OGLE-2016-BLG-1045: A Test of Cheap Space-Based Microlens Parallaxes
I.-G. Shin, A. Udalski, J. C. Yee, S. Calchi Novati, G. Christie, R., Poleski, P. Mr\'oz, J. Skowron, M. K. Szyma\'nski, I. Soszy\'nski, P., Pietrukowicz, S. Koz{\l}owski, K. Ulaczyk, M. Pawlak, T. Natusch, R. W., Pogge, A. Gould, C. Han, M. D. Albrow, S.-J. Chung, K.-H. Hwang

TL;DR
This paper tests a cost-effective method for measuring microlens parallax using minimal space-based observations, demonstrating its accuracy in determining the properties of isolated objects in the Galaxy.
Contribution
It provides the first practical validation of the 'cheap space-based microlens parallax' method using real high-magnification microlensing data.
Findings
The method yields sufficient accuracy for physical property determination.
The test confirms the feasibility of using minimal space-based observations.
It enables building a complete sample of isolated objects for mass function studies.
Abstract
Microlensing is a powerful and unique technique to probe isolated objects in the Galaxy. To study the characteristics of these interesting objects based on the microlensing method, measurement of the microlens parallax is required to determine the properties of the lens. Of the various methods to measure microlens parallax, the most robust way is to make simultaneous ground- and space-based observations, i.e., by measuring the space-based microlens parallax. However, space-based campaigns usually require "expensive" resources. Gould & Yee (2012) proposed an idea called the "cheap space-based microlens parallax" that can measure the lens-parallax using only or space-based observations of high-magnification events. This cost-effective observation strategy to measure microlens parallaxes could be used by space-borne telescopes to build a complete sample for studying isolated…
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