2MASS J13243553+6358281 is an Early T-Type Planetary-Mass Object in the AB Doradus Moving Group
Jonathan Gagn\'e, Katelyn N. Allers, Christopher A. Theissen,, Jacqueline K. Faherty, Daniella C. Bardalez Gagliuffi, \'Etienne Artigau

TL;DR
This paper confirms that 2MASS J13243553+6358281 is a young, planetary-mass object in the AB Doradus group, providing new measurements of its properties and insights into the L/T transition at a known age.
Contribution
It presents new radial velocity and parallax data confirming membership in the AB Doradus group and constrains the L/T transition temperature at a specific young age.
Findings
Confirmed membership in AB Doradus group.
Estimated mass of 11-12 Jupiter masses.
L/T transition occurs at ~1150 K at 150 Myr.
Abstract
We present new radial velocity and trigonometric parallax measurements indicating that the unusually red and photometrically variable T2 dwarf 2MASS J13243553+6358281 is a member of the young (~150 Myr) AB Doradus moving group based on its space velocity. We estimate its model-dependent mass in the range 11-12 at the age of the AB Doradus moving group, and its trigonometric parallax distance of 12.7 1.5 pc makes it one of the nearest known isolated planetary-mass objects. The unusually red continuum of 2MASS J13243553+6358281 in the near-infrared was previously suspected to be caused by an unresolved L+T brown dwarf binary, although it was never observed with high-spatial resolution imaging. This new evidence of youth suggests that a low surface gravity may be sufficient to explain this peculiar feature. Using the new parallax we find that its absolute -band…
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