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: Chapter in Book/Report/Conference proceedingConference contribution

3 Scopus citations

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)
Title of host publicationGround-based and Airborne Instrumentation for Astronomy VII
EditorsLuc Simard, Luc Simard, Christopher J. Evans, Hideki Takami
PublisherSPIE
ISBN (Print)9781510619579
DOIs
StatePublished - Jan 1 2018
Externally publishedYes
EventGround-based and Airborne Instrumentation for Astronomy VII 2018 - Austin, United States
Duration: Jun 10 2018Jun 14 2018

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume10702
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Other

OtherGround-based and Airborne Instrumentation for Astronomy VII 2018
CountryUnited States
CityAustin
Period6/10/186/14/18

Keywords

  • Adaptive optics
  • exoplanet imaging
  • exoplanet instrumentation
  • integral field spectroscopy

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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  • Cite this

    Skemer, A. J., Stelter, D., Mawet, D., Fitzgerald, M., Mazin, B., Guyon, O., Marois, C., Briesemeister, Z., Brandt, T., Chilcote, J., Delorme, J. R., Jovanovic, N., Lu, J., Millar-Blanchaer, M., Wallace, J., Vasisht, G., Roberts, L. C., & Wang, J. (2018). The planetary systems imager: 2-5 micron channel. In L. Simard, L. Simard, C. J. Evans, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy VII [10702A5] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10702). SPIE. https://doi.org/10.1117/12.2314173