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Keck Planet Imager and Characterizer: concept and phased implementation

Mawet, D. and Wizinowich, P. and Dekany, R. and Chun, M. and Hall, D. and Cetre, S. and Guyon, O. and Wallace, J. K. and Bowler, B. and Liu, M. and Ruane, G. and Serabyn, E. and Bartos, R. and Wang, J. and Vasisht, G. and Fitzgerald, M. and Skemer, A. and Ireland, M. and Fucik, J. and Fortney, J. and Crossfield, I. and Hu, R. and Benneke, B. (2016) Keck Planet Imager and Characterizer: concept and phased implementation. In: Adaptive Optics Systems V. Proceedings of SPIE. No.9909. Society of Photo-Optical Instrumentation Engineers , Bellingham, WA, Art. No. 99090D. ISBN 9781510601970. http://resolver.caltech.edu/CaltechAUTHORS:20180605-131826047

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Abstract

The 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 (ExAO) coronagraphs. KPIC will explore new scientific niches in exoplanet science, while maturing critical technologies and systems for future ground-based (TMT, EELT, 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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.2233658DOIArticle
ORCID:
AuthorORCID
Mawet, D.0000-0002-8895-4735
Guyon, O.0000-0002-1097-9908
Liu, M.0000-0003-2232-7664
Ruane, G.0000-0003-4769-1665
Fitzgerald, M.0000-0002-0176-8973
Skemer, A.0000-0001-6098-3924
Fortney, J.0000-0002-9843-4354
Additional Information:© 2016 SPIE. This work was partially carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:Exoplanets, high contrast imaging, high contrast high resolution spectroscopy, small inner working angle coronagraphy, vortex coronagraph, on-axis segmented telescopes, apodization, Extremely Large Telescopes
Record Number:CaltechAUTHORS:20180605-131826047
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180605-131826047
Official Citation:D. 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, B. Benneke, "Keck Planet Imager and Characterizer: concept and phased implementation," Proc. SPIE 9909, Adaptive Optics Systems V, 99090D (26 July 2016)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:86796
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:05 Jun 2018 21:41
Last Modified:05 Jun 2018 21:41

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