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Sakircan Beyazit

Modelling low-mass star-forming galaxies and determining galaxy stellar mass function and star-forming rate density as a function of mass in simulations to compare with observations of field dwarf galaxies using the latest and upcoming surveys.

Sakircan Beyazit graduated from the University of Manchester with an Integrated Masters in Physics with Theoretical Physics in July 2022.


His Masters project was focused on to analyse how dark matter, gas, and stars assemble in massive clusters, and how the baryon fractions depend on the cluster’s assembly history with the use of hydrodynamical simulations MACSIS.

He will be continuing to work on hydrodynamical simulations for his research project within LIV.INNO to model the low-mass star-forming galaxies