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Synthetic Photometry
Model:
POPSTAR with Chabrier IMF
PopStar Evolutionary synthesis models. Using IMF from Chabrier (2003). This grid of Single Stellar Populations covers a wide range in both, age and metallicity. The models use the most recent evolutionary tracks together with the use of new NLTE atmosphere models.
Model parameters
Flux type:(?)
Log(t): - (?)
Z: - (?)

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