source finding using HI data cubes.
3. Probing the first galaxies in the Universe
We will investigate the Epoch of Reionization and use HERA data to probe the HI 21cm signal from the early Universe. There are several projects, including simulations of the signal, the observation pipeline and data analysis techniques (such techniques can include machine learning methods).
6. Probing Dark Energy
Dark Energy is thought to be the source of the accelerating expansion of the Universe, and its properties can be accurately measured by using the probes extracted from HI and other surveys – such as the power spectrum, bispectrum, BAO scale, redshift-space distortions (RSD) and weak lensing. There are several possible projects, associated with different probes.
7. Testing Einstein’s theory of General Relativity
We will explore whether the acceleration of the Universe is possibly not from Dark Energy, but instead from a modification of General Relativity – using the probes from HI and other surveys (especially RSD). There are several possible projects, associated with different probes and different tests.
8. Extracting ‘fossil’ information from the very early Universe
The primordial fluctuations generated in the first instants of the Universe provide the seeds for the formation of the large-scale structure. Imprints of the primordial Universe are ‘frozen’ in the large-scale distribution of matter. Using HI and other surveys, we can extract this ‘fossil’ information via some of the probes listed in Topic 6. There are several possible projects, associated with different probes and different properties.
We can also consider other topics on a case by case basis.