Photometry and Proper Motions of M, L, and T Dwarfs from the Pan-STARRS1 3$\pi$ Survey
William M. J. Best, Eugene A. Magnier, Michael C. Liu, Kimberly M., Aller, Zhoujian Zhang, W. S. Burgett, K. C. Chambers, P. Draper, H., Flewelling, N. Kaiser, R.-P. Kudritzki, N. Metcalfe, J. L. Tonry, R. J., Wainscoat, C. Waters

TL;DR
This paper presents a comprehensive catalog of nearly 10,000 M, L, and T dwarfs from the Pan-STARRS1 survey, providing new proper motions, photometry, and insights into their kinematics and colors, significantly enhancing the data available for ultracool dwarf studies.
Contribution
The study offers the largest homogeneous proper motion dataset for L and T dwarfs, combining multiple surveys to improve accuracy and coverage, and provides detailed color and kinematic analysis of ultracool dwarfs.
Findings
Median proper motion precision of 2.9 mas/yr.
Largest sample of L dwarfs detected at blue wavelengths.
Bluer late-M and L dwarfs tend to have higher tangential velocities.
Abstract
We present a catalog of 9888 M, L and T dwarfs detected in the Pan-STARRS1 3 Survey (PS1), covering three-quarters of the sky. Our catalog contains nearly all known objects of spectral types L0-T2 in the PS1 field, with objects as early as M0 and as late as T9, and includes PS1, 2MASS, AllWISE, and Gaia DR1 photometry. We analyze the different types of photometry reported by PS1, and use two types in our catalog to maximize both depth and accuracy. Using parallaxes from the literature, we construct empirical SEDs for field ultracool dwarfs spanning 0.5-12 m. We determine typical colors of M0-T9 dwarfs, and we highlight the distinctive colors of subdwarfs and young objects. Our catalog includes 492 L dwarfs detected in , the largest sample of L dwarfs detected at such blue wavelengths. We combine astrometry from PS1, 2MASS, and Gaia DR1 to calculate new proper…
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