Constraining Exoplanet Mass from Transmission Spectroscopy
Determination of an exoplanet's mass is a key to understanding its basic properties, including its potential for supporting life. To date, mass constraints for exoplanets are predominantly based on radial velocity (RV) measurements, which are not suited for planets with low masses, large semima...
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American Association for the Advancement of Science (AAAS)
2018
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| Online Access: | http://hdl.handle.net/1721.1/118910 https://orcid.org/0000-0003-2415-2191 https://orcid.org/0000-0002-6892-6948 |