A Search for L/T Transition Dwarfs With Pan-STARRS1 and WISE: Discovery of Seven Nearby Objects Including Two Candidate Spectroscopic Variables
William M. J. Best, Michael C. Liu, Eugene A. Magnier, Kimberly M., Aller, Niall R. Deacon, Trent J. Dupuy, Joshua Redstone, W. S. Burgett, K. C., Chambers, K. W. Hodapp, N. Kaiser, R.-P. Kudritzki, J. S. Morgan, P. A., Price, J. L. Tonry, and R. J. Wainscoat

TL;DR
This study uses combined optical and mid-infrared surveys to identify nearby L/T transition brown dwarfs, discovering seven objects and revealing variability and binary candidates, advancing understanding of these faint, complex objects.
Contribution
First wide-field search combining Pan-STARRS1 and WISE data to find L/T transition brown dwarfs within 25 pc, discovering seven new objects and candidate variables.
Findings
Identified seven nearby L/T transition brown dwarfs.
Detected spectroscopic and photometric variability in some objects.
Found candidate unresolved binary systems.
Abstract
We present initial results from a wide-field (30,000 deg^2) search for L/T transition brown dwarfs within 25 pc using the Pan-STARRS1 and WISE surveys. Previous large-area searches have been incomplete for L/T transition dwarfs, because these objects are faint in optical bands and have near-infrared colors that are difficult to distinguish from background stars. To overcome these obstacles, we have cross-matched the Pan-STARRS1 (optical) and WISE (mid-IR) catalogs to produce a unique multi-wavelength database for finding ultracool dwarfs. As part of our initial discoveries, we have identified seven brown dwarfs in the L/T transition within 9-15 pc of the Sun. The L9.5 dwarf PSO J140.2308+45.6487 and the T1.5 dwarf PSO J307.6784+07.8263 (both independently discovered by Mace et al. 2013) show possible spectroscopic variability at the Y- and J-bands. Two more objects in our sample show…
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