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Present and upcoming NASA missions will be intensively observing a selected,partially overlapping set of stars for exoplanet studies. Key physical andchemical information about these stars and their systems is needed for planningobservations and interpreting the results. A target star archive of such datawould benefit a wide cross-section of the exoplanet community by enhancing thechances of mission success and improving the efficiency of missionobservatories. It would also provide a common, accessible resource forscientific analysis based on standardized assumptions, while revealing gaps ordeficiencies in existing knowledge of stellar properties necessary forexoplanetary system characterization.

Final Report for SAG 22: A Target Star Archive for Exoplanet Science