TY - JOUR
T1 - The planetary systems imager
T2 - 2-5 micron channel
AU - Skemer, Andrew J.
AU - Stelter, Deno
AU - Mawet, Dimitri
AU - Fitzgerald, Michael
AU - Mazin, Benjamin
AU - Guyon, Olivier
AU - Marois, Christian
AU - Briesemeister, Zackery
AU - Brandt, Timothy
AU - Chilcote, Jeffrey
AU - Delorme, Jacques Robert
AU - Jovanovic, Nemanja
AU - Lu, Jessica
AU - Millar-Blanchaer, Maxwell
AU - Wallace, James
AU - Vasisht, Gautam
AU - Roberts, Lewis C.
AU - Wang, Ji
N1 - Publisher Copyright:
Copyright © 2018, The Authors. All rights reserved.
Copyright:
Copyright 2020 Elsevier B.V., All rights reserved.
PY - 2018/8/9
Y1 - 2018/8/9
N2 - 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.
AB - 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.
KW - Adaptive optics
KW - Exoplanet imaging
KW - Exoplanet instrumentation
KW - Integral field spectroscopy
UR - http://www.scopus.com/inward/record.url?scp=85094507437&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85094507437&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:85094507437
JO - Nuclear Physics A
JF - Nuclear Physics A
SN - 0375-9474
ER -