SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies

Julien Lozi; Olivier Guyon; Nemanja Jovanovic; Sean Goebel; Prashant Pathak; Nour Skaf; Ananya Sahoo; Barnaby Norris; Frantz Martinache; Mamadou N'Diaye; Ben Mazin; Alex B. Walter; Peter Tuthill; Tomoyuki Kudo; Hajime Kawahara; Takayuki Kotani; Michael Ireland; Nick Cvetojevic; Elsa Huby; Sylvestre Lacour; Sébastien Vievard; Tyler D. Groff; Jeffrey K. Chilcote; Jeremy Kasdin; Justin Knight; Frans Snik; David Doelman; Yosuke Minowa; Christophe Clergeon; Naruhisa Takato; Motohide Tamura; Thayne Currie; Hideki Takami; Masa Hayashi

doi:10.1117/12.2314282

SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies

Julien Lozi^*, Olivier Guyon, Nemanja Jovanovic, Sean Goebel, Prashant Pathak, Nour Skaf, Ananya Sahoo, Barnaby Norris, Frantz Martinache, Mamadou N'Diaye, Ben Mazin, Alex B. Walter, Peter Tuthill, Tomoyuki Kudo, Hajime Kawahara, Takayuki Kotani, Michael Ireland, Nick Cvetojevic, Elsa Huby, Sylvestre LacourSébastien Vievard, Tyler D. Groff, Jeffrey K. Chilcote, Jeremy Kasdin, Justin Knight, Frans Snik, David Doelman, Yosuke Minowa, Christophe Clergeon, Naruhisa Takato, Motohide Tamura, Thayne Currie, Hideki Takami, Masa Hayashi

^*Corresponding author for this work

Australian Astronomical Optics

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

46 Citations (Scopus)

Abstract

The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is an extremely modular high- contrast instrument installed on the Subaru telescope in Hawaii. SCExAO has a dual purpose. Its position in the northern hemisphere on a 8-meter telescope makes it a prime instrument for the detection and characterization of exoplanets and stellar environments over a large portion of the sky. In addition, SCExAO's unique design makes it the ideal instrument to test innovative technologies and algorithms quickly in a laboratory setup and subsequently deploy them on-sky. SCExAO benefits from a first stage of wavefront correction with the facility adaptive optics AO188, and splits the 600-2400 nm spectrum towards a variety of modules, in visible and near infrared, optimized for a large range of science cases. The integral field spectrograph CHARIS, with its J, H or K-band high-resolution mode or its broadband low-resolution mode, makes SCExAO a prime instrument for exoplanet detection and characterization. Here we report on the recent developments and scientific results of the SCExAO instrument. Recent upgrades were performed on a number of modules, like the visible polarimetric module VAMPIRES, the high-performance infrared coronagraphs, various wavefront control algorithms, as well as the real-time controller of AO188. The newest addition is the 20k-pixel Microwave Kinetic Inductance Detector (MKIDS) Exoplanet Camera (MEC) that will allow for previously unexplored science and technology developments. MEC, coupled with novel photon-counting speckle control, brings SCExAO closer to the final design of future high-contrast instruments optimized for Giant Segmented Mirror Telescopes (GSMTs).

Original language	English
Title of host publication	Adaptive Optics Systems VI
Editors	Laird M. Close, Laura Schreiber, Dirk Schmidt
Place of Publication	Bellingham, Washington
Publisher	SPIE
Pages	1-12
Number of pages	12
ISBN (Electronic)	9781510619609
ISBN (Print)	9781510619593
DOIs	https://doi.org/10.1117/12.2314282
Publication status	Published - 13 Jul 2018
Event	Adaptive Optics Systems VI 2018 - Austin, United States Duration: 10 Jun 2018 → 15 Jun 2018

Publication series

Name	Proceedings of SPIE
Publisher	SPIE
Volume	10703
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Adaptive Optics Systems VI 2018
Country/Territory	United States
City	Austin
Period	10/06/18 → 15/06/18

Keywords

Coronagraphy
Extreme Adaptive Optics
High-Contrast Imaging
MKID
Polarimetry
Pyramid Wavefront Sensor
Single-Mode Fiber Injection

Access to Document

10.1117/12.2314282

Cite this

Lozi, J., Guyon, O., Jovanovic, N., Goebel, S., Pathak, P., Skaf, N., Sahoo, A., Norris, B., Martinache, F., N'Diaye, M., Mazin, B., Walter, A. B., Tuthill, P., Kudo, T., Kawahara, H., Kotani, T., Ireland, M., Cvetojevic, N., Huby, E., ... Hayashi, M. (2018). SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies. In L. M. Close, L. Schreiber, & D. Schmidt (Eds.), Adaptive Optics Systems VI (pp. 1-12). Article 1070359 (Proceedings of SPIE; Vol. 10703). SPIE. https://doi.org/10.1117/12.2314282

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title = "SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies",

abstract = "The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is an extremely modular high- contrast instrument installed on the Subaru telescope in Hawaii. SCExAO has a dual purpose. Its position in the northern hemisphere on a 8-meter telescope makes it a prime instrument for the detection and characterization of exoplanets and stellar environments over a large portion of the sky. In addition, SCExAO's unique design makes it the ideal instrument to test innovative technologies and algorithms quickly in a laboratory setup and subsequently deploy them on-sky. SCExAO benefits from a first stage of wavefront correction with the facility adaptive optics AO188, and splits the 600-2400 nm spectrum towards a variety of modules, in visible and near infrared, optimized for a large range of science cases. The integral field spectrograph CHARIS, with its J, H or K-band high-resolution mode or its broadband low-resolution mode, makes SCExAO a prime instrument for exoplanet detection and characterization. Here we report on the recent developments and scientific results of the SCExAO instrument. Recent upgrades were performed on a number of modules, like the visible polarimetric module VAMPIRES, the high-performance infrared coronagraphs, various wavefront control algorithms, as well as the real-time controller of AO188. The newest addition is the 20k-pixel Microwave Kinetic Inductance Detector (MKIDS) Exoplanet Camera (MEC) that will allow for previously unexplored science and technology developments. MEC, coupled with novel photon-counting speckle control, brings SCExAO closer to the final design of future high-contrast instruments optimized for Giant Segmented Mirror Telescopes (GSMTs).",

keywords = "Coronagraphy, Extreme Adaptive Optics, High-Contrast Imaging, MKID, Polarimetry, Pyramid Wavefront Sensor, Single-Mode Fiber Injection",

author = "Julien Lozi and Olivier Guyon and Nemanja Jovanovic and Sean Goebel and Prashant Pathak and Nour Skaf and Ananya Sahoo and Barnaby Norris and Frantz Martinache and Mamadou N'Diaye and Ben Mazin and Walter, {Alex B.} and Peter Tuthill and Tomoyuki Kudo and Hajime Kawahara and Takayuki Kotani and Michael Ireland and Nick Cvetojevic and Elsa Huby and Sylvestre Lacour and S{\'e}bastien Vievard and Groff, {Tyler D.} and Chilcote, {Jeffrey K.} and Jeremy Kasdin and Justin Knight and Frans Snik and David Doelman and Yosuke Minowa and Christophe Clergeon and Naruhisa Takato and Motohide Tamura and Thayne Currie and Hideki Takami and Masa Hayashi",

year = "2018",

month = jul,

day = "13",

doi = "10.1117/12.2314282",

language = "English",

isbn = "9781510619593",

series = "Proceedings of SPIE",

publisher = "SPIE",

pages = "1--12",

editor = "Close, {Laird M.} and Laura Schreiber and Dirk Schmidt",

booktitle = "Adaptive Optics Systems VI",

address = "United States",

note = "Adaptive Optics Systems VI 2018 ; Conference date: 10-06-2018 Through 15-06-2018",

}

Lozi, J, Guyon, O, Jovanovic, N, Goebel, S, Pathak, P, Skaf, N, Sahoo, A, Norris, B, Martinache, F, N'Diaye, M, Mazin, B, Walter, AB, Tuthill, P, Kudo, T, Kawahara, H, Kotani, T, Ireland, M, Cvetojevic, N, Huby, E, Lacour, S, Vievard, S, Groff, TD, Chilcote, JK, Kasdin, J, Knight, J, Snik, F, Doelman, D, Minowa, Y, Clergeon, C, Takato, N, Tamura, M, Currie, T, Takami, H & Hayashi, M 2018, SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies. in LM Close, L Schreiber & D Schmidt (eds), Adaptive Optics Systems VI., 1070359, Proceedings of SPIE, vol. 10703, SPIE, Bellingham, Washington, pp. 1-12, Adaptive Optics Systems VI 2018, Austin, United States, 10/06/18. https://doi.org/10.1117/12.2314282

SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies. / Lozi, Julien; Guyon, Olivier; Jovanovic, Nemanja et al.
Adaptive Optics Systems VI. ed. / Laird M. Close; Laura Schreiber; Dirk Schmidt. Bellingham, Washington: SPIE, 2018. p. 1-12 1070359 (Proceedings of SPIE; Vol. 10703).

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

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AU - Kudo, Tomoyuki

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AU - Huby, Elsa

AU - Lacour, Sylvestre

AU - Vievard, Sébastien

AU - Groff, Tyler D.

AU - Chilcote, Jeffrey K.

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AU - Knight, Justin

AU - Snik, Frans

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AU - Takami, Hideki

AU - Hayashi, Masa

PY - 2018/7/13

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N2 - The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is an extremely modular high- contrast instrument installed on the Subaru telescope in Hawaii. SCExAO has a dual purpose. Its position in the northern hemisphere on a 8-meter telescope makes it a prime instrument for the detection and characterization of exoplanets and stellar environments over a large portion of the sky. In addition, SCExAO's unique design makes it the ideal instrument to test innovative technologies and algorithms quickly in a laboratory setup and subsequently deploy them on-sky. SCExAO benefits from a first stage of wavefront correction with the facility adaptive optics AO188, and splits the 600-2400 nm spectrum towards a variety of modules, in visible and near infrared, optimized for a large range of science cases. The integral field spectrograph CHARIS, with its J, H or K-band high-resolution mode or its broadband low-resolution mode, makes SCExAO a prime instrument for exoplanet detection and characterization. Here we report on the recent developments and scientific results of the SCExAO instrument. Recent upgrades were performed on a number of modules, like the visible polarimetric module VAMPIRES, the high-performance infrared coronagraphs, various wavefront control algorithms, as well as the real-time controller of AO188. The newest addition is the 20k-pixel Microwave Kinetic Inductance Detector (MKIDS) Exoplanet Camera (MEC) that will allow for previously unexplored science and technology developments. MEC, coupled with novel photon-counting speckle control, brings SCExAO closer to the final design of future high-contrast instruments optimized for Giant Segmented Mirror Telescopes (GSMTs).

AB - The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is an extremely modular high- contrast instrument installed on the Subaru telescope in Hawaii. SCExAO has a dual purpose. Its position in the northern hemisphere on a 8-meter telescope makes it a prime instrument for the detection and characterization of exoplanets and stellar environments over a large portion of the sky. In addition, SCExAO's unique design makes it the ideal instrument to test innovative technologies and algorithms quickly in a laboratory setup and subsequently deploy them on-sky. SCExAO benefits from a first stage of wavefront correction with the facility adaptive optics AO188, and splits the 600-2400 nm spectrum towards a variety of modules, in visible and near infrared, optimized for a large range of science cases. The integral field spectrograph CHARIS, with its J, H or K-band high-resolution mode or its broadband low-resolution mode, makes SCExAO a prime instrument for exoplanet detection and characterization. Here we report on the recent developments and scientific results of the SCExAO instrument. Recent upgrades were performed on a number of modules, like the visible polarimetric module VAMPIRES, the high-performance infrared coronagraphs, various wavefront control algorithms, as well as the real-time controller of AO188. The newest addition is the 20k-pixel Microwave Kinetic Inductance Detector (MKIDS) Exoplanet Camera (MEC) that will allow for previously unexplored science and technology developments. MEC, coupled with novel photon-counting speckle control, brings SCExAO closer to the final design of future high-contrast instruments optimized for Giant Segmented Mirror Telescopes (GSMTs).

KW - Coronagraphy

KW - Extreme Adaptive Optics

KW - High-Contrast Imaging

KW - MKID

KW - Polarimetry

KW - Pyramid Wavefront Sensor

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T3 - Proceedings of SPIE

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PB - SPIE

CY - Bellingham, Washington

Y2 - 10 June 2018 through 15 June 2018

ER -

SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies

Abstract

Publication series

Conference

Keywords

Access to Document

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