Star Formation Histories¶
Parametric and stochastic star formation history models.
SFH with Double Bursts: Old and Recent Star Formation
SFH with Double Bursts: Old and Recent Star Formation
SFH Quenching Scenarios: Constant, Exponential, Sharp, and Burst+Decay
SFH Quenching Scenarios: Constant, Exponential, Sharp, and Burst+Decay
The Wrong-SEDModel Trap: Parametric Bias in Derived Quantities
The Wrong-SEDModel Trap: Parametric Bias in Derived Quantities