Straddling the traditional realms of the planets and the stars, objects below the edge of the
main sequence have such unique properties, and are being discovered in such quantities …

Previous computations of low-temperature Rosseland and Planck mean opacities from
Alexander & Ferguson are updated and expanded. The new computations include a more …

We generate theoretical albedo and reflection spectra for a full range of extrasolar giant
planet (EGP) models, from Jovian to 51 Pegasi class objects. Our albedo modeling utilizes …

We present a comprehensive description of the theory and practice of opacity calculations
from the infrared to the ultraviolet needed to generate models of the atmospheres of brown …

We present a comprehensive theory of the spectra and atmospheres of irradiated extrasolar
giant planets. We explore the dependences on stellar type, orbital distance, cloud …

Global maps of Jupiter's atmospheric temperatures, gaseous composition and aerosol
opacity are derived from a programme of 5–20 µm mid-infrared spectroscopic observations …

In this paper we review current ideas about the composition, horizontal and vertical
distribution, and microphysical properties of clouds and aerosols in Jupiter's upper …

Exoplanets that receive stellar irradiance approximately equal to Earth's or less have been
discovered and many are suitable for spectral characterization. Here, we focus on the …

The highest spatial resolution Voyager IRIS spectra are used to produce zonal averages of
the temperature at the 150-and 270-mb pressure levels, of the para-hydrogen fraction at 270 …

The global distribution of phosphine (PH3) on Jupiter and Saturn is derived using 2.5 cm− 1
spectral resolution Cassini/CIRS observations. We extend the preliminary PH3 analyses on …