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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:
URLURL TypeDescription
https://doi.org/10.1117/12.2314173DOIArticle
https://arxiv.org/abs/1808.03304arXivDiscussion Paper
ORCID:
AuthorORCID
Skemer, Andrew J.0000-0001-6098-3924
Mawet, Dimitri0000-0002-8895-4735
Fitzgerald, Michael0000-0002-0176-8973
Guyon, Olivier0000-0002-1097-9908
Marois, Christian0000-0002-4164-4182
Brandt, Timothy0000-0003-2630-8073
Chilcote, Jeffrey0000-0001-6305-7272
Lu, Jessica0000-0001-9611-0009
Millar-Blanchaer, Maxwell0000-0001-6205-9233
Vasisht, Gautam0000-0002-1871-6264
Roberts, Lewis C., Jr.0000-0003-3892-2900
Wang, Ji0000-0002-4361-8885
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 AgencyGrant Number
NSFAST-1608834
NSFAST-1614320
Subject Keywords:Adaptive optics, integral field spectroscopy, exoplanet imaging, exoplanet instrumentation
Series Name:Proceedings of SPIE
Issue or Number:10702
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:09 Oct 2019 21:17

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