The Extreme Microlensing Event OGLE-2007-BLG-224: Terrestrial Parallax Observation of a Thick-Disk Brown Dwarf
A. Gould (Ohio State), A. Udalski (Warsaw Univ. Obs.), B. Monard, (Bronberg Obs.), K. Horne (St. Andrews), Subo Dong (Ohio State), N.Miyake, (Nagoya), K. Sahu (STScI), D.P. Bennett (Notre Dame), and the OGLE, MicroFUN,, RoboNet, MOA, PLANET collaborations (73 authors)

TL;DR
This paper reports the first detection of a thick-disk brown dwarf via an extreme microlensing event using terrestrial parallax, providing new insights into sub-stellar objects in the galaxy.
Contribution
It demonstrates the application of terrestrial parallax in extreme microlensing to measure the properties of a brown dwarf in the thick disk, a novel observational achievement.
Findings
Brown dwarf mass estimated at 0.056 solar masses.
Distance to the brown dwarf is approximately 525 parsecs.
The brown dwarf's velocity indicates it belongs to the thick disk.
Abstract
Parallax is the most fundamental technique to measure distances to astronomical objects. Although terrestrial parallax was pioneered over 2000 years ago by Hipparchus (ca. 140 BCE) to measure the distance to the Moon, the baseline of the Earth is so small that terrestrial parallax can generally only be applied to objects in the Solar System. However, there exists a class of extreme gravitational microlensing events in which the effects of terrestrial parallax can be readily detected and so permit the measurement of the distance, mass, and transverse velocity of the lens. Here we report observations of the first such extreme microlensing event OGLE-2007-BLG-224, from which we infer that the lens is a brown dwarf of mass M=0.056 +- 0.004 Msun, with a distance of 525 +- 40 pc and a transverse velocity of 113 +- 21 km/s. The velocity places the lens in the thick disk, making this the…
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