An alternating minimization algorithm with trajectory for direct exoplanet detection

The AMAT algorithm

¹ ICTEAM Institute, UCLouvain, 1348 Louvain-la-Neuve, Belgium
² Vlaamse Instelling voor Technologisch Onderzoek (VITO), 2400 Mol, Belgium
³ Department of Statistics, University of Oxford, Oxford, UK
⁴ STAR Institute, Université de Liège, 4000 Liège, Belgium
⁵ Univ. Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France
⁶ Deptartment of Mathematics and Operational Research, University of Mons, Mons, Belgium
⁷ Innopolis University, Innopolis, Russia

^★ Corresponding author; hazan.daglayan@uclouvain.be

Received: 25 June 2024
Accepted: 8 October 2024

Abstract

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.