Spectrally dispersed kernel phase interferometry with SCExAO/CHARIS: proof of concept and calibration strategies
Author
Chaushev, A.Sallum, S.

Lozi, J.
Martinache, F.

Chilcote, J.
Groff, T.
Guyon, O.

Kasdin, J.
Norris, B.
Skemer, A.
Affiliation
Steward Observatory, University of ArizonaIssue Date
2023-05-03
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Alexander Chaushev, Steph E. Sallum, Julien Lozi, Frantz Martinache, Jeffrey K. Chilcote, Tyler D. Groff, Olivier Guyon, N. Jeremy Kasdin, Barnaby R. M. Norris, and Andrew J. Skemer "Spectrally dispersed kernel phase interferometry with SCExAO/CHARIS: proof of concept and calibration strategies," Journal of Astronomical Telescopes, Instruments, and Systems 9(2), 028004 (3 May 2023). https://doi.org/10.1117/1.JATIS.9.2.028004Rights
© The Authors. Published by SPIE under a Creative Commons Attribution 4.0 International License.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Kernel phase interferometry (KPI) is a data processing technique that allows for the detection of asymmetries (such as companions or disks) in high-Strehl images, close to and within the classical diffraction limit. We show that KPI can successfully be applied to hyperspectral image cubes generated from integral field spectrographs (IFSs). We demonstrate this technique of spectrally dispersed kernel phase by recovering a known binary with the SCExAO/CHARIS IFS in high-resolution K-band mode. We also explore a spectral differential imaging (SDI) calibration strategy that takes advantage of the information available in images from multiple wavelength bins. Such calibrations have the potential to mitigate high-order, residual systematic kernel phase errors, which currently limit the achievable contrast of KPI. The SDI calibration presented is applicable to searches for line emission or sharp absorption features and is a promising avenue toward achieving photon-noise-limited kernel phase observations. The high angular resolution and spectral coverage provided by dispersed kernel phase offers opportunities for science observations that would have been challenging to achieve otherwise. © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 International License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.Note
Immediate accessISSN
2329-4124Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/1.JATIS.9.2.028004
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Except where otherwise noted, this item's license is described as © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 International License.