Moderate resolution spectroscopy of HR 8799bcd - Exo3 conference (2020)

Jean-Baptiste Ruffio - CaltechDec 21, 2020
Planet Detection
Atmospheric characterization
Instrumentation & Observational techniques
exoplanet
direct imaging
spectroscopy
The four directly imaged planets orbiting the star HR 8799 are an ideal laboratory to probe atmospheric physics and formation models. We present more than a decade's worth of Keck/OSIRIS moderate spectral resolution (R=4,000) of HR 8799 b, c, and d. This includes: detection of molecules, planetary radial velocity, and ...
You need to be logged in to ask a question