Machine Learning Workflow for Morphological Classification of Galaxies
Bernd Doser, Kai L. Polsterer, Andreas Fehlner, Sebastian, Trujillo-Gomez

TL;DR
This paper presents a comprehensive, reproducible machine learning workflow for classifying galaxy morphologies using deep learning, scalable to large datasets from exascale cosmological simulations.
Contribution
It introduces a full pipeline from data collection to deployment, emphasizing reproducibility, scalability, and open-source standards for galaxy morphological classification.
Findings
Effective reduction of complex galaxy data to low-dimensional spherical latent space
Enabling explorative visualization with Hierarchical Progressive Surveys (HiPS)
Workflow ensures reproducibility and scalability for large-scale astrophysical data
Abstract
As part of the EU-funded Center of Excellence SPACE (Scalable Parallel Astrophysical Codes for Exascale), seven commonly used astrophysics simulation codes are being optimized to exploit exascale computing platforms. Exascale cosmological simulations will produce large amounts of data (i.e. several petabytes) that will soon be waiting to be analyzed, with enormous potential for scientific breakthroughs. Our tool Spherinator enables the reduction of these complex data sets to a low-dimensional space using Generative Deep Learning to understand the morphological structure of simulated galaxies. A spherical latent space allows the HiPSter module to provide explorative visualization using Hierarchical Progressive Surveys (HiPS) in the Aladin software. Here we present a machine-learning workflow covering all stages, from data collection to preprocessing, training, prediction, and final…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Computational Physics and Python Applications
