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
Realistic background galaxies (beyond skymaker) CP
use spiral model etc.
Multi bandwidth
compute colors
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.
realistic background distribution of galaxies CP
use adapthop catalogs
inversion vary cosmological parameters
Our purpose is to constraint the geometry of the lens (cosmology) and probe the clumpiness of the potential.