$Spitzer$ Microlensing Parallax for OGLE-2017-BLG-0896 Reveals a Counter-Rotating Low-Mass Brown Dwarf
Yossi Shvartzvald, Jennifer C. Yee, Jan Skowron, Chung-Uk Lee, Andrzej, Udalski, Sebastiano Calchi Novati, Valerio Bozza, Charles A. Beichman,, Geoffery Bryden, Sean Carey, B. Scott Gaudi, Calen B. Henderson, Wei Zhu,, Etienne Bachelet, Greg Bolt, Grant Christie, Dan Maoz

TL;DR
This study uses $Spitzer$ microlensing parallax data combined with ground observations to measure the mass and motion of a low-mass brown dwarf, revealing its potential origin and kinematic properties in the Galaxy.
Contribution
It presents the first measurement of an isolated brown dwarf's mass near the deuterium-fusion boundary using combined space and ground microlensing data.
Findings
Brown dwarf mass measured at ~19 M_J
Located ~4 kpc toward the Galactic bulge
Proper motion suggests possible halo origin
Abstract
The kinematics of isolated brown dwarfs in the Galaxy, beyond the solar neighborhood, is virtually unknown. Microlensing has the potential to probe this hidden population, as it can measure both the mass and five of the six phase-space coordinates (all except the radial velocity) even of a dark isolated lens. However, the measurements of both the microlens parallax and finite-source effects are needed in order to recover the full information. Here, we combine satellite parallax measurement with the ground-based light curve, which exhibits strong finite-source effects, of event OGLE-2017-BLG-0896. We find two degenerate solutions for the lens (due to the known satellite-parallax degeneracy), which are consistent with each other except for their proper motion. The lens is an isolated brown dwarf with a mass of either or . This is the lowest isolated-object…
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