Studying correlations between galaxy properties across different cosmic web environments

The cosmic web, a vast interconnected network of voids, sheets, filaments and clusters, serves as the large-scale scaffolding upon which galaxies form and evolve. It is plausible that these large-scale environments exert an influence on the galaxy properties. Using observational data from Sloan Digital Sky Survey (SDSS), we explored the correlations among key galaxy properties such as colour, stellar mass, specific star formation rate and stellar metallicity and examined whether these associations exhibit any dependence on the geometric environments of the cosmic web.