activity
19982025
most citedReflected Spectra and Albedos of Extrasolar Giant Planets I: Clear and Cloudy Atmospheres

315 citations · 799 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025

A Survey Of Model Fits to Brown Dwarf Spectra Through the L-T Sequence

Savanah K. Turner, Denise C. Stephens, Conner B. Scoresby +1

We fit archival near-infrared spectra of 305 brown dwarfs with atmosphere models from the Sonora and Phoenix groups. Using the parameters of the best-fit models as estimates for th…

astro-ph2008★ 26 cited

CLOUDS search for variability in brown dwarf atmospheres

B. Goldman, M. C. Cushing, M. S. Marley +21

Context: L-type ultra-cool dwarfs and brown dwarfs have cloudy atmospheres that could host weather-like phenomena. The detection of photometric or spectral variability would provid…

astro-ph2007★ 106 cited

Physical and Spectral Characteristics of the T8 and Later-Type Dwarfs

S. K. Leggett, M. S. Marley, R. Freedman +5

We use new and published near-IR spectra, with synthetic spectra, to derive physical properties of three of the latest-type T dwarfs. A new R~1700 spectrum of the T7.5 dwarf HD 365…

astro-ph2006★ 115 cited

Physical parameters of two very cool T dwarfs

D. Saumon, M. S. Marley, S. K. Leggett +8

We present new infrared spectra of the T8 brown dwarf 2MASS J04151954-0935066: 2.9-4.1 micron spectra obtained with the Infrared Camera and Spectrograph on the Subaru Telescope, an…

astro-ph2006★ 98 cited

3.6-7.9 um Photometry of L and T Dwarfs and the Prevalence of Vertical Mixing in their Atmospheres

S. K. Leggett, D. Saumon, M. S. Marley +4

We present new L' (3.75 um) photometry of six L and T dwarfs, and M' (4.70 um) photometry of ten L and T dwarfs, observed at Gemini Observatory, and new 3.55, 4.49, 5.73 and 7.87 u…

astro-ph2003★ 138 cited

JHK Magnitudes for L and T Dwarfs and Infrared Photometric Systems

Denise C. Stephens, Sandy K. Leggett

L and T dwarfs emit most of their radiation in the near infrared and their spectral energy distributions are dominated by strong molecular absorption bands. These highly structured…