Chapitres
- Theory
of flux- and surface-brightness
anomalies due to mass substructure
in strong lens galaxies
- Observational
effects of mass substructures in
strong lens galaxies and optimal
observational strategies.
- Modeling
of and inferences about mass
substructure in strong lens
galaxies.
Résumé
In
this series of three lectures on
mass-subtructure in strong lens
galaxies I will (i) introduce the
theory basis of flux and
surface-brightness anomalies in
lensed image due to mass
subtructure, (ii) illustrate the
effects of mass substructure in a
number of systems that show these
anomalies and what observational
strategies should be followed to
distinguish these from other
effects, and (iii) discuss how
these anomalies can be modeled
(individually or statistically) to
derive constraints on the
substructure properties, their
mass function and potentially
their evolution with cosmic time.
These three topics will be
sequentially covered in 3x1hr
lectures. |
Bibliographie
The
lecture slides will function as notes
and will include references to relevant
papers and books.
|