Uniform Forward-Modeling Analysis of Ultracool Dwarfs. II. Atmospheric Properties of 55 Late-T Dwarfs

Abstract

We present a large uniform forward-modeling analysis for 55 late-T (T7−T9) dwarfs, using low-resolution (R ≈ 50−250) nearinfrared (1.0 − 2.5 µm) spectra and cloudless Sonora-Bobcat model atmospheres. We derive the objects' effective temperatures, surface gravities, metallicities, radii, masses, and bolometric luminosities using our newly developed Bayesian framework, and use the resulting population properties to test the model atmospheres. We find (1) our objects' fitted metallicities are 0.3 − 0.4 dex lower than those of nearby stars; (2) their ages derived from spectroscopic parameters are implausibly young (10 Myr−0.4 Gyr);(3) their fitted effective temperatures show a similar spread as empirical temperature scales at a given spectral type but are ∼ 50 − 200 K hotter for T8 dwarfs; and (4) their spectroscopically inferred masses are unphysically small (mostly 1 − 8 M Jup ). These suggest the Sonora-Bobcat assumptions of cloudless and chemical-equilibrium atmospheres do not adequately reproduce late-T dwarf spectra. We also find a gravity-and a metallicity-dependence of effective temperatures as a function of spectral type. Combining the resulting parameter posteriors of our sample, we quantify the degeneracy between fitted surface gravity and metallicity such that an increase in Z combined with a 3.4× increase in log g results in a spectrum that has similar fitted parameters. We note the systematic difference between late-T dwarf spectra and Sonora-Bobcat models is on average ≈ 2% − 4% of the objects' peak J-band fluxes over the 1.0 − 2.5 µm range, implying modeling systematics will exceed measurement uncertainties when analyzing data with J-band S/N 50. Using our large, high-quality sample, we examine the spectral-fitting residuals as a function of wavelength and atmospheric properties to discern how to improve the model assumptions. Our work constitutes the largest analysis of brown dwarf spectra using multi-metallicity models and the most systematic examination of ultracool model atmospheres to date.