280510 UE Exercises in Stellar evolution and population sythesis (PI) (2014W)
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Note: The time of your registration within the registration period has no effect on the allocation of places (no first come, first served).
- Registration is open from Fr 19.09.2014 00:00 to Fr 17.10.2014 23:59
- Deregistration possible until Fr 17.10.2014 23:59
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Last modified: Mo 07.09.2020 15:42
*) simulating stellar populations of increasing complexity, starting from public isochrones
*) a simple case of CMD-reconstruction: a galaxy with a few bursts of star formation