High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS

Kellen Lawson; Thayne Currie; John P. Wisniewski; Jun Hashimoto; Olivier Guyon; N, Jeremy Kasdin; Tyler D. Groff; Julien Lozi; Timothy D. Brandt; Jeffrey Chilcote; Vincent Deo; Taichi Uyama; Sebastien Vievard

doi:10.1117/12.2594819

High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS

Kellen Lawson, Thayne Currie, John P. Wisniewski, Jun Hashimoto, Olivier Guyon, N, Jeremy Kasdin, Tyler D. Groff, Julien Lozi, Timothy D. Brandt, Jeffrey Chilcote, Vincent Deo, Taichi Uyama, Sebastien Vievard

Optical Sciences

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

1 Scopus citations

Abstract

We describe a new high-contrast imaging capability well suited for studying planet-forming disks: near-infrared (NIR) high-contrast spectropolarimetric imaging with the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system coupled with the CHARIS integral field spectrograph (IFS). The advent of extreme AO systems, like SCExAO, has enabled recovery of planet-mass companions at the expected locations of gas-giant formation in young disks alongside disk structures (such as gaps or spirals) that may indicate protoplanet formation. In combination with SCExAO, the CHARIS IFS in polarimetry mode allows characterization of these systems at wavelengths spanning the NIR J, H, and K bands (1.1-2.4 μm, R∼20) and at angular separations as small as 0.04".

Original language	English (US)
Title of host publication	Techniques and Instrumentation for Detection of Exoplanets X
Editors	Stuart B. Shaklan, Garreth J. Ruane
Publisher	SPIE
ISBN (Electronic)	9781510644847
DOIs	https://doi.org/10.1117/12.2594819
State	Published - 2021
Event	Techniques and Instrumentation for Detection of Exoplanets X 2021 - San Diego, United States Duration: Aug 1 2021 → Aug 5 2021

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11823
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Techniques and Instrumentation for Detection of Exoplanets X 2021
Country/Territory	United States
City	San Diego
Period	8/1/21 → 8/5/21

ASJC Scopus subject areas

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

Access to Document

10.1117/12.2594819

Cite this

Lawson, K., Currie, T., Wisniewski, J. P., Hashimoto, J., Guyon, O., Kasdin, N. J., Groff, T. D., Lozi, J., Brandt, T. D., Chilcote, J., Deo, V., Uyama, T., & Vievard, S. (2021). High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS. In S. B. Shaklan, & G. J. Ruane (Eds.), Techniques and Instrumentation for Detection of Exoplanets X [118230D] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11823). SPIE. https://doi.org/10.1117/12.2594819

High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS. / Lawson, Kellen; Currie, Thayne; Wisniewski, John P. et al.

Techniques and Instrumentation for Detection of Exoplanets X. ed. / Stuart B. Shaklan; Garreth J. Ruane. SPIE, 2021. 118230D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11823).

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

Lawson, K, Currie, T, Wisniewski, JP, Hashimoto, J, Guyon, O, Kasdin, NJ, Groff, TD, Lozi, J, Brandt, TD, Chilcote, J, Deo, V, Uyama, T & Vievard, S 2021, High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS. in SB Shaklan & GJ Ruane (eds), Techniques and Instrumentation for Detection of Exoplanets X., 118230D, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11823, SPIE, Techniques and Instrumentation for Detection of Exoplanets X 2021, San Diego, United States, 8/1/21. https://doi.org/10.1117/12.2594819

Lawson K, Currie T, Wisniewski JP, Hashimoto J, Guyon O, Kasdin NJ et al. High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS. In Shaklan SB, Ruane GJ, editors, Techniques and Instrumentation for Detection of Exoplanets X. SPIE. 2021. 118230D. (Proceedings of SPIE - The International Society for Optical Engineering). https://doi.org/10.1117/12.2594819

@inproceedings{90969e6777d34b4a92774a47fdc3bf18,

title = "High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS",

abstract = "We describe a new high-contrast imaging capability well suited for studying planet-forming disks: near-infrared (NIR) high-contrast spectropolarimetric imaging with the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system coupled with the CHARIS integral field spectrograph (IFS). The advent of extreme AO systems, like SCExAO, has enabled recovery of planet-mass companions at the expected locations of gas-giant formation in young disks alongside disk structures (such as gaps or spirals) that may indicate protoplanet formation. In combination with SCExAO, the CHARIS IFS in polarimetry mode allows characterization of these systems at wavelengths spanning the NIR J, H, and K bands (1.1-2.4 μm, R∼20) and at angular separations as small as 0.04{"}.",

author = "Kellen Lawson and Thayne Currie and Wisniewski, {John P.} and Jun Hashimoto and Olivier Guyon and Kasdin, {N, Jeremy} and Groff, {Tyler D.} and Julien Lozi and Brandt, {Timothy D.} and Jeffrey Chilcote and Vincent Deo and Taichi Uyama and Sebastien Vievard",

note = "Funding Information: The development of SCExAO was supported by the Japan Society for the Promotion of Science (Grant-in-Aid for Research #23340051, #26220704, #23103002, #19H00703 & #19H00695), the Astrobiology Center of the National Institutes of Natural Sciences, Japan, the Mt Cuba Foundation and the director{\textquoteright}s contingency fund at Subaru Telescope. We acknowledge funding support from the NASA XRP program via grants 80NSSC20K0252 and NNX17AF88G. T.C. was supported by a NASA Senior Postdoctoral Fellowship. Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Techniques and Instrumentation for Detection of Exoplanets X 2021 ; Conference date: 01-08-2021 Through 05-08-2021",

year = "2021",

doi = "10.1117/12.2594819",

language = "English (US)",

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

publisher = "SPIE",

editor = "Shaklan, {Stuart B.} and Ruane, {Garreth J.}",

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

}

TY - GEN

T1 - High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS

AU - Lawson, Kellen

AU - Currie, Thayne

AU - Wisniewski, John P.

AU - Hashimoto, Jun

AU - Guyon, Olivier

AU - Kasdin, N, Jeremy

AU - Groff, Tyler D.

AU - Lozi, Julien

AU - Brandt, Timothy D.

AU - Chilcote, Jeffrey

AU - Deo, Vincent

AU - Uyama, Taichi

AU - Vievard, Sebastien

N1 - Funding Information: The development of SCExAO was supported by the Japan Society for the Promotion of Science (Grant-in-Aid for Research #23340051, #26220704, #23103002, #19H00703 & #19H00695), the Astrobiology Center of the National Institutes of Natural Sciences, Japan, the Mt Cuba Foundation and the director’s contingency fund at Subaru Telescope. We acknowledge funding support from the NASA XRP program via grants 80NSSC20K0252 and NNX17AF88G. T.C. was supported by a NASA Senior Postdoctoral Fellowship. Publisher Copyright: © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.

PY - 2021

Y1 - 2021

N2 - We describe a new high-contrast imaging capability well suited for studying planet-forming disks: near-infrared (NIR) high-contrast spectropolarimetric imaging with the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system coupled with the CHARIS integral field spectrograph (IFS). The advent of extreme AO systems, like SCExAO, has enabled recovery of planet-mass companions at the expected locations of gas-giant formation in young disks alongside disk structures (such as gaps or spirals) that may indicate protoplanet formation. In combination with SCExAO, the CHARIS IFS in polarimetry mode allows characterization of these systems at wavelengths spanning the NIR J, H, and K bands (1.1-2.4 μm, R∼20) and at angular separations as small as 0.04".

AB - We describe a new high-contrast imaging capability well suited for studying planet-forming disks: near-infrared (NIR) high-contrast spectropolarimetric imaging with the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system coupled with the CHARIS integral field spectrograph (IFS). The advent of extreme AO systems, like SCExAO, has enabled recovery of planet-mass companions at the expected locations of gas-giant formation in young disks alongside disk structures (such as gaps or spirals) that may indicate protoplanet formation. In combination with SCExAO, the CHARIS IFS in polarimetry mode allows characterization of these systems at wavelengths spanning the NIR J, H, and K bands (1.1-2.4 μm, R∼20) and at angular separations as small as 0.04".

UR - http://www.scopus.com/inward/record.url?scp=85117442154&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85117442154&partnerID=8YFLogxK

U2 - 10.1117/12.2594819

DO - 10.1117/12.2594819

M3 - Conference contribution

AN - SCOPUS:85117442154

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

BT - Techniques and Instrumentation for Detection of Exoplanets X

A2 - Shaklan, Stuart B.

A2 - Ruane, Garreth J.

PB - SPIE

T2 - Techniques and Instrumentation for Detection of Exoplanets X 2021

Y2 - 1 August 2021 through 5 August 2021

ER -

High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS

Abstract

Publication series

Conference

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this