2 papers
astro-ph.GA2024
RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution
Elizaveta Sazonova, Cameron R Morgan, Michael Balogh +13
Structural disturbances, such as galaxy mergers or instabilities, are key candidates for driving galaxy evolution, so it is important to detect and quantify galaxies hosting these…
astro-ph.GA2024
The quiescent population at : Environmental impact on the mass-size relation
M. Figueira, M. Siudek, A. Pollo +5
How the quiescent galaxies evolve with redshift and the factors that impact their evolution are still debated. It is still unclear what the dominant mechanisms of passive galaxy gr…