The detection and treatment of distance errors in kinematic analyses of stars
We present a new method for detecting and correcting systematic errors in the distances to stars when both proper motions and line-of-sight velocities are available. The method, which is applicable for samples of 200 or more stars that have a significant
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Schonrich_The_detection_and_treatment_of_2012.pdf||1.24 MB||Adobe PDF||Request a copy|
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