Using Machine Learning to Identify Extragalactic Globular Cluster Candidates from Ground-Based Photometric Surveys of M87
Emilia Barbisan, Jeff Huang, Kristen C. Dage, Daryl Haggard, Robin, Arnason, Arash Bahramian, William I. Clarkson, Arunav Kundu, Stephen E. Zepf

TL;DR
This study applies supervised machine learning algorithms, specifically random forests and neural networks, to identify globular clusters in M87 from ground-based photometry, demonstrating high accuracy and potential for future large-scale surveys.
Contribution
The paper introduces the use of ML classification methods to identify extragalactic GCs from ground-based data, comparing their performance to human classifications and previous studies.
Findings
Random forest reselects 61.2% of HST GCs
Neural networks reselect 95.0% of HST GCs
ML methods show promise for upcoming large surveys
Abstract
Globular clusters (GCs) have been at the heart of many longstanding questions in many sub-fields of astronomy and, as such, systematic identification of GCs in external galaxies has immense impacts. In this study, we take advantage of M87's well-studied GC system to implement supervised machine learning (ML) classification algorithms - specifically random forest and neural networks - to identify GCs from foreground stars and background galaxies using ground-based photometry from the Canada-France-Hawai'i Telescope (CFHT). We compare these two ML classification methods to studies of "human-selected" GCs and find that the best performing random forest model can reselect 61.2% 8.0% of GCs selected from HST data (ACSVCS) and the best performing neural network model reselects 95.0% 3.4%. When compared to human-classified GCs and contaminants selected from CFHT data - independent…
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