Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-02-15
Astronomy and Astrophysics
Astrophysics
Lecture to be published in "Formation and Evolution of Galaxies", eds. O. Le Fevre and S. Charlot, Les Houches School Series,
Scientific paper
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).
No associations
LandOfFree
Luminosity Functions and Field Galaxy Population Evolution does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Luminosity Functions and Field Galaxy Population Evolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminosity Functions and Field Galaxy Population Evolution will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-572323