Convolutional Neural Networks for classifying galaxy mergers: Can faint tidal features aid in classifying mergers?
Yeonkyung Lee, Hyunmi Song, Jihye Shin, Sungryong Hong, Jaehyun Lee, Kyungwon Chun

TL;DR
This study evaluates the effectiveness of convolutional neural networks in classifying galaxy mergers using deep, LSST-like images, highlighting the importance of faint tidal features for improved accuracy.
Contribution
It demonstrates that CNNs can distinguish galaxy mergers from non-mergers with improved accuracy when faint tidal features are included in the images.
Findings
CNN achieved 67-70% accuracy with faint features
Including faint tidal features improved classification accuracy by ~5%
Faint tidal features are effective indicators for merger classification
Abstract
Identifying mergers from observational data has been a crucial aspect of studying galaxy evolution and formation. Tidal features, typically fainter than 26 , exhibit a diverse range of appearances depending on the merger characteristics and are expected to be investigated in greater detail with the Rubin Observatory Large Synoptic Survey Telescope (LSST), which will reveal the low surface brightness universe with unprecedented precision. Our goal is to assess the feasibility of developing a convolutional neural network (CNN) that can distinguish between mergers and non-mergers based on LSST-like deep images. To this end, we used Illustris TNG50, one of the highest-resolution cosmological hydrodynamic simulations to date, allowing us to generate LSST-like mock images with a depth 29 for low-redshift () galaxies, with…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
