 
	
	
		
	
	
	| M | T | W | T | F | S | S | 
|---|---|---|---|---|---|---|
| 23 | 24 | 25 | 26 | 27 | 28 | 1 | 
| 2 | 3 | 4 | 5 | 6 | 7 | 8 | 
| 9 | 10 | 11 | 12 | 13 | 14 | 15 | 
| 16 | 17 | 18 | 19 | 20 | 21 | 22 | 
| 23 | 24 | 25 | 26 | 27 | 28 | 29 | 
| 30 | 31 | 1 | 2 | 3 | 4 | 5 | 
Different regimes and improvement over litterature
 Strong, intermediate lensing & Weak lensing DA
 use GR
 Strong, intermediate lensing & Weak lensing DA
 use GR
 Realistic background galaxies (beyond skymaker) CP
 use spiral model etc.
 Realistic background galaxies (beyond skymaker) CP
 use spiral model etc.
 Multi bandwidth 
compute colors
 Multi bandwidth 
compute colors 
 clusters, filaments and galaxies 
  have lots of random zooms + different orientation and redshift combinations
 clusters, filaments and galaxies 
  have lots of random zooms + different orientation and redshift combinations
 volume lensing or plane lensing. CP
code true geodesic distorsion in volume.
 volume lensing or plane lensing. CP
code true geodesic distorsion in volume.
 realistic background distribution of galaxies CP
use adapthop catalogs
 realistic background distribution of galaxies CP
use adapthop catalogs
 inversion  vary cosmological parameters
 inversion  vary cosmological parameters
Our purpose is to constraint the geometry of the lens (cosmology) and probe the clumpiness of the potential.
 
	


