Keck Planet Imager and Characterizer: concept and phased implementation
Wallace, J. K.
AffiliationUniv Arizona, Lunar & Planetary Lab
high contrast imaging
high contrast high resolution spectroscopy
small inner working angle coronagraphy
on-axis segmented telescopes
Extremely Large Telescopes
MetadataShow full item record
PublisherSPIE-INT SOC OPTICAL ENGINEERING
CitationD. Mawet ; P. Wizinowich ; R. Dekany ; M. Chun ; D. Hall ; S. Cetre ; O. Guyon ; J. K. Wallace ; B. Bowler ; M. Liu ; G. Ruane ; E. Serabyn ; R. Bartos ; J. Wang ; G. Vasisht ; M. Fitzgerald ; A. Skemer ; M. Ireland ; J. Fucik ; J. Fortney ; I. Crossfield ; R. Hu and B. Benneke " Keck Planet Imager and Characterizer: concept and phased implementation ", Proc. SPIE 9909, Adaptive Optics Systems V, 99090D (July 26, 2016); doi:10.1117/12.2233658; http://dx.doi.org/10.1117/12.2233658
JournalADAPTIVE OPTICS SYSTEMS V
Rights© 2016 SPIE.
Collection InformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at email@example.com.
AbstractThe Keck Planet Imager and Characterizer (KPIC) is a cost-effective upgrade path to the W.M. Keck observatory (WMKO) adaptive optics (AO) system, building on the lessons learned from first and second-generation extreme AO (ExA0) coronagraphs. KPIC will explore new scientific niches in exoplanet science, while maturing critical technologies and systems for future ground-based (TMT, FELT, GMT) and space-based planet imagers (HabEx, LUVOIR). The advent of fast low-noise IR cameras (IR-APD, MKIDS, electron injectors), the rapid maturing of efficient wavefront sensing (WFS) techniques (Pyramid, Zernike), small inner working angle (IWA) coronagraphs (e.g., vortex) and associated low-order wavefront sensors (LOWFS), as well as recent breakthroughs in high contrast high resolution spectroscopy, open new direct exoplanet exploration avenues that are complementary to planet imagers such as VLT-SPHERE and the Gemini Planet Imager (GPI). For instance, the search and detailed characterization of planetary systems on solar-system scales around late-type stars, mostly beyond SPHERE and GPI's reaches, can be initiated now at WMKO.
VersionFinal published version