The Planetary Systems Imager: 2-5 Micron Channel

Skemer, Andrew J. and Stelter, Deno and Mawet, Dimitri and Fitzgerald, Michael and Mazin, Benjamin and Guyon, Olivier and Marois, Christian and Briesemeister, Zackery and Brandt, Timothy and Chilcote, Jeffrey and Delorme, Jacques-Robert and Jovanovic, Nemanja and Lu, Jessica and Millar-Blanchaer, Maxwell and Wallace, James and Vasisht, Gautam and Roberts, Lewis C., Jr. and Wang, Ji (2018) The Planetary Systems Imager: 2-5 Micron Channel. In: Ground-based and Airborne Instrumentation for Astronomy VII. Proceedings of SPIE. No.10702. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 10702A5. ISBN 9781510619579. https://resolver.caltech.edu/CaltechAUTHORS:20181203-101750008

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Abstract

We summarize the red channel (2-5 micron) of the Planetary Systems Imager (PSI), a proposed second-generation instrument for the TMT. Cold exoplanets emit the majority of their light in the thermal infrared, which means these exoplanets can be detected at a more modest contrast than at other wavelengths. PSI-Red will be able to detect and characterize a wide variety of exoplanets, including radial-velocity planets on wide orbits, accreting protoplanets in nearby star-forming regions, and reflected-light planets around the nearest stars. PSI-Red will feature an imager, a low-resolution lenslet integral field spectrograph, a medium-resolution lenslet+slicer integral field spectrograph, and a fiber-fed high-resolution spectrograph.

Item Type:

Book Section

Related URLs:

URL	URL Type	Description
https://doi.org/10.1117/12.2314173	DOI	Article
https://arxiv.org/abs/1808.03304	arXiv	Discussion Paper

ORCID:

Author	ORCID
Skemer, Andrew J.	0000-0001-6098-3924
Mawet, Dimitri	0000-0002-8895-4735
Fitzgerald, Michael	0000-0002-0176-8973
Guyon, Olivier	0000-0002-1097-9908
Marois, Christian	0000-0002-4164-4182
Brandt, Timothy	0000-0003-2630-8073
Chilcote, Jeffrey	0000-0001-6305-7272
Lu, Jessica	0000-0001-9611-0009
Millar-Blanchaer, Maxwell	0000-0001-6205-9233
Vasisht, Gautam	0000-0002-1871-6264
Roberts, Lewis C., Jr.	0000-0003-3892-2900
Wang, Ji	0000-0002-4361-8885

Additional Information:

© 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors wish to acknowledge the Center for Adaptive Optics Fall Retreat and the TMT Science Forum, where much of this work originated. This paper is based on work funded by NSF Grants 1608834 and 1614320.

Group:

Thirty Meter Telescope, Astronomy Department

Funders:

Funding Agency	Grant Number
NSF	AST-1608834
NSF	AST-1614320

Subject Keywords:

Adaptive optics, integral field spectroscopy, exoplanet imaging, exoplanet instrumentation

Series Name:

Proceedings of SPIE

Issue or Number:

10702

DOI:

10.1117/12.2314173

Record Number:

CaltechAUTHORS:20181203-101750008

Persistent URL:

https://resolver.caltech.edu/CaltechAUTHORS:20181203-101750008

Official Citation:

Andrew J. Skemer, Deno Stelter, Dimitri Mawet, Michael Fitzgerald, Benjamin Mazin, Olivier Guyon, Christian Marois, Zackery Briesemeister, Timothy Brandt, Jeffrey Chilcote, Jacques-Robert Delorme, Nemanja Jovanovic, Jessica Lu, Maxwell Millar-Blanchaer, James Wallace, Gautam Vasisht, Lewis C. Roberts, and Ji Wang "The planetary systems imager: 2-5 micron channel", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 10702A5 (16 July 2018); https://doi.org/10.1117/12.2314173

Usage Policy:

No commercial reproduction, distribution, display or performance rights in this work are provided.

ID Code:

91396

Collection:

CaltechAUTHORS

Deposited By:

Tony Diaz

Deposited On:

03 Dec 2018 19:41

Last Modified:

16 Nov 2021 03:41

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