
Hiring: 2 Research Assistants
Research Assistant in Astronomy & Astrophysics
THISâĻ

Morphological classification of Radio Galaxies using Semi-Supervised Group Equivariant CNNs
Out of the estimated few trillion galaxies, only around a millionâĻ

āĻĒāĻžāϞāϏāĻžāϰā§āϰ āĻŦāĻŋāĻŽā§ āϏā§āĻĨāĻžāύāĻāĻžāϞā§āϰ āĻĸā§āĻ
āĻāĻ āĻĨā§āĻā§ āĻĒā§āϰāĻžāϝāĻŧ ā§§ā§Šā§Ļ āĻā§āĻāĻŋâĻ

āĻ āĻĻā§āĻļā§āϝ āĻāϞā§āϤ⧠āĻāĻāĻžāĻļāĻāĻā§āĻāĻžāϰ āĻ āύā§āϤāϰ
āĻĒā§āĻĨāĻŋāĻŦā§āϰ āϏāĻŦāĻā§āϝāĻŧā§ āĻāĻžāϞ⧠āϰā§āĻĄāĻŋāĻâĻ

Mining mini-halos with MeerKAT I. Calibration and imaging
Radio mini-halos are clouds of diffuse, low-surface brightnessâĻ

The 1.28 GHz MeerKAT Galactic Center Mosaic
The inner $\sim 200$ pc region of the Galaxy contains a 4 millionâĻ

Primary beam effects of radio astronomy antennas â II. Modelling MeerKAT L-band beams
After a decade of design and construction, South AfricaâsâĻ

Constraining the intergalactic medium at z â 9.1 using LOFAR Epoch of Reionization observations
We derive constraints on the thermal and ionization states ofâĻ

Improved upper limits on the 21âcm signal power spectrum of neutral hydrogen at z â 9.1 from LOFAR
A new upper limit on the 21âcm signal power spectrum at aâĻ

The 1.28 GHz MeerKAT DEEP2 Image
We present the confusion-limited 1.28 GHz MeerKAT DEEP2 imageâĻ
