- Lensed arcs of galaxies from COSMOS.
- Pin galaxies of the lens according to the properties of its density profile.
- Add noise and psf according to SDSS observation.
- Calibrating the flux values of the galaxies from COSMOS and SDSS.
- Inputting these simulated images into the pipeline and make it running.
- Try CFHTLens too? For example, use the mock catalog from SpaceWraps.
Notes of Some Discussion about Our Project
Coming soon...