Paper
16 July 2018 The planetary systems imager: 2-5 micron channel
Author Affiliations +
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.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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
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Cited by 4 scholarly publications.
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KEYWORDS
Exoplanets

Planets

Imaging systems

Adaptive optics

Imaging spectroscopy

Planetary systems

Spectrographs

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