A possible nearby microlensing stellar remnant hiding in Gaia DR3 astrometry

Massive galactic lenses with large Einstein Radii should cause a measurable astrometric microlensing e ffect, that is, a light centroid shift due to the motion of the two images. Such a shift in the position of a background star due to microlensing was not included in the Gaia astrometric model, and therefore significant deviation should cause Gaia's astrometric parameters to be determined incorrectly. Here we study one of the photometric microlensing events reported in the Gaia Data Release 3, GaiaDR3-ULENS-001, for which a poor goodness of Gaia fit and erroneous parallax could indicate the presence of an astrometric microlensing signal. Based on the photometric microlensing model, we simulated Gaia astrometric time series with the astrometric microlensing e ffect added. We find that including microlensing with an angular Einstein radius of theta(E) = 2.60(-0:24)(+0:21) mas (2.47(-0.24)(+0.28) mas) assuming a positive (negative) impact parameter, u(0), reproduces the astrometric quantities reported by Gaia well. We estimate the mass of the lens to be 1.00(-0.18)(+0.23) M-circle dot (0.70(-0.13)(+0.17) M-circle dot) and its distance 0.90(-0.11)(+0.14) kpc (0.69(-0.09)(+0.13) kpc), proposing the lens could be a nearby isolated white dwarf.