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Accurate measurement of exoplanetary masses is a critical step in addressing key aspects of NASA’s science vision. Astrometry can detect and measure masses of planets orbiting the target star. However, the signal for earth-analogs is in the sub-microarcsecond regime, well beyond our instrumentation. In this paper, we study part of an astrometry error budget for the HabEx Workhorse Camera and we propose a calibration approach to reach earth-analog sensitivity.
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Eduardo A. Bendek, Stefan Martin, Olivier Guyon, "Astrometry exoplanet detection using the Habex Workhorse camera," Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 1182317 (1 August 2021); https://doi.org/10.1117/12.2594996