The simulated data can be found on the WG0 Wiki here. So, if you are not yet a member of WG0, you should sign up on tasoc.dk to access the simulated data.
With the simulated data we would like to address the following questions:
- How do we remove cosmic rays from 20s data?
- How do we estimate sky-background from 20s data? - what is the needed size of postage stamps?
- How do we properly estimate the sky-background in large fields (FFIs), with varying amounts of crowding?
- How do we best define pixel-mask for targets in postage-stamps and FFIs, and this in fields with different amounts of crowding?