Keck Planet Imager and Characterizer: Concept and phased implementation

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

doi:10.1117/12.2233658

Keck Planet Imager and Characterizer: Concept and phased implementation

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. FortneyI. Crossfield, R. Hu, B. Benneke

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › peer-review

69 Citations (Scopus)

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.

Original language	English
Title of host publication	Adaptive Optics Systems V
Editors	Enrico Marchetti, Jean-Pierre Veran, Laird M. Close
Publisher	SPIE
ISBN (Electronic)	9781510601970
DOIs	https://doi.org/10.1117/12.2233658
Publication status	Published - 2016
Event	Adaptive Optics Systems V - Edinburgh, United Kingdom Duration: 26 Jun 2016 → 1 Jul 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9909
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Adaptive Optics Systems V
Country/Territory	United Kingdom
City	Edinburgh
Period	26/06/16 → 1/07/16

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10.1117/12.2233658

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Mawet, D., Wizinowich, P., Dekany, R., Chun, M., Hall, D., Cetre, S., Guyon, O., Wallace, J. K., Bowler, B., Liu, M., Ruane, G., Serabyn, E., Bartos, R., Wang, J., Vasisht, G., Fitzgerald, M., Skemer, A., Ireland, M., Fucik, J., ... Benneke, B. (2016). Keck Planet Imager and Characterizer: Concept and phased implementation. In E. Marchetti, J.-P. Veran, & L. M. Close (Eds.), Adaptive Optics Systems V Article 99090F (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9909). SPIE. https://doi.org/10.1117/12.2233658

@inproceedings{bc50b7e95447472fbf3f32701a91f803,

title = "Keck Planet Imager and Characterizer: Concept and phased implementation",

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.",

keywords = "Apodization, Exoplanets, Extremely Large Telescopes, High contrast high resolution spectroscopy, High contrast imaging, On-Axis segmented telescopes, Small inner working angle coronagraphy, Vortex coronagraph",

author = "D. Mawet and P. Wizinowich and R. Dekany and M. Chun and D. Hall and S. Cetre and O. Guyon and Wallace, \{J. K.\} and B. Bowler and M. Liu and G. Ruane and E. Serabyn and R. Bartos and J. Wang and G. Vasisht and M. Fitzgerald and A. Skemer and M. Ireland and J. Fucik and J. Fortney and I. Crossfield and R. Hu and B. Benneke",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Adaptive Optics Systems V ; Conference date: 26-06-2016 Through 01-07-2016",

year = "2016",

doi = "10.1117/12.2233658",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Enrico Marchetti and Jean-Pierre Veran and Close, \{Laird M.\}",

booktitle = "Adaptive Optics Systems V",

address = "United States",

}

Mawet, D, Wizinowich, P, Dekany, R, Chun, M, Hall, D, Cetre, S, Guyon, O, Wallace, JK, Bowler, B, Liu, M, Ruane, G, Serabyn, E, Bartos, R, Wang, J, Vasisht, G, Fitzgerald, M, Skemer, A, Ireland, M, Fucik, J, Fortney, J, Crossfield, I, Hu, R & Benneke, B 2016, Keck Planet Imager and Characterizer: Concept and phased implementation. in E Marchetti, J-P Veran & LM Close (eds), Adaptive Optics Systems V., 99090F, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9909, SPIE, Adaptive Optics Systems V, Edinburgh, United Kingdom, 26/06/16. https://doi.org/10.1117/12.2233658

Keck Planet Imager and Characterizer: Concept and phased implementation. / Mawet, D.; Wizinowich, P.; Dekany, R. et al.
Adaptive Optics Systems V. ed. / Enrico Marchetti; Jean-Pierre Veran; Laird M. Close. SPIE, 2016. 99090F (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9909).

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › peer-review

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T2 - Adaptive Optics Systems V

AU - Mawet, D.

AU - Wizinowich, P.

AU - Dekany, R.

AU - Chun, M.

AU - Hall, D.

AU - Cetre, S.

AU - Guyon, O.

AU - Wallace, J. K.

AU - Bowler, B.

AU - Liu, M.

AU - Ruane, G.

AU - Serabyn, E.

AU - Bartos, R.

AU - Wang, J.

AU - Vasisht, G.

AU - Fitzgerald, M.

AU - Skemer, A.

AU - Ireland, M.

AU - Fucik, J.

AU - Fortney, J.

AU - Crossfield, I.

AU - Hu, R.

AU - Benneke, B.

PY - 2016

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N2 - 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.

AB - 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.

KW - Apodization

KW - Exoplanets

KW - Extremely Large Telescopes

KW - High contrast high resolution spectroscopy

KW - High contrast imaging

KW - On-Axis segmented telescopes

KW - Small inner working angle coronagraphy

KW - Vortex coronagraph

UR - https://www.scopus.com/pages/publications/85002131213

U2 - 10.1117/12.2233658

DO - 10.1117/12.2233658

M3 - Conference Paper

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Adaptive Optics Systems V

A2 - Marchetti, Enrico

A2 - Veran, Jean-Pierre

A2 - Close, Laird M.

PB - SPIE

Y2 - 26 June 2016 through 1 July 2016

ER -

Keck Planet Imager and Characterizer: Concept and phased implementation

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