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Theory for the Secondary Eclipse Fluxes, Spectra, Atmospheres, and Light Curves of Transiting Extrasolar Giant Planets
A. Burrows, D. Sudarsky, I. Hubeny
We have created a general methodology for calculating the wavelength-dependent light curves of close-in extrasolar giant planets (EGPs) as they traverse their orbits. Focussing on…
L and T Dwarf Models and the L to T Transition
Adam Burrows, David Sudarsky, Ivan Hubeny
Using a model for refractory clouds, a novel algorithm for handling them, and the latest gas-phase molecular opacities, we have produced a new series of L and T dwarf spectral and…
Theoretical Interpretation of the Measurements of the Secondary Eclipses of TrES-1 and HD209458b
A. Burrows, I. Hubeny, D. Sudarsky
We calculate the planet-star flux-density ratios as a function of wavelength from 0.5 microns to 25 microns for the transiting extrasolar giant planets TrES-1 and HD209458b and com…
Phase Functions and Light Curves of Wide Separation Extrasolar Giant Planets
David Sudarsky, Adam Burrows, Ivan Hubeny +1
We calculate self-consistent extrasolar giant planet (EGP) phase functions and light curves for orbital distances ranging from 0.2 AU to 15 AU. We explore the dependence on wavelen…
Theoretical Radii of Transiting Giant Planets: The Case of OGLE-TR-56b
A. Burrows, I. Hubeny, W. B. Hubbard +2
We calculate radius versus age trajectories for the photometrically-selected transiting extrasolar giant planet, OGLE-TR-56b, and find agreement between theory and observation, wit…
Spectra and Diagnostics for the Direct Detection of Wide-Separation Extrasolar Giant Planets
Adam Burrows, David Sudarsky, Ivan Hubeny
We calculate as a function of orbital distance, mass, and age the theoretical spectra and orbit-averaged planet/star flux ratios for representative wide-separation extrasolar giant…