The planetary systems imager: 2-5 micron channel

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, Ji Wang

Research output: Contribution to journalArticlepeer-review

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.

Original languageEnglish (US)
JournalUnknown Journal
StatePublished - Aug 9 2018
Externally publishedYes

Keywords

  • Adaptive optics
  • Exoplanet imaging
  • Exoplanet instrumentation
  • Integral field spectroscopy

ASJC Scopus subject areas

  • General

Fingerprint Dive into the research topics of 'The planetary systems imager: 2-5 micron channel'. Together they form a unique fingerprint.

Cite this