Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference

We develop a framework for using clustering-based redshift inference (cluster-z) to measure the evolving galaxy luminosity function (GLF) and galaxy stellar mass function (GSMF) using WISE W1 (3.4\mu m) mid-infrared photometry and positions. We use multiple reference sets from the Galaxy And Mass Assembly (GAMA) survey, Sloan Digital Sky Survey... Show more