Photometric brown-dwarf classification. II. A homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 with accurate spectral types
N. Skrzypek, S.J. Warren, J.K. Faherty

TL;DR
This paper presents a large, homogeneous sample of 1361 L and T dwarfs with accurate spectral classifications, providing valuable data for understanding ultracool dwarfs and identifying peculiar objects.
Contribution
The study offers a new, extensive catalog of ultracool dwarfs classified with high accuracy using photometry, including 998 newly identified objects and detailed spectral and color information.
Findings
Sample is effectively complete to the magnitude limit for spectral types L0 to T8.
Identified a color discontinuity between L7 and L8 spectral types.
Discovered and characterized peculiar objects, including a low-gravity L2γ dwarf.
Abstract
We present a homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 (of which 998 are new), from an effective area of 3070 deg2, classified by the photo-type method to an accuracy of one spectral sub-type using izYJHKW1W2 photometry from SDSS+UKIDSS+WISE. Other than a small bias in the early L types, the sample is shown to be effectively complete to the magnitude limit, for all spectral types L0 to T8. The nature of the bias is an incompleteness estimated at 3% because peculiar blue L dwarfs of type L4 and earlier are classified late M. There is a corresponding overcompleteness because peculiar red (likely young) late M dwarfs are classified early L. Contamination of the sample is confirmed to be small: so far spectroscopy has been obtained for 19 sources in the catalogue and all are confirmed to be ultracool dwarfs. We provide coordinates and izYJHKW1W2 photometry of all…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Galaxies: Formation, Evolution, Phenomena
