Astronomical observations often involve capturing faint signals from celestial objects, such as distant galaxies or dim stars. These signals can be easily overwhelmed by noise, which includes electronic noise, atmospheric interference, and other artifacts. It is then clear that using an effective denoising algorithm is crucial to improve the accuracy of data interpretation by extracting the actual astronomical signals from the noisy background. In this work, we introduce a novel denoising approach based on deep neural networks with pixel attention derived from the topological structure extracted by 0-dimensional Persistent Homology (PH). Our network architecture combines an AutoEncoder (AE) with a Topological Module (TM) that assigns weights to pixels based on PH, providing nuanced attention to the relevant image regions. Our methodology is evaluated against widely used denoising methods, showcasing its potential for enhancing the quality of astronomical images.
Topological attention for denoising astronomical images / Ceccaroni, Riccardo; Brutti, Pierpaolo. - (2024), pp. 316-321. (Intervento presentato al convegno Statistics and Data Science Conference, SDS 2024 tenutosi a Palermo, Italy).
Topological attention for denoising astronomical images
Riccardo Ceccaroni;Pierpaolo Brutti
2024
Abstract
Astronomical observations often involve capturing faint signals from celestial objects, such as distant galaxies or dim stars. These signals can be easily overwhelmed by noise, which includes electronic noise, atmospheric interference, and other artifacts. It is then clear that using an effective denoising algorithm is crucial to improve the accuracy of data interpretation by extracting the actual astronomical signals from the noisy background. In this work, we introduce a novel denoising approach based on deep neural networks with pixel attention derived from the topological structure extracted by 0-dimensional Persistent Homology (PH). Our network architecture combines an AutoEncoder (AE) with a Topological Module (TM) that assigns weights to pixels based on PH, providing nuanced attention to the relevant image regions. Our methodology is evaluated against widely used denoising methods, showcasing its potential for enhancing the quality of astronomical images.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.