The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system

Rebecca Jensen-Clem; Philip Hinz; Maaike Von Kooten; Michael P. Fitzgerald; Steph Sallum; Benjamin Mazin; Mark Chun; Claire Max; Maxwell Millar-Blanchaer; Olivier Guyon; Andrew Skemer; R. Deno Stelter; Ji Wang

doi:10.1117/12.2594005

The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system

Rebecca Jensen-Clem, Philip Hinz, Maaike Von Kooten, Michael P. Fitzgerald, Steph Sallum, Benjamin Mazin, Mark Chun, Claire Max, Maxwell Millar-Blanchaer, Olivier Guyon, Andrew Skemer, R. Deno Stelter, Ji Wang

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Scopus citations

Abstract

The Planetary Systems Imager (PSI) is a proposed instrument for the Thirty Meter Telescope (TMT) that provides an extreme adaptive optics (AO) correction to a multi-wavelength instrument suite optimized for high contrast science. PSI's broad range of capabilities, spanning imaging, polarimetry, integral field spectroscopy, and high resolution spectroscopy from 0.6-5 μm, with a potential channel at 10 μm, will enable breakthrough science in the areas of exoplanet formation and evolution. Here, we present a preliminary optical design and performance analysis of the 2-5 μm component of the PSI AO system, which must deliver the wavefront quality necessary to support infrared high contrast science cases.

Original language	English (US)
Title of host publication	Techniques and Instrumentation for Detection of Exoplanets X
Editors	Stuart B. Shaklan, Garreth J. Ruane
Publisher	SPIE
ISBN (Electronic)	9781510644847
DOIs	https://doi.org/10.1117/12.2594005
State	Published - 2021
Event	Techniques and Instrumentation for Detection of Exoplanets X 2021 - San Diego, United States Duration: Aug 1 2021 → Aug 5 2021

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11823

Conference

Conference	Techniques and Instrumentation for Detection of Exoplanets X 2021
Country/Territory	United States
City	San Diego
Period	8/1/21 → 8/5/21

Keywords

Adaptive Optics
Coronagraphy
Exoplanets

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2594005

Cite this

Jensen-Clem, R., Hinz, P., Von Kooten, M., Fitzgerald, M. P., Sallum, S., Mazin, B., Chun, M., Max, C., Millar-Blanchaer, M., Guyon, O., Skemer, A., Stelter, R. D., & Wang, J. (2021). The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system. In S. B. Shaklan, & G. J. Ruane (Eds.), Techniques and Instrumentation for Detection of Exoplanets X Article 1182309 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11823). SPIE. https://doi.org/10.1117/12.2594005

The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system. / Jensen-Clem, Rebecca; Hinz, Philip; Von Kooten, Maaike et al.
Techniques and Instrumentation for Detection of Exoplanets X. ed. / Stuart B. Shaklan; Garreth J. Ruane. SPIE, 2021. 1182309 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11823).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Jensen-Clem, R, Hinz, P, Von Kooten, M, Fitzgerald, MP, Sallum, S, Mazin, B, Chun, M, Max, C, Millar-Blanchaer, M, Guyon, O, Skemer, A, Stelter, RD & Wang, J 2021, The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system. in SB Shaklan & GJ Ruane (eds), Techniques and Instrumentation for Detection of Exoplanets X., 1182309, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11823, SPIE, Techniques and Instrumentation for Detection of Exoplanets X 2021, San Diego, United States, 8/1/21. https://doi.org/10.1117/12.2594005

Jensen-Clem R, Hinz P, Von Kooten M, Fitzgerald MP, Sallum S, Mazin B et al. The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system. In Shaklan SB, Ruane GJ, editors, Techniques and Instrumentation for Detection of Exoplanets X. SPIE. 2021. 1182309. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2594005

Jensen-Clem, Rebecca ; Hinz, Philip ; Von Kooten, Maaike et al. / The Planetary Systems Imager adaptive optics system : An initial optical design and performance analysis tool for the PSI-Red AO system. Techniques and Instrumentation for Detection of Exoplanets X. editor / Stuart B. Shaklan ; Garreth J. Ruane. SPIE, 2021. (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{17dd2ce7caec4e6ca5cdb8cd7a9c535f,

title = "The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system",

abstract = "The Planetary Systems Imager (PSI) is a proposed instrument for the Thirty Meter Telescope (TMT) that provides an extreme adaptive optics (AO) correction to a multi-wavelength instrument suite optimized for high contrast science. PSI's broad range of capabilities, spanning imaging, polarimetry, integral field spectroscopy, and high resolution spectroscopy from 0.6-5 μm, with a potential channel at 10 μm, will enable breakthrough science in the areas of exoplanet formation and evolution. Here, we present a preliminary optical design and performance analysis of the 2-5 μm component of the PSI AO system, which must deliver the wavefront quality necessary to support infrared high contrast science cases.",

keywords = "Adaptive Optics, Coronagraphy, Exoplanets",

author = "Rebecca Jensen-Clem and Philip Hinz and {Von Kooten}, Maaike and Fitzgerald, {Michael P.} and Steph Sallum and Benjamin Mazin and Mark Chun and Claire Max and Maxwell Millar-Blanchaer and Olivier Guyon and Andrew Skemer and Stelter, {R. Deno} and Ji Wang",

note = "Funding Information: This work was partially supported by the National Science Foundation AST-ATI Grant 2008822, the Heising-Simons Foundation, and the University of California Observatories minigrant program. RJ-C also thanks UC Santa Cruz Profs. Brant Robertson and Daniel Fremont for computational resources used as part of this study. The authors thank all participants in the PSI collaboration and all staff members at the TMT and WMKO for their support of this effort. Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Techniques and Instrumentation for Detection of Exoplanets X 2021 ; Conference date: 01-08-2021 Through 05-08-2021",

year = "2021",

doi = "10.1117/12.2594005",

language = "English (US)",

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

publisher = "SPIE",

editor = "Shaklan, {Stuart B.} and Ruane, {Garreth J.}",

booktitle = "Techniques and Instrumentation for Detection of Exoplanets X",

}

TY - GEN

T1 - The Planetary Systems Imager adaptive optics system

T2 - Techniques and Instrumentation for Detection of Exoplanets X 2021

AU - Jensen-Clem, Rebecca

AU - Hinz, Philip

AU - Von Kooten, Maaike

AU - Fitzgerald, Michael P.

AU - Sallum, Steph

AU - Mazin, Benjamin

AU - Chun, Mark

AU - Max, Claire

AU - Millar-Blanchaer, Maxwell

AU - Guyon, Olivier

AU - Skemer, Andrew

AU - Stelter, R. Deno

AU - Wang, Ji

N1 - Funding Information: This work was partially supported by the National Science Foundation AST-ATI Grant 2008822, the Heising-Simons Foundation, and the University of California Observatories minigrant program. RJ-C also thanks UC Santa Cruz Profs. Brant Robertson and Daniel Fremont for computational resources used as part of this study. The authors thank all participants in the PSI collaboration and all staff members at the TMT and WMKO for their support of this effort. Publisher Copyright: © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.

PY - 2021

Y1 - 2021

N2 - The Planetary Systems Imager (PSI) is a proposed instrument for the Thirty Meter Telescope (TMT) that provides an extreme adaptive optics (AO) correction to a multi-wavelength instrument suite optimized for high contrast science. PSI's broad range of capabilities, spanning imaging, polarimetry, integral field spectroscopy, and high resolution spectroscopy from 0.6-5 μm, with a potential channel at 10 μm, will enable breakthrough science in the areas of exoplanet formation and evolution. Here, we present a preliminary optical design and performance analysis of the 2-5 μm component of the PSI AO system, which must deliver the wavefront quality necessary to support infrared high contrast science cases.

AB - The Planetary Systems Imager (PSI) is a proposed instrument for the Thirty Meter Telescope (TMT) that provides an extreme adaptive optics (AO) correction to a multi-wavelength instrument suite optimized for high contrast science. PSI's broad range of capabilities, spanning imaging, polarimetry, integral field spectroscopy, and high resolution spectroscopy from 0.6-5 μm, with a potential channel at 10 μm, will enable breakthrough science in the areas of exoplanet formation and evolution. Here, we present a preliminary optical design and performance analysis of the 2-5 μm component of the PSI AO system, which must deliver the wavefront quality necessary to support infrared high contrast science cases.

KW - Adaptive Optics

KW - Coronagraphy

KW - Exoplanets

UR - http://www.scopus.com/inward/record.url?scp=85114254622&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85114254622&partnerID=8YFLogxK

U2 - 10.1117/12.2594005

DO - 10.1117/12.2594005

M3 - Conference contribution

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

BT - Techniques and Instrumentation for Detection of Exoplanets X

A2 - Shaklan, Stuart B.

A2 - Ruane, Garreth J.

PB - SPIE

Y2 - 1 August 2021 through 5 August 2021

ER -

The Planetary Systems Imager adaptive optics system: An initial optical design and performance analysis tool for the PSI-Red AO system

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this