Objectives
This WP builds on the expertise gained in the other WP to prepare the tools in preparation of the EUCLID Deep survey. The whole WP will start later, in Year 3, in order that it can be built on the foundation of the results of other WPs.
Description of work
There will be two different aspects:
- To improv the existing simulator of the EUCLID data in order to simulate the data anticipated from EUCLID Deep survey. This will be undertaken both with the real the CANDELS imaging and grism data, as well as using other tools that start from entirely theoretical models of galaxies and spectra.
- Uses the tools developed in WP3 to analyse the synthetic data produced in WP6100, to test scalability and accuracy at the EUCLID level.