Galaxy And Mass Assembly (GAMA): \mathbf{z \sim 0} Galaxy Luminosity Function down to \mathbf{L \sim 10^{6}~L_\odot} via Clustering Based Redshift Inference
In this study we present a new experimental design using clustering-based redshift inference to measure the evolving galaxy luminosity function (GLF) spanning 5.5 decades from L \sim 10^{11.5} to 10^6 ~ \mathrm{L}_\odot. We use data from the Galaxy And Mass Assembly (GAMA) survey and the Kilo-Degree Survey (KiDS). We... Show more
Galaxy And Mass Assembly (GAMA): $\mathbf{z \sim 0}$ Galaxy Luminosity Function down to $\mathbf{L \sim 10^{6}~L_\odot}$ via Clustering Based Redshift Inference