Water vapor distribution in the Martian atmosphere from solar ...
The internal calibration of the BP and RP spectra does not remove this effect and there- fore the spectra used to generate the SSO reflectance spectra in.
Atmospheric correctionfor high-resolution near-infrared spectroscopy The fifth chapter has the goal to confirm or refute planetary companion detection around two stars, ? Aql and HD 192263, with near-infrared spectroscopic data.
Journal Pre-proof - University College London To quantify these effects, we developed a 3D radiative-transfer model able to generate transmission spectra of atmospheres based on 3D atmospheric structures.
Overcoming the stellar activity impact on exoplanet detection and ... We describe a new software package capable of predicting the spectra of Solar system planets, exoplanets, brown dwarfs and cool stars.
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