A Statistical Survey of Peculiar L and T Dwarfs in SDSS, 2MASS, and WISE

We present the final results from a targeted search for brown dwarfs with unusual near-infrared colors. From a positional cross-match of SDSS, 2MASS and WISE, we have identified 144 candidate peculiar L and T dwarfs. Spectroscopy confirms that 20 of the objects are peculiar or are candidate binaries. Nine of the 420 objects in our sample are young ($\lesssim$200 Myr; 2.1%) and another 8 (1.9%) are unusually red with no signatures of youth. With a spectroscopic $J-K_s$ color of 2.58 $\pm$ 0.11 mag, one of the new objects, the L6 dwarf 2MASS J03530419+0418193, is among the reddest field dwarfs currently known and is one of the reddest objects with no signatures of youth known to date. We have also discovered another potentially very low gravity object, the L1 dwarf 2MASS J00133470+1109403, and independently identified the young L7 dwarf 2MASS J00440332+0228112, first reported by Schneider and collaborators. Our results confirm that signatures of low gravity are no longer discernible in low to moderate resolution spectra of objects older than $\sim$200 Myr. The 1.9% of unusually red L dwarfs that do not show other signatures of youth could be slightly older, up to $\sim$400 Myr. In this case a red $J-K_s$ color may be more diagnostic of moderate youth than individual spectral features. However, its is also possible that these objects are relatively metal-rich, and so have an enhanced atmospheric dust content.Comment: 27 pages, 7 figures, 5 tables, accepted to A

Brown Dwarf Atmospheres at High Cadence and Spectral Resolution: A Speed Limit on Brown Dwarf Rotation and a Spectroscopic Atlas of a 1050 K Atmosphere

Brown dwarfs are sub-stellar objects that form like stars but are not sufficiently massive to sustain hydrogen fusion in their cores. Characterized by cool, molecule-rich atmospheres, brown dwarfs demonstrate great diversity in spectroscopic appearance and share many properties with giant exoplanets. In this thesis I present two investigations: the first is a detailed photometric and spectroscopic study of the three most rapidly rotating brown dwarfs. The second examines a spectrum of a cool brown dwarf at unprecedented spectral resolution and signal-to-noise ratio to study the accuracy of theoretical model photospheres. Photometric monitoring of brown dwarfs has revealed that periodic variability is common and that brown dwarf atmospheres are composed of patchy, multi-layer clouds of varying thicknesses and compositions. In my first paper, I present the discovery of rapid photometric variability in three brown dwarfs from long-duration photometric monitoring with the Spitzer Space Telescope. Using moderate-resolution infrared spectroscopy I find a large degree of rotational broadening in each of these brown dwarfs, confirming that the rapid variability is due to fast rotation. These three brown dwarfs have the shortest rotation periods ever measured, between 1.08 and 1.23 hours. When put in context with the entire sample of brown dwarfs with known rotation periods, the clustering near the short-period end suggests that brown dwarfs are unlikely to spin much faster than once an hour. In my second paper, I study the atmospheric composition of a cold 1050 +- 50 K (T6-type) brown dwarf. Even the most up-to-date theoretical model photospheres do not completely reproduce observed spectroscopic features in cold brown dwarfs, limiting our ability to constrain their fundamental properties. I compare the observed data to these models to assess their accuracy and completeness. I draw conclusions about which models are the most reliable and which spectroscopic regions should be used to estimate physical parameters of cold brown dwarfs and, by extension, exoplanets. Additionally, I present the first unambiguous detections of hydrogen sulfide in an extra-solar atmosphere. These data comprise the most detailed atlas of spectroscopic lines in a cold brown dwarf available to date

Effects of Stimulant Medication, Incentives, and Event Rate on Reaction Time Variability in Children With ADHD

This study examined the effects of methylphenidate (MPH) on reaction time (RT) variability in children with attention deficit hyperactivity disorder (ADHD). Using a broad battery of computerized tasks, and both conventional and ex-Gaussian indicators of RT variability, in addition to within-task manipulations of incentive and event rate (ER), this study comprehensively examined the breadth, specificity, and possible moderators of effects of MPH on RT variability. A total of 93 children with ADHD completed a 4-week within-subject, randomized, double-blind, placebo-controlled crossover trial of MPH to identify an optimal dosage. Children were then randomly assigned to receive either their optimal MPH dose or placebo after which they completed five neuropsychological tasks, each allowing trial-by-trial assessment of RTs. Stimulant effects on RT variability were observed on both measures of the total RT distribution (ie, coefficient of variation) as well as on an ex-Gaussian measure examining the exponential portion of the RT distribution (ie, τ). There was minimal, if any, effect of MPH on performance accuracy or RT speed. Within-task incentive and ER manipulations did not appreciably affect stimulant effects across the tasks. The pattern of significant and pervasive effects of MPH on RT variability, and few effects of MPH on accuracy and RT speed suggest that MPH primarily affects RT variability. Given the magnitude and breadth of effects of MPH on RT variability as well as the apparent specificity of these effects of MPH on RT variability indicators, future research should focus on neurophysiological correlates of effects of MPH on RT variability in an effort to better define MPH pharmacodynamics