Mass measurement of a single unseen star and planetary detection efficiency for OGLE 2007-BLG-050
V. Batista, Subo Dong, A. Gould, J.P. Beaulieu, A. Cassan, G.W., Christie, C. Han, A. Udalski, W. Allen, D.L. DePoy, A. Gal-Yam, B.S. Gaudi,, B. Johnson, S. Kaspi, C.U. Lee, D. Maoz, J. McCormick, I. McGreer, B. Monard,, T. Natusch, E. Ofek, B.-G. Park, R.W. Pogge, D. Polishook

TL;DR
This study measures the mass of an unseen star using microlensing data and evaluates the event's sensitivity to detecting planets, finding high sensitivity to Neptune-mass planets but no planetary signatures.
Contribution
First precise mass estimate of an isolated unseen object via microlensing, enabling physical unit planet detection efficiency analysis.
Findings
Measured lens mass as 0.50 +/- 0.14 M_Sun
High sensitivity to Neptune-mass planets
Excluded Jupiter and Neptune-mass planets in certain ranges
Abstract
We analyze OGLE-2007-BLG-050, a high magnification microlensing event (A ~ 432) whose peak occurred on 2 May, 2007, with pronounced finite-source and parallax effects. We compute planet detection efficiencies for this event in order to determine its sensitivity to the presence of planets around the lens star. Both finite-source and parallax effects permit a measurement of the angular Einstein radius \theta_E = 0.48 +/- 0.01 mas and the parallax \pi_E = 0.12 +/- 0.03, leading to an estimate of the lens mass M = 0.50 +/- 0.14 M_Sun and its distance to the observer D_L = 5.5 +/- 0.4 kpc. This is only the second determination of a reasonably precise (<30%) mass estimate for an isolated unseen object, using any method. This allows us to calculate the planetary detection efficiency in physical units (r_\perp, m_p), where r_\perp is the projected planet-star separation and m_p is the planet…
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