High-resolution spectroscopy
Chapter in ExoFrontiers: Big Questions in Exoplanetary Science, IOP Publishing (2021) 8-1
Abstract:
High-resolution spectroscopy (HRS) allows resolving the spectrum of an exoplanetary atmosphere into individual lines and using the Doppler shift of the planet spectrum to disentangle it from other sources, such as telluric contamination and the host star spectrum. The method excels at identifying chemical species with numerous spectral lines and can be used for transmission, day/night-side emission, and reflected light spectroscopy. This chapter discusses the state of the art and important questions and goals for HRS, the opportunities it offers and the challenges it faces.Detecting life outside our solar system with a large high-contrast-imaging mission
EXPERIMENTAL ASTRONOMY (2021)
Origins space telescope: from first light to life
EXPERIMENTAL ASTRONOMY (2021)
High-contrast observations of brown dwarf companion HR 2562 B with the vector Apodizing Phase Plate coronagraph
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 506:3 (2021) 3224-3238
Vector-apodizing phase plate coronagraph: design, current performance, and future development [Invited].
Applied Optics Optica Publishing Group 60:19 (2021) d52-d72