The expected stellar populations in the Kepler and CoRoT fields
Leo Girardi, Mauro Barbieri, Andrea Miglio, Diego Bossini, Alessandro, Bressan, Paola Marigo, Thaise S. Rodrigues
TL;DR
This paper uses the TRILEGAL tool to predict the types and distributions of stars in the Kepler and CoRoT observational fields, aiding in the interpretation of data from these missions.
Contribution
It provides the first detailed predictions of stellar populations specifically tailored for the Kepler and CoRoT fields using a comprehensive synthesis model.
Findings
Predicted stellar type distributions for Kepler and CoRoT fields
Estimated star counts and brightness distributions
Insights into the expected stellar variability in these fields
Abstract
Using the stellar population synthesis tool TRILEGAL, we discuss the expected stellar populations in the Kepler and CoRoT fields
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