Article (Scientific journals)
An alternating minimization algorithm with trajectory for direct exoplanet detection: The AMAT algorithm
Daglayan, H.; Vary, S.; Absil, Olivier et al.
2024In Astronomy and Astrophysics, 692, p. 126
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Keywords :
methods: data analysis; techniques: image processing; planets and; satellites: detection
Abstract :
[en] Context. Effective image post-processing algorithms are vital for the successful direct imaging of exoplanets. Standard point spread function (PSF) subtraction methods use techniques based on a low-rank approximation to separate the rotating planet signal from the quasi-static speckles and rely on signal-to-noise ratio maps to detect the planet. These steps do not interact or feed each other, leading to potential limitations in the accuracy and efficiency of exoplanet detection. Aims. We aim to develop a novel approach that iteratively finds the flux of the planet and the low-rank approximation of quasi-static signals in an attempt to improve upon current PSF subtraction techniques. Methods. In this study, we extend the standard L2 norm minimization paradigm to an L1 norm minimization framework in order to better account for noise statistics in the high contrast images. Then, we propose a new method, referred to as the alternating minimization algorithm with trajectory (AMAT), that makes more advanced use of estimating the low-rank approximation of the speckle field and the planet flux by alternating between them and utilizing both L1 and L2 norms. For the L1 norm minimization, we propose using L1 norm low-rank approximation (L1-LRA), a low-rank approximation computed using an exact block-cyclic coordinate descent method, while we use randomized singular value decomposition for the L2 norm minimization. Additionally, we enhance the visibility of the planet signal using a likelihood ratio as a post-processing step. Results. Numerical experiments performed on a VLT/SPHERE-IRDIS dataset show the potential of AMAT to improve upon the existing approaches in terms of higher S/N, sensitivity limits (contrast curves), and receiver operating characteristic curves. Moreover, for a systematic comparison, we used datasets from the exoplanet data challenge to compare our algorithm with other algorithms in the challenge, and we find AMAT with a likelihood ratio map performs better than most algorithms tested on the exoplanet data challenge.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Daglayan, H.;  ICTEAM Institute, UCLouvain, 1348, Louvain-la-Neuve, Belgium, Vlaamse Instelling voor Technologisch Onderzoek (VITO), 2400, Mol, Belgium,
Vary, S.;  University of Oxford, UK
Absil, Olivier  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO)
Cantalloube, F.;  Institute de Planetologie et d'Astrophysique de Grenoble
Christiaens, Valentin  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Planetary & Stellar systems Imaging Laboratory
Gillis, N.;  Deptartment of Mathematics and Operational Research, University of Mons, Mons, Belgium
Jacques, L.;  ICTEAM Institute, UCLouvain, 1348, Louvain-la-Neuve, Belgium,
Leplat, V.;  Innopolis University, Tatarstan
Absil, P. -A.;  ICTEAM Institute, UCLouvain, 1348, Louvain-la-Neuve, Belgium,
Language :
English
Title :
An alternating minimization algorithm with trajectory for direct exoplanet detection: The AMAT algorithm
Publication date :
06 December 2024
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP
Volume :
692
Pages :
A126
Peer reviewed :
Peer Reviewed verified by ORBi
European Projects :
H2020 - 819155 - EPIC - Earth-like Planet Imaging with Cognitive computing
Funders :
ERC - European Research Council
F.R.S.-FNRS - Fonds de la Recherche Scientifique
BELSPO - Belgian Federal Science Policy Office
European Union
Commentary :
Copyright ESO 2024, published by EDP Sciences - https://www.aanda.org/articles/aa/full_html/2024/12/aa51242-24/aa51242-24.html
Available on ORBi :
since 27 December 2024

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