AETC - Example 2 : Star cluster
Simulation of J-band observations of a star cluster
in a nearby galaxy as would be obtained with
MICADO@
E-ELT.
The total exposure time is 3h This simulation was used
in
Gullieuszik et al. (2014, A&A).
The input star list consists of two components:
- the host galaxy body: spatially uniform distribution of stars. Magnitudes are calculated assuming a constant star formation rate
over the last 12 Gyr,
- the star cluster: stars are distruted according to a King-like profile. Magitudes are taken along theoretical isocrones obtained with the CMD web interface.
details can be found in
Gullieuszik et al. (2014, A&A).