ShapeNet: Shape constraint for galaxy image deconvolution - CEA - Commissariat à l’énergie atomique et aux énergies alternatives Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2022

ShapeNet: Shape constraint for galaxy image deconvolution


Deep learning (DL) has shown remarkable results in solving inverse problems in various domains. In particular, the Tikhonet approach is very powerful in deconvolving optical astronomical images. However, this approach only uses the ℓ2 loss, which does not guarantee the preservation of physical information (e.g., flux and shape) of the object that is reconstructed in the image. A new loss function has been proposed in the framework of sparse deconvolution that better preserves the shape of galaxies and reduces the pixel error. In this paper, we extend the Tikhonet approach to take this shape constraint into account and apply our new DL method, called ShapeNet, to a simulated optical and radio-interferometry dataset. The originality of the paper relies on i) the shape constraint we use in the neural network framework, ii) the application of DL to radio-interferometry image deconvolution for the first time, and iii) the generation of a simulated radio dataset that we make available for the community. A range of examples illustrates the results.
Fichier principal
Vignette du fichier
aa42626-21.pdf (1.56 Mo) Télécharger le fichier
Origin : Publication funded by an institution

Dates and versions

cea-03728008 , version 1 (19-07-2022)



F. Nammour, U. Akhaury, J. N. Girard, F. Lanusse, F. Sureau, et al.. ShapeNet: Shape constraint for galaxy image deconvolution. Astronomy and Astrophysics - A&A, 2022, 663, pp.A69. ⟨10.1051/0004-6361/202142626⟩. ⟨cea-03728008⟩
12 View
30 Download



Gmail Facebook Twitter LinkedIn More