Presentation + Paper
1 September 2021 High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS
Author Affiliations +
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”.
Conference Presentation
© (2021) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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, and Sebastien Vievard "High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARIS", Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 118230D (1 September 2021); https://doi.org/10.1117/12.2594819
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KEYWORDS
Polarization

Data modeling

Point spread functions

Adaptive optics

Coronagraphy

Polarimetry

Calibration

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