The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope

Mary Anne Peters-Limbach; Tyler D. Groff; N. Jeremy Kasdin; Dave Driscoll; Michael Galvin; Allen Foster; Michael A. Carr; Dave LeClerc; Rad Fagan; Michael W. McElwain; Gillian Knapp; Timothy Brandt; Markus Janson; Olivier Guyon; Nemanja Jovanovic; Frantz Martinache; Masahiko Hayashi; Naruhisa Takato

doi:10.1117/12.2024070

The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope

Mary Anne Peters-Limbach, Tyler D. Groff, N. Jeremy Kasdin, Dave Driscoll, Michael Galvin, Allen Foster, Michael A. Carr, Dave LeClerc, Rad Fagan, Michael W. McElwain, Gillian Knapp, Timothy Brandt, Markus Janson, Olivier Guyon, Nemanja Jovanovic, Frantz Martinache, Masahiko Hayashi, Naruhisa Takato

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

28 Scopus citations

Abstract

High-contrast imaging techniques now make possible both imaging and spectroscopy of planets around nearby stars. We present the optical design for the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS), a lenslet-based, cryogenic integral field spectrograph (IFS) for imaging exoplanets on the Subaru telescope. The IFS will provide spectral information for 138×138 spatial elements over a 2.07 arcsec × 2.07 arcsec field of view (FOV). CHARIS will operate in the near infrared (λ = 1.15 - 2.5μm) and will feature two spectral resolution modes of R ≈ 18 (low-res mode) and R ≈ 73 (high-res mode). Taking advantage of the Subaru telescope adaptive optics systems and coronagraphs (AO188 and SCExAO), CHARIS will provide sufficient contrast to obtain spectra of young self-luminous Jupiter-mass exoplanets. CHARIS will undergo CDR in October 2013 and is projected to have first light by the end of 2015. We report here on the current optical design of CHARIS and its unique innovations.

Original language	English (US)
Title of host publication	Techniques and Instrumentation for Detection of Exoplanets VI
DOIs	https://doi.org/10.1117/12.2024070
State	Published - 2013
Event	Techniques and Instrumentation for Detection of Exoplanets VI - San Diego, CA, United States Duration: Aug 26 2013 → Aug 29 2013

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	8864
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Techniques and Instrumentation for Detection of Exoplanets VI
Country/Territory	United States
City	San Diego, CA
Period	8/26/13 → 8/29/13

All Science Journal Classification (ASJC) codes

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

Keywords

Adaptive Optics
Coronagraphy
Exoplanets
High Contrast Imaging
Integral Field Spectrograph

Access to Document

10.1117/12.2024070

Cite this

Peters-Limbach, M. A., Groff, T. D., Kasdin, N. J., Driscoll, D., Galvin, M., Foster, A., Carr, M. A., LeClerc, D., Fagan, R., McElwain, M. W., Knapp, G., Brandt, T., Janson, M., Guyon, O., Jovanovic, N., Martinache, F., Hayashi, M., & Takato, N. (2013). The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope. In Techniques and Instrumentation for Detection of Exoplanets VI Article 88641N (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8864). https://doi.org/10.1117/12.2024070

@inproceedings{7eecd49b663446e7be0501849d4f67a7,

title = "The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope",

abstract = "High-contrast imaging techniques now make possible both imaging and spectroscopy of planets around nearby stars. We present the optical design for the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS), a lenslet-based, cryogenic integral field spectrograph (IFS) for imaging exoplanets on the Subaru telescope. The IFS will provide spectral information for 138×138 spatial elements over a 2.07 arcsec × 2.07 arcsec field of view (FOV). CHARIS will operate in the near infrared (λ = 1.15 - 2.5μm) and will feature two spectral resolution modes of R ≈ 18 (low-res mode) and R ≈ 73 (high-res mode). Taking advantage of the Subaru telescope adaptive optics systems and coronagraphs (AO188 and SCExAO), CHARIS will provide sufficient contrast to obtain spectra of young self-luminous Jupiter-mass exoplanets. CHARIS will undergo CDR in October 2013 and is projected to have first light by the end of 2015. We report here on the current optical design of CHARIS and its unique innovations.",

keywords = "Adaptive Optics, Coronagraphy, Exoplanets, High Contrast Imaging, Integral Field Spectrograph",

author = "Peters-Limbach, {Mary Anne} and Groff, {Tyler D.} and Kasdin, {N. Jeremy} and Dave Driscoll and Michael Galvin and Allen Foster and Carr, {Michael A.} and Dave LeClerc and Rad Fagan and McElwain, {Michael W.} and Gillian Knapp and Timothy Brandt and Markus Janson and Olivier Guyon and Nemanja Jovanovic and Frantz Martinache and Masahiko Hayashi and Naruhisa Takato",

year = "2013",

doi = "10.1117/12.2024070",

language = "English (US)",

isbn = "9780819497147",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

booktitle = "Techniques and Instrumentation for Detection of Exoplanets VI",

note = "Techniques and Instrumentation for Detection of Exoplanets VI ; Conference date: 26-08-2013 Through 29-08-2013",

}

Peters-Limbach, MA, Groff, TD, Kasdin, NJ, Driscoll, D, Galvin, M, Foster, A, Carr, MA, LeClerc, D, Fagan, R, McElwain, MW, Knapp, G, Brandt, T, Janson, M, Guyon, O, Jovanovic, N, Martinache, F, Hayashi, M & Takato, N 2013, The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope. in Techniques and Instrumentation for Detection of Exoplanets VI., 88641N, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8864, Techniques and Instrumentation for Detection of Exoplanets VI, San Diego, CA, United States, 8/26/13. https://doi.org/10.1117/12.2024070

The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope. / Peters-Limbach, Mary Anne; Groff, Tyler D.; Kasdin, N. Jeremy et al.
Techniques and Instrumentation for Detection of Exoplanets VI. 2013. 88641N (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8864).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - The optical design of CHARIS

T2 - Techniques and Instrumentation for Detection of Exoplanets VI

AU - Peters-Limbach, Mary Anne

AU - Groff, Tyler D.

AU - Kasdin, N. Jeremy

AU - Driscoll, Dave

AU - Galvin, Michael

AU - Foster, Allen

AU - Carr, Michael A.

AU - LeClerc, Dave

AU - Fagan, Rad

AU - McElwain, Michael W.

AU - Knapp, Gillian

AU - Brandt, Timothy

AU - Janson, Markus

AU - Guyon, Olivier

AU - Jovanovic, Nemanja

AU - Martinache, Frantz

AU - Hayashi, Masahiko

AU - Takato, Naruhisa

PY - 2013

Y1 - 2013

N2 - High-contrast imaging techniques now make possible both imaging and spectroscopy of planets around nearby stars. We present the optical design for the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS), a lenslet-based, cryogenic integral field spectrograph (IFS) for imaging exoplanets on the Subaru telescope. The IFS will provide spectral information for 138×138 spatial elements over a 2.07 arcsec × 2.07 arcsec field of view (FOV). CHARIS will operate in the near infrared (λ = 1.15 - 2.5μm) and will feature two spectral resolution modes of R ≈ 18 (low-res mode) and R ≈ 73 (high-res mode). Taking advantage of the Subaru telescope adaptive optics systems and coronagraphs (AO188 and SCExAO), CHARIS will provide sufficient contrast to obtain spectra of young self-luminous Jupiter-mass exoplanets. CHARIS will undergo CDR in October 2013 and is projected to have first light by the end of 2015. We report here on the current optical design of CHARIS and its unique innovations.

AB - High-contrast imaging techniques now make possible both imaging and spectroscopy of planets around nearby stars. We present the optical design for the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS), a lenslet-based, cryogenic integral field spectrograph (IFS) for imaging exoplanets on the Subaru telescope. The IFS will provide spectral information for 138×138 spatial elements over a 2.07 arcsec × 2.07 arcsec field of view (FOV). CHARIS will operate in the near infrared (λ = 1.15 - 2.5μm) and will feature two spectral resolution modes of R ≈ 18 (low-res mode) and R ≈ 73 (high-res mode). Taking advantage of the Subaru telescope adaptive optics systems and coronagraphs (AO188 and SCExAO), CHARIS will provide sufficient contrast to obtain spectra of young self-luminous Jupiter-mass exoplanets. CHARIS will undergo CDR in October 2013 and is projected to have first light by the end of 2015. We report here on the current optical design of CHARIS and its unique innovations.

KW - Adaptive Optics

KW - Coronagraphy

KW - Exoplanets

KW - High Contrast Imaging

KW - Integral Field Spectrograph

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U2 - 10.1117/12.2024070

DO - 10.1117/12.2024070

M3 - Conference contribution

AN - SCOPUS:84888986534

SN - 9780819497147

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Techniques and Instrumentation for Detection of Exoplanets VI

Y2 - 26 August 2013 through 29 August 2013

ER -

The optical design of CHARIS: An exoplanet IFS for the Subaru Telescope

Abstract

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All Science Journal Classification (ASJC) codes

Keywords

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