2023A&A...679A..18R


Query : 2023A&A...679A..18R

2023A&A...679A..18R - Astronomy and Astrophysics, volume 679A18 (2023/11-1)

Karhunen-Loève data imputation in high-contrast imaging.

REN B.B.

Abstract (from CDS):

The detection and characterization of extended structures is a crucial goal in high-contrast imaging. However, these structures face challenges in data reduction, leading to over-subtraction from speckles and self-subtraction with most existing methods. Iterative post-processing methods offer promising results, but their integration into existing pipelines is hindered by selective algorithms, the high computational cost, and algorithmic regularization. To address this for reference differential imaging (RDI), here we propose a data imputation concept for the Karhunen-Loève transform (DIKL) by modifying two steps in the standard Karhunen-Loève image projection (KLIP) method. Specifically, we partition an image to two matrices: an anchor matrix that focuses only on the speckles to obtain the DIKL coefficients, and a boat matrix that focuses on the regions of astrophysical interest for speckle removal using DIKL components. As an analytical approach, DIKL achieves high-quality results with significantly reduced computational cost (∼3 orders of magnitude less than iterative methods). Being a derivative method of KLIP, DIKL is seamlessly integrable into high-contrast imaging pipelines for RDI observations.

Abstract Copyright: © The Authors 2023

Journal keyword(s): circumstellar matter - quasars: general - techniques: high angular resolution - techniques: image processing - methods: statistical

VizieR on-line data: <Available at CDS (J/A+A/679/A18): list.dat fits/*>

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V351 Ori Ae* 05 44 18.7949456328 +00 08 40.410217104 9.44 9.22 8.87     A7V 128 0
2 HD 129590 * 14 44 30.9625895592 -39 59 20.628246480   9.96 9.33     G3V 73 0
3 HD 169142 Ae* 18 24 29.7799891464 -29 46 49.327400568   8.42 8.16     F1VekA3mA3_lB? 535 0

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