Spectrally dispersed kernel phase interferometry with SCExAO/CHARIS: proof of concept and calibration strategies

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE
A. Chaushev, Steph Sallum, J. Lozi, F. Martinache, J. Chilcote, T. Groff, O. Guyon, J. Kasdin, B. Norris, A. Skemer
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引用次数: 2

Abstract

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.
SCExAO/CHARIS的光谱分散核相干涉测量:概念验证和校准策略
摘要核相位干涉(KPI)是一种数据处理技术,允许在接近并在经典衍射极限内的高strehl图像中检测不对称性(例如伴星或圆盘)。我们证明KPI可以成功地应用于由积分场光谱仪(ifs)生成的高光谱图像立方体。我们通过在高分辨率k波段模式下使用SCExAO/CHARIS IFS恢复已知的二进制数据来演示这种光谱分散核相技术。我们还探索了一种光谱差分成像(SDI)校准策略,该策略利用了来自多个波长箱的图像中的可用信息。这种校准有可能减轻高阶,残余的系统核相位误差,目前限制了KPI的可实现对比。提出的SDI校准适用于线发射或锐吸收特征的搜索,是实现光子噪声限制核相观测的有希望的途径。分散核相提供的高角分辨率和光谱覆盖范围为科学观测提供了机会,否则很难实现。
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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
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