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Keck Planet Imager and Characterizer: demonstrating advanced exoplanet characterization techniques for future extremely large telescopes (Conference Presentation)

Jovanovic, Nemanja and Delorme, Jacques-Robert and Bond, Charlotte Z. and Cetre, Sylvain and Mawet, Dimitri and Echeverri, Daniel and Wallace, James K. and Bartos, Randall and Lilley, Scott and Ragland, Sam and Ruane, Garreth and Wizinowich, Peter and Chun, Mark and Wang, Ji and Wang, Jason and Fitzgerald, Michael and Pezzato, Jacklyn and Matthews, Keith and Calvin, Ben and Millar-Blanchaer, Maxwell and Martin, Emily C. and Wetherell, Edward and Wang, Eric and Jacobson, Shane and Warmbier, Eric and Lockhart, Charles and Hall, Don and Jensen-Clem, Rebecca and McEwen, Eden (2019) Keck Planet Imager and Characterizer: demonstrating advanced exoplanet characterization techniques for future extremely large telescopes (Conference Presentation). In: Techniques and Instrumentation for Detection of Exoplanets IX. Proceedings of SPIE. No.11117. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 111170T. ISBN 9781510629271. https://resolver.caltech.edu/CaltechAUTHORS:20190912-110942196

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Abstract

The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system enabling high contrast imaging and high-resolution spectroscopic characterization of giant exoplanets in the mid-infrared (2-5 microns). The KPIC instrument will be developed in phases. Phase I entails the installation of an infrared pyramid wavefront sensor (PyWFS) based on a fast, low-noise SAPHIRA IR-APD array. The ultra-sensitive infrared PyWFS will enable high contrast studies of infant exoplanets around cool, red, and/or obscured targets in star forming regions. In addition, the light downstream of the PyWFS will be coupled into an array of single-mode fibers with the aid of an active fiber injection unit (FIU). In turn, these fibers route light to Keck's high-resolution infrared spectrograph NIRSPEC, so that high dispersion coronagraphy (HDC) can be implemented for the first time. HDC optimally pairs high contrast imaging and high-resolution spectroscopy allowing detailed characterization of exoplanet atmospheres, including molecular composition, spin measurements, and Doppler imaging. We will provide an overview of the instrument, its science scope, and report on recent results from on-sky commissioning of Phase I. We will discuss plans for optimizing the instrument to seed designs for similar modes on extremely large telescopes.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.2529330DOIVideo
https://arxiv.org/abs/1909.04541arXivDiscussion Paper
ORCID:
AuthorORCID
Mawet, Dimitri0000-0002-8895-4735
Echeverri, Daniel0000-0002-1583-2040
Ruane, Garreth0000-0003-4769-1665
Wizinowich, Peter0000-0002-1646-442X
Wang, Ji0000-0002-4361-8885
Wang, Jason0000-0003-0774-6502
Fitzgerald, Michael0000-0002-0176-8973
Millar-Blanchaer, Maxwell0000-0001-6205-9233
Martin, Emily C.0000-0002-0618-5128
Jensen-Clem, Rebecca0000-0003-0054-2953
Additional Information:© 2019 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors would like to acknowledge the financial support of the Heising-Simons foundation. We thank Dr. Rebecca Jensen-Clem for loaning AOSE for use within the KPIC phase II testbed. We would like to thank the SCExAO project for lending KPIC roof prisms for the NIR PyWFS. Part of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration (NASA). The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.
Funders:
Funding AgencyGrant Number
Heising-Simons FoundationUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:Wavefront sensing, high contrast imaging, exoplanets, high dispersion coronography, high resolution spectroscopy
Series Name:Proceedings of SPIE
Issue or Number:11117
Record Number:CaltechAUTHORS:20190912-110942196
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190912-110942196
Official Citation:Nemanja Jovanovic, Jacques-Robert Delorme, Charlotte Z. Bond, Sylvain Cetre, Dimitri Mawet, Daniel Echeverri, James K. Wallace, Randy Bartos, Scott Lilley, Sam Ragland, Garreth Ruane, Peter Wizinowich, Mark Chun, Ji Wang, Jason Wang, Michael Fitzgerald, Jacklyn Pezzato, Keith Matthews, Ben Calvin, Maxwell Millar-Blanchaer, Emily C. Martin, Edward Wetherell, Eric Wang, Shane Jacobson, Eric Warmbier, Charles Lockhart, Don Hall, Rebecca Jensen-Clem, and Eden McEwen "The Keck Planet Imager and Characterizer: demonstrating advanced exoplanet characterization techniques for future extremely large telescopes (Conference Presentation)", Proc. SPIE 11117, Techniques and Instrumentation for Detection of Exoplanets IX, 111170T (9 September 2019); https://doi.org/10.1117/12.2529330
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98610
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:12 Sep 2019 18:27
Last Modified:19 Nov 2019 17:14

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