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Molecular opacities for exoplanets
Spectroscopic observations of exoplanets are now possible by transit methods and direct emission. Spectroscopic requirements for exoplanets are reviewed based on existing measurements and model predictions for hot Jupiters and super-Earths. Molecular opacities needed to simulate astronomical observa...
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| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
The Royal Society Publishing
2014
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| Témata: | |
| On-line přístup: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3982428/ https://ncbi.nlm.nih.gov/pubmed/24664921 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2013.0087 |
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