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Constructing Impactful Machine Learning Research for Astronomy: Best Practices for Researchers and Reviewers

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arxiv 2310.12528 v1 pith:BPISL74H submitted 2023-10-19 astro-ph.IM cs.LG

classification astro-ph.IMcs.LG
keywords learningmachineresultsastronomicalbestcommunitymethodpractices
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Machine learning has rapidly become a tool of choice for the astronomical community. It is being applied across a wide range of wavelengths and problems, from the classification of transients to neural network emulators of cosmological simulations, and is shifting paradigms about how we generate and report scientific results. At the same time, this class of method comes with its own set of best practices, challenges, and drawbacks, which, at present, are often reported on incompletely in the astrophysical literature. With this paper, we aim to provide a primer to the astronomical community, including authors, reviewers, and editors, on how to implement machine learning models and report their results in a way that ensures the accuracy of the results, reproducibility of the findings, and usefulness of the method.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars

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    Galactic OB-star HR-diagram data imply a constant core overshoot α_ov ≈ 0.33 for 12–40 M_sun, yielding larger helium cores than standard prescriptions.

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    cs.AI 2025-07 conditional novelty 6.0 of 10

    A multi-agent LLM system with a Planning & Control strategy performs an autonomous Union2.1 cosmology fit and beats single-LLM baselines on a 50-problem DS-1000 subset.

  3. The ATLAS Virtual Research Assistant

    astro-ph.IM 2025-06 conditional novelty 6.0 of 10

    A gradient-boosted tree pair scoring alerts as real and extragalactic reduces ATLAS eyeballing workload by 85% with a measured potential follow-up loss below 0.08%.

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