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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. . (Submitted) http://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:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
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
Lu, Jessica0000-0001-9611-0009
Vasisht, Gautam0000-0002-1871-6264
Roberts, Lewis C., Jr.0000-0003-3892-2900
Additional Information: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.
Funders:
Funding AgencyGrant Number
NSFAST-1608834
NSFAST-1614320
Subject Keywords:Adaptive optics, integral field spectroscopy, exoplanet imaging, exoplanet instrumentation
Record Number:CaltechAUTHORS:20181203-101750008
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20181203-101750008
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:03 Dec 2018 19:41

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