Astrometric monitoring of stars provides a promising method for discovery of low-mass planets around nearby Sun-like stars. The astronomical community has proposed several telescopes designed to perform high-precision astrometric observations. One limiting factor intrinsic to stars is the astrometric noise – or “jitter” – induced by surface stellar activity such as starspots and faculae. Despite […] The post Astrometric Exoplanet Detection Survi…
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