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most citedTheoretical Spectra and Light Curves of Close-in Extrasolar Giant Planets and Comparison with Data

299 citations · 537 across the 4 of their papers we have counts for

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astro-ph200872 cited

NLTE model calculations for the solar atmosphere with an iterative treatment of opacity distribution functions

M. Haberreiter, W. Schmutz, I. Hubeny

Modeling the variability of the solar spectral irradiance is a key factor for understanding the solar influence on the climate of the Earth. As a first step to calculating the sola…

astro-ph2007299 cited

Theoretical Spectra and Light Curves of Close-in Extrasolar Giant Planets and Comparison with Data

A. Burrows, J. Budaj, I. Hubeny

We present theoretical atmosphere, spectral, and light-curve models for extrasolar giant planets (EGPs) undergoing strong irradiation for which {\it Spitzer} planet/star contrast r…

astro-ph2007161 cited

A Systematic Study of Departures from Chemical Equilibrium in the Atmospheres of Substellar Mass Objects

Ivan Hubeny, Adam Burrows

We present a systematic study of the spectral consequences of departures from chemical equilibrium in the atmospheres of L and T dwarfs, and for even cooler dwarfs. The temperature…

astro-ph2005

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…

astro-ph2003

FUSE observations of G226-29: First detection of the H_2 quasi-molecular satellite at 1150A

N. F. Allard, G. Hébrard, J. Dupuis +4

We present new FUV observations of the pulsating DA white dwarf G226-29 obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). This ZZ Ceti star is the brightest one of i…

astro-ph2003

A comparison of DA white dwarf temperatures and gravities from FUSE Lyman line and ground-based Balmer line observations

M. A. Barstow, S. A. Good, M. R. Burleigh +3

Observation of the strengths and profiles of the hydrogen Balmer absorption series is an established technique for determining the effective temperature and surface gravity of hot…