The SCExAO high contrast imager: Transitioning from commissioning to science

N. Jovanovic; O. Guyon; J. Lozi; T. Currie; J. Hagelberg; B. Norris; G. Singh; P. Pathak; D. Doughty; S. Goebel; J. Males; J. Kuhn; E. Serabyn; P. Tuthill; G. Schworer; F. Martinache; T. Kudo; H. Kawahara; T. Kotani; M. Ireland; T. Feger; A. Rains; J. Bento; C. Schwab; D. Coutts; N. Cvetojevic; S. Gross; A. Arriola; T. Lagadec; J. Kasdin; T. Groff; B. Mazin; Y. Minowa; N. Takato; M. Tamura; H. Takami; M. Hayashi

doi:10.1117/12.2234294

The SCExAO high contrast imager: Transitioning from commissioning to science

N. Jovanovic, O. Guyon, J. Lozi, T. Currie, J. Hagelberg, B. Norris, G. Singh, P. Pathak, D. Doughty, S. Goebel, J. Males, J. Kuhn, E. Serabyn, P. Tuthill, G. Schworer, F. Martinache, T. Kudo, H. Kawahara, T. Kotani, M. IrelandT. Feger, A. Rains, J. Bento, C. Schwab, D. Coutts, N. Cvetojevic, S. Gross, A. Arriola, T. Lagadec, J. Kasdin, T. Groff, B. Mazin, Y. Minowa, N. Takato, M. Tamura, H. Takami, M. Hayashi

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

18 Scopus citations

Abstract

SCExAO is the premier high-contrast imaging platform for the Subaru Telescope. It offers high Strehl ratios at near-IR wavelengths (y-K band) with stable pointing and coronagraphs with extremely small inner working angles, optimized for imaging faint companions very close to the host. In the visible, it has several interferometric imagers which offer polarimetric and spectroscopic capabilities. A recent addition is the RHEA spectrograph enabling spatially resolved high resolution spectroscopy of the surfaces of giant stars, for example. New capabilities on the horizon include post-coronagraphic spectroscopy, spectral differential imaging, nulling interferometry as well as an integral field spectrograph and an MKID array. Here we present the new modules of SCExAO, give an overview of the current commissioning status of each of the modules and present preliminary results.

Original language	English (US)
Title of host publication	Adaptive Optics Systems V
Editors	Enrico Marchetti, Jean-Pierre Veran, Laird M. Close
Publisher	SPIE
ISBN (Electronic)	9781510601970
DOIs	https://doi.org/10.1117/12.2234294
State	Published - 2016
Event	Adaptive Optics Systems V - Edinburgh, United Kingdom Duration: Jun 26 2016 → Jul 1 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9909
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Adaptive Optics Systems V
Country/Territory	United Kingdom
City	Edinburgh
Period	6/26/16 → 7/1/16

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
Coro-nagraphs
Exoplanets
Extreme AO
Fiber injection
High contrast imaging
Imager
Sparse aperture masking

Access to Document

10.1117/12.2234294

Cite this

Jovanovic, N., Guyon, O., Lozi, J., Currie, T., Hagelberg, J., Norris, B., Singh, G., Pathak, P., Doughty, D., Goebel, S., Males, J., Kuhn, J., Serabyn, E., Tuthill, P., Schworer, G., Martinache, F., Kudo, T., Kawahara, H., Kotani, T., ... Hayashi, M. (2016). The SCExAO high contrast imager: Transitioning from commissioning to science. In E. Marchetti, J.-P. Veran, & L. M. Close (Eds.), Adaptive Optics Systems V Article 99090W (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9909). SPIE. https://doi.org/10.1117/12.2234294

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title = "The SCExAO high contrast imager: Transitioning from commissioning to science",

abstract = "SCExAO is the premier high-contrast imaging platform for the Subaru Telescope. It offers high Strehl ratios at near-IR wavelengths (y-K band) with stable pointing and coronagraphs with extremely small inner working angles, optimized for imaging faint companions very close to the host. In the visible, it has several interferometric imagers which offer polarimetric and spectroscopic capabilities. A recent addition is the RHEA spectrograph enabling spatially resolved high resolution spectroscopy of the surfaces of giant stars, for example. New capabilities on the horizon include post-coronagraphic spectroscopy, spectral differential imaging, nulling interferometry as well as an integral field spectrograph and an MKID array. Here we present the new modules of SCExAO, give an overview of the current commissioning status of each of the modules and present preliminary results.",

keywords = "Adaptive optics, Coro-nagraphs, Exoplanets, Extreme AO, Fiber injection, High contrast imaging, Imager, Sparse aperture masking",

author = "N. Jovanovic and O. Guyon and J. Lozi and T. Currie and J. Hagelberg and B. Norris and G. Singh and P. Pathak and D. Doughty and S. Goebel and J. Males and J. Kuhn and E. Serabyn and P. Tuthill and G. Schworer and F. Martinache and T. Kudo and H. Kawahara and T. Kotani and M. Ireland and T. Feger and A. Rains and J. Bento and C. Schwab and D. Coutts and N. Cvetojevic and S. Gross and A. Arriola and T. Lagadec and J. Kasdin and T. Groff and B. Mazin and Y. Minowa and N. Takato and M. Tamura and H. Takami and M. Hayashi",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Adaptive Optics Systems V ; Conference date: 26-06-2016 Through 01-07-2016",

year = "2016",

doi = "10.1117/12.2234294",

language = "English (US)",

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

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editor = "Enrico Marchetti and Jean-Pierre Veran and Close, {Laird M.}",

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Jovanovic, N, Guyon, O, Lozi, J, Currie, T, Hagelberg, J, Norris, B, Singh, G, Pathak, P, Doughty, D, Goebel, S, Males, J, Kuhn, J, Serabyn, E, Tuthill, P, Schworer, G, Martinache, F, Kudo, T, Kawahara, H, Kotani, T, Ireland, M, Feger, T, Rains, A, Bento, J, Schwab, C, Coutts, D, Cvetojevic, N, Gross, S, Arriola, A, Lagadec, T, Kasdin, J, Groff, T, Mazin, B, Minowa, Y, Takato, N, Tamura, M, Takami, H & Hayashi, M 2016, The SCExAO high contrast imager: Transitioning from commissioning to science. in E Marchetti, J-P Veran & LM Close (eds), Adaptive Optics Systems V., 99090W, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9909, SPIE, Adaptive Optics Systems V, Edinburgh, United Kingdom, 6/26/16. https://doi.org/10.1117/12.2234294

The SCExAO high contrast imager: Transitioning from commissioning to science. / Jovanovic, N.; Guyon, O.; Lozi, J. et al.
Adaptive Optics Systems V. ed. / Enrico Marchetti; Jean-Pierre Veran; Laird M. Close. SPIE, 2016. 99090W (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9909).

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

TY - GEN

T1 - The SCExAO high contrast imager

T2 - Adaptive Optics Systems V

AU - Jovanovic, N.

AU - Guyon, O.

AU - Lozi, J.

AU - Currie, T.

AU - Hagelberg, J.

AU - Norris, B.

AU - Singh, G.

AU - Pathak, P.

AU - Doughty, D.

AU - Goebel, S.

AU - Males, J.

AU - Kuhn, J.

AU - Serabyn, E.

AU - Tuthill, P.

AU - Schworer, G.

AU - Martinache, F.

AU - Kudo, T.

AU - Kawahara, H.

AU - Kotani, T.

AU - Ireland, M.

AU - Feger, T.

AU - Rains, A.

AU - Bento, J.

AU - Schwab, C.

AU - Coutts, D.

AU - Cvetojevic, N.

AU - Gross, S.

AU - Arriola, A.

AU - Lagadec, T.

AU - Kasdin, J.

AU - Groff, T.

AU - Mazin, B.

AU - Minowa, Y.

AU - Takato, N.

AU - Tamura, M.

AU - Takami, H.

AU - Hayashi, M.

PY - 2016

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N2 - SCExAO is the premier high-contrast imaging platform for the Subaru Telescope. It offers high Strehl ratios at near-IR wavelengths (y-K band) with stable pointing and coronagraphs with extremely small inner working angles, optimized for imaging faint companions very close to the host. In the visible, it has several interferometric imagers which offer polarimetric and spectroscopic capabilities. A recent addition is the RHEA spectrograph enabling spatially resolved high resolution spectroscopy of the surfaces of giant stars, for example. New capabilities on the horizon include post-coronagraphic spectroscopy, spectral differential imaging, nulling interferometry as well as an integral field spectrograph and an MKID array. Here we present the new modules of SCExAO, give an overview of the current commissioning status of each of the modules and present preliminary results.

AB - SCExAO is the premier high-contrast imaging platform for the Subaru Telescope. It offers high Strehl ratios at near-IR wavelengths (y-K band) with stable pointing and coronagraphs with extremely small inner working angles, optimized for imaging faint companions very close to the host. In the visible, it has several interferometric imagers which offer polarimetric and spectroscopic capabilities. A recent addition is the RHEA spectrograph enabling spatially resolved high resolution spectroscopy of the surfaces of giant stars, for example. New capabilities on the horizon include post-coronagraphic spectroscopy, spectral differential imaging, nulling interferometry as well as an integral field spectrograph and an MKID array. Here we present the new modules of SCExAO, give an overview of the current commissioning status of each of the modules and present preliminary results.

KW - Adaptive optics

KW - Coro-nagraphs

KW - Exoplanets

KW - Extreme AO

KW - Fiber injection

KW - High contrast imaging

KW - Imager

KW - Sparse aperture masking

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DO - 10.1117/12.2234294

M3 - Conference contribution

AN - SCOPUS:85001932779

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

BT - Adaptive Optics Systems V

A2 - Marchetti, Enrico

A2 - Veran, Jean-Pierre

A2 - Close, Laird M.

PB - SPIE

Y2 - 26 June 2016 through 1 July 2016

ER -

The SCExAO high contrast imager: Transitioning from commissioning to science

Abstract

Publication series

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All Science Journal Classification (ASJC) codes

Keywords

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