An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System

Rebecca Jensen-Clem; Philip M. Hinz; M. A.M. van Kooten; Michael P. Fitzgerald; Steph Sallum; Benjamin A. Mazin; Mark Chun; Maxwell A. Millar-Blanchaer; Andy Skemer; Ji Wang; R. Deno Stelter; Olivier Guyon

doi:10.1117/12.2630526

An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System

Rebecca Jensen-Clem, Philip M. Hinz, M. A.M. van Kooten, Michael P. Fitzgerald, Steph Sallum, Benjamin A. Mazin, Mark Chun, Maxwell A. Millar-Blanchaer, Andy Skemer, Ji Wang, R. Deno Stelter, Olivier Guyon

Optical Sciences

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

2 Scopus citations

Abstract

The Planetary Systems Imager (PSI), a proposed instrument suite for the Thirty Meter Telescope (TMT), enables a broad range of extreme-AO, high-contrast observations. PSI is specifically optimized for high contrast exoplanet science from 0.5 to 13 µm and to that end includes a core near-IR AO system that feeds multiple AO+science instrument subsystems. In this paper, we present a preliminary optical design for the full PSI-AO system, feeding the PSI-Red (2-5 µm), PSI-Blue (0.5-1.8 µm), and PSI-10 (8-13 µm) subsystems. We discuss an initial concept of testing and operations for the system that feeds into the conceptual design. We build on our preliminary end-to-end PSI-Red AO simulation to estimate the raw planet-to-star contrast ratios associated with PSI-Red and extrapolate these results to represent the effects of a PSI-Blue deformable mirror.

Original language	English (US)
Title of host publication	Adaptive Optics Systems VIII
Editors	Laura Schreiber, Dirk Schmidt, Elise Vernet
Publisher	SPIE
ISBN (Electronic)	9781510653511
DOIs	https://doi.org/10.1117/12.2630526
State	Published - 2022
Event	Adaptive Optics Systems VIII 2022 - Montreal, Canada Duration: Jul 17 2022 → Jul 22 2022

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	12185
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Adaptive Optics Systems VIII 2022
Country/Territory	Canada
City	Montreal
Period	7/17/22 → 7/22/22

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

10.1117/12.2630526

Cite this

Jensen-Clem, R., Hinz, P. M., van Kooten, M. A. M., Fitzgerald, M. P., Sallum, S., Mazin, B. A., Chun, M., Millar-Blanchaer, M. A., Skemer, A., Wang, J., Deno Stelter, R., & Guyon, O. (2022). An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System. In L. Schreiber, D. Schmidt, & E. Vernet (Eds.), Adaptive Optics Systems VIII Article 1218546 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12185). SPIE. https://doi.org/10.1117/12.2630526

An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System. / Jensen-Clem, Rebecca; Hinz, Philip M.; van Kooten, M. A.M. et al.
Adaptive Optics Systems VIII. ed. / Laura Schreiber; Dirk Schmidt; Elise Vernet. SPIE, 2022. 1218546 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12185).

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

Jensen-Clem, R, Hinz, PM, van Kooten, MAM, Fitzgerald, MP, Sallum, S, Mazin, BA, Chun, M, Millar-Blanchaer, MA, Skemer, A, Wang, J, Deno Stelter, R & Guyon, O 2022, An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System. in L Schreiber, D Schmidt & E Vernet (eds), Adaptive Optics Systems VIII., 1218546, Proceedings of SPIE - The International Society for Optical Engineering, vol. 12185, SPIE, Adaptive Optics Systems VIII 2022, Montreal, Canada, 7/17/22. https://doi.org/10.1117/12.2630526

Jensen-Clem R, Hinz PM, van Kooten MAM, Fitzgerald MP, Sallum S, Mazin BA et al. An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System. In Schreiber L, Schmidt D, Vernet E, editors, Adaptive Optics Systems VIII. SPIE. 2022. 1218546. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2630526

@inproceedings{f73de776ef66430783174345f4f98231,

title = "An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System",

abstract = "The Planetary Systems Imager (PSI), a proposed instrument suite for the Thirty Meter Telescope (TMT), enables a broad range of extreme-AO, high-contrast observations. PSI is specifically optimized for high contrast exoplanet science from 0.5 to 13 µm and to that end includes a core near-IR AO system that feeds multiple AO+science instrument subsystems. In this paper, we present a preliminary optical design for the full PSI-AO system, feeding the PSI-Red (2-5 µm), PSI-Blue (0.5-1.8 µm), and PSI-10 (8-13 µm) subsystems. We discuss an initial concept of testing and operations for the system that feeds into the conceptual design. We build on our preliminary end-to-end PSI-Red AO simulation to estimate the raw planet-to-star contrast ratios associated with PSI-Red and extrapolate these results to represent the effects of a PSI-Blue deformable mirror.",

keywords = "Adaptive Optics, Coronagraphy, Exoplanets",

author = "Rebecca Jensen-Clem and Hinz, {Philip M.} and {van Kooten}, {M. A.M.} and Fitzgerald, {Michael P.} and Steph Sallum and Mazin, {Benjamin A.} and Mark Chun and Millar-Blanchaer, {Maxwell A.} and Andy Skemer and Ji Wang and {Deno Stelter}, R. and Olivier Guyon",

note = "Publisher Copyright: {\textcopyright} 2022 SPIE.; Adaptive Optics Systems VIII 2022 ; Conference date: 17-07-2022 Through 22-07-2022",

year = "2022",

doi = "10.1117/12.2630526",

language = "English (US)",

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

publisher = "SPIE",

editor = "Laura Schreiber and Dirk Schmidt and Elise Vernet",

booktitle = "Adaptive Optics Systems VIII",

}

TY - GEN

T1 - An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System

AU - Jensen-Clem, Rebecca

AU - Hinz, Philip M.

AU - van Kooten, M. A.M.

AU - Fitzgerald, Michael P.

AU - Sallum, Steph

AU - Mazin, Benjamin A.

AU - Chun, Mark

AU - Millar-Blanchaer, Maxwell A.

AU - Skemer, Andy

AU - Wang, Ji

AU - Deno Stelter, R.

AU - Guyon, Olivier

PY - 2022

Y1 - 2022

N2 - The Planetary Systems Imager (PSI), a proposed instrument suite for the Thirty Meter Telescope (TMT), enables a broad range of extreme-AO, high-contrast observations. PSI is specifically optimized for high contrast exoplanet science from 0.5 to 13 µm and to that end includes a core near-IR AO system that feeds multiple AO+science instrument subsystems. In this paper, we present a preliminary optical design for the full PSI-AO system, feeding the PSI-Red (2-5 µm), PSI-Blue (0.5-1.8 µm), and PSI-10 (8-13 µm) subsystems. We discuss an initial concept of testing and operations for the system that feeds into the conceptual design. We build on our preliminary end-to-end PSI-Red AO simulation to estimate the raw planet-to-star contrast ratios associated with PSI-Red and extrapolate these results to represent the effects of a PSI-Blue deformable mirror.

AB - The Planetary Systems Imager (PSI), a proposed instrument suite for the Thirty Meter Telescope (TMT), enables a broad range of extreme-AO, high-contrast observations. PSI is specifically optimized for high contrast exoplanet science from 0.5 to 13 µm and to that end includes a core near-IR AO system that feeds multiple AO+science instrument subsystems. In this paper, we present a preliminary optical design for the full PSI-AO system, feeding the PSI-Red (2-5 µm), PSI-Blue (0.5-1.8 µm), and PSI-10 (8-13 µm) subsystems. We discuss an initial concept of testing and operations for the system that feeds into the conceptual design. We build on our preliminary end-to-end PSI-Red AO simulation to estimate the raw planet-to-star contrast ratios associated with PSI-Red and extrapolate these results to represent the effects of a PSI-Blue deformable mirror.

KW - Adaptive Optics

KW - Coronagraphy

KW - Exoplanets

UR - http://www.scopus.com/inward/record.url?scp=85178514576&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85178514576&partnerID=8YFLogxK

U2 - 10.1117/12.2630526

DO - 10.1117/12.2630526

M3 - Conference contribution

AN - SCOPUS:85178514576

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

BT - Adaptive Optics Systems VIII

A2 - Schreiber, Laura

A2 - Schmidt, Dirk

A2 - Vernet, Elise

PB - SPIE

T2 - Adaptive Optics Systems VIII 2022

Y2 - 17 July 2022 through 22 July 2022

ER -

An Updated Preliminary Optical Design and Performance analysis of the Planetary Systems Imager Adaptive Optics System

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this