Prediction of Astrometric Microlensing Events during the Gaia Mission
Svea Proft, Markus Demleitner, Joachim Wambsganss

TL;DR
This paper identifies and verifies candidate stars for astrometric microlensing during Gaia's mission, highlighting the potential for precise stellar mass measurements and the challenges posed by erroneous proper motion data.
Contribution
It constructs a catalog of 43 confirmed astrometric microlensing candidates for Gaia, improving candidate verification and prediction methods.
Findings
96% of high proper motions were erroneous
43 confirmed candidates for Gaia microlensing
Potential to measure centroid shifts between 100 and 4000 microarcsec
Abstract
We identify stars with large proper motions that are potential candidates for the astrometric microlensing effect during the Gaia mission i.e. between 2012 and 2019. The effect allows a precise measurement of the mass of a single star that is acting as a lens. We construct a candidate list by combining information from several input catalogs including PPMXL, LSPM, PPMX, OGLEBG, and UCAC3. The selection of the microlensing candidates includes the verification of their proper motions as well as the calculation of the centroid shift of the source resulting from the astrometric microlensing effect. The assembled microlensing catalog comprises 1118 candidates for the years 2012 to 2019. Our analysis demonstrates that 96% of the (high) proper motions of these candidates are erroneous. We are thus left with 43 confirmed candidates for astrometric microlensing during the expected Gaia mission.…
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