R, I and L bands light curve of OGLE-2016-BLG-1093Lb

The precise measurement of the microlens parallax effect for this event, combined with the measurement of finite-source effects, leads to a direct measurement of the lens masses and system distance, M_host_=0.38-0.57M{sun} and m_p_=0.59-0.87MJup, and the system is located at the Galactic bulge (DL~8.1kpc).

Because this was a high-magnification event, we are also able to empirically show that the "cheap-space parallax" concept produces well-constrained (and consistent) results for |{pi}E|. This demonstrates that this concept can be extended to many two-body lenses. Finally, we briefly explore systematics in the Spitzer light curve in this event and show that their potential impact is strongly mitigated by the color constraint.