Status of the Keck Planet Imager and Characterizer Phase II Development
Jacklyn Pezzato, Nemanja Jovanovic, Dimitri Mawet, Garreth Ruane,, Jason Wang, James K. Wallace, Jennah K. Colborn, Sylvain Cetre, Charlotte Z., Bond, Randall Bartos, Benjamin Calvin, Jacques-Robert Delorme, Daniel, Echeverri, Rebecca Jensen-Clem, Eden McEwen, Scott Lilley

TL;DR
The paper discusses the development and testing of Phase II upgrades for the Keck Planet Imager and Characterizer, aimed at enhancing direct imaging and spectroscopy of exoplanets with new advanced modules.
Contribution
It introduces the design and laboratory testing results of the Phase II system enhancements for KPIC, including new submodules for improved performance.
Findings
Successful laboratory testing of new submodules
Enhanced system throughput and contrast expected
Preparation for deployment at Keck in early 2020
Abstract
The Keck Planet Imager and Characterizer comprises of a series of upgrades to the Keck II adaptive optics system and instrument suite to improve the direct imaging and high resolution spectroscopy capabilities of the facility instruments NIRC2 and NIRSPEC, respectively. Phase I of KPIC includes a NIR pyramid wavefront sensor and a Fiber Injection Unit (FIU) to feed NIRSPEC with a single mode fiber, which have already been installed and are currently undergoing commissioning. KPIC will enable High Dispersion Coronagraphy (HDC) of directly imaged exoplanets for the first time, providing potentially improved detection significance and spectral characterization capabilities compared to direct imaging. In favorable cases, Doppler imaging, spin measurements, and molecule mapping are also possible. This science goal drives the development of phase II of KPIC, which is scheduled to be deployed…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Adaptive optics and wavefront sensing
