Luminosity Functions and Field Galaxy Population Evolution

Abstract

Galaxy redshift surveys are outstanding tools for observational cosmology. Mapping the universe as outlined by galaxies leads to fundamental measurements which refine our knowledge of its structure and evolution. Redshift acquisition has undergone tremendous progress thanks to advances in technology, and redshift surveys appear nowadays as routine. Even though they may look simple at face-value, the strategy of a survey and the galaxy-selection criteria have crucial impacts on the interpretation of results. In this lecture, I concentrate on the galaxy luminosity function and its evolution. In particular I consider the luminosity function derived from optically magnitude-selected field galaxy redshift surveys. The aim is to describe the approach to designing state-of-the-art of galaxy surveys and their impact on measurements on luminosity functions. I start by discussing survey strategies, (Section 2). I continue by describing the data required (Section 3), and then review the different estimators to measure luminosity funtions (Section 4). I discuss the luminosity function evolution (Section 5) and I follow by summarizing the status of luminosity measurements (Section 6).