Michael Line
0000-0002-2338-476X
33 papers found
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Forward and Inverse Modeling of the Emission and Transmission Spectrum of Gj 436b: Investigating Metal Enrichment, Tidal Heating, and Clouds
SPITZERPHASE CURVE CONSTRAINTS FOR WASP-43b AT 3.6 AND 4.5μm
Near-Infrared Emission Spectrum of Wasp-103b Usinghubble Space Telescope/Wide Field Camera 3
Developing Atmospheric Retrieval Methods for Direct Imaging Spectroscopy of Gas Giants in Reflected Light. I. Methane Abundances and Basic Cloud Properties
No Thermal Inversion and a Solar Water Abundance for the Hot Jupiter Hd 209458b Fromhst/Wfc3 Spectroscopy
On the Composition of Young, Directly Imaged Giant Planets
The Impact of Non-Uniform Thermal Structure on the Interpretation of Exoplanet Emission Spectra
A Characteristic Transmission Spectrum Dominated by H2o Applies to the Majority Ofhst/Wfc3 Exoplanet Observations
The WATER ABUNDANCE OF THE DIRECTLY IMAGED SUBSTELLAR COMPANIONκAND B RETRIEVED FROM a NEAR INFRARED SPECTRUM
A DETECTION OF WATER IN THE TRANSMISSION SPECTRUM OF THE HOT JUPITER WASP-12b AND IMPLICATIONS FOR ITS ATMOSPHERIC COMPOSITION
Spitzersecondary Eclipse Observations of Five Cool Gas Giant Planets and Empirical Trends in Cool Planet Emission Spectra
Uniform Atmospheric Retrieval Analysis of Ultracool Dwarfs. I. Characterizing Benchmarks, Gl 570D and HD 3651B
NEW ANALYSIS INDICATES NO THERMAL INVERSION IN THE ATMOSPHERE OF HD 209458b
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