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Showing 1 to 3 of 3 for “"wasp 43b"”.
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Observations, Thermochemical Calculations, and Modeling of Exoplanetary Atmospheres
… analysis and atmospheric characterization of WASP-14b. The decrease in flux when a planet passes behind its host star reveals the planet dayside thermal emission, which, in turn, tells us about the atmospheric temperature and pressure profiles and molecular abundances. WASP-14b is a highly …
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Probing the atmospheres of transiting exoplanets using ground-based multi-object spectroscopy
… flexibility.<br/><br/>My FORS2 observations of WASP-103b reveal a featureless optical spectrum and result in a detection of H2O when combined with GMOS, WFC3 and Spitzer data. The most likely explanation for this featureless spectrum may simply be a combination of low signal-to-noise and the …
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New Avenues in Atmospheric Modelling of Exoplanets
… work I have shown that the thermal inversion on WASP-121b can be explained by all the visible absorbers listed above. These thermal inversions are of great importance as the species responsible may be observed with current observational capabilities, thus providing testable observations for these …