Third-Generation Calibrations for MeerKAT Observation

Superclusters and galaxy clusters offer a wide range of astrophysical science topics with regards to studying the evolution distribution galaxies, intra-cluster magnetization mediums, cosmic ray accelerations large scale diffuse radio sources all in one observation. Recent developments new telescopes advanced calibration software have completely changed data quality that was never possible old generation telescopes. Hence, observations superclusters are very promising avenue gather rich information large-scale structure (LSS) their formation mechanisms. These newer wide-band field-of-view (FOV) require state-of-the-art analysis procedures, including imaging, order provide deep high dynamic (DR) images which study faint emissions supercluster environments. Sometimes, strong point hamper limit achievement DR. In this paper, we shown DR improvements around MeerKAT observation Saraswati by applying third-generation (3GC) techniques using CubiCal killMS software. We also calculated statistical parameters quantify sources. This advocates for use maximize scientific returns from new-generation