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dc.contributor.authorChaushev, A.
dc.contributor.authorSallum, S.
dc.contributor.authorLozi, J.
dc.contributor.authorMartinache, F.
dc.contributor.authorChilcote, J.
dc.contributor.authorGroff, T.
dc.contributor.authorGuyon, O.
dc.contributor.authorKasdin, J.
dc.contributor.authorNorris, B.
dc.contributor.authorSkemer, A.
dc.date.accessioned2024-08-05T18:56:50Z
dc.date.available2024-08-05T18:56:50Z
dc.date.issued2023-05-03
dc.identifier.citationAlexander 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.9.2.028004
dc.identifier.issn2329-4124
dc.identifier.doi10.1117/1.JATIS.9.2.028004
dc.identifier.urihttp://hdl.handle.net/10150/673780
dc.description.abstractKernel 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.
dc.language.isoen
dc.publisherSPIE
dc.rights© The Authors. Published by SPIE under a Creative Commons Attribution 4.0 International License.
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectcalibration
dc.subjectdata processing
dc.subjecthigh angular resolution
dc.subjectkernel phase
dc.titleSpectrally dispersed kernel phase interferometry with SCExAO/CHARIS: proof of concept and calibration strategies
dc.typeArticle
dc.typetext
dc.contributor.departmentSteward Observatory, University of Arizona
dc.identifier.journalJournal of Astronomical Telescopes, Instruments, and Systems
dc.description.noteImmediate access
dc.description.collectioninformationThis 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.
dc.eprint.versionFinal Published Version
dc.source.journaltitleJournal of Astronomical Telescopes, Instruments, and Systems
refterms.dateFOA2024-08-05T18:56:50Z


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© The Authors. Published by SPIE under a Creative Commons Attribution 4.0 International License.
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.