Chapitres
- Introduction
on strong lensing & the key
features used for probing the high
redshift Universe
- Strong
lensing modeling techniques
- Counting
lensed galaxies
- Probing
z>6 lensed galaxies
Résumé
| In
these 2 lectures, I will present
the topic of strong lensing and
how it can be used to probe the
high redshift Universe. I will
start with an introduction of
strong lensing and its key
features in studying the distant
Universe: magnification and source
plane dilution. I will then
explain how we do model strong
lensing system with a detailed
discussion of the constraints and
the different techniques used. I
will then explain how strong
lensing has been used to count
lensed galaxies and how we can
uses lenses to probe the high
redshift z>6 universe. |
Bibliographie
- Lens
modeling
- Mellier
et al 1993
- Kneib
et al 1993, 1996
- Jullo
et al 2007
- Coe
et al 2010
- Kneib
& Natarajan 2011
- Counting
Lensed Galaxies
- Altieri
et al 1999
- Blain
et al 1999
- Metcalf
et al 2003
- Knudsen
et al 2008
- Distant
Strong Lensed galaxies
- Ellis
et al 2001
- Kneib
et al 2004
- Richard
et al 2008
|
