TL;DR
This paper demonstrates that deep convolutional neural networks can accurately predict a galaxy's neutral hydrogen content from optical images, revealing morphology-gas content connections and environmental effects.
Contribution
It introduces a CNN-based method to estimate HI mass fraction from optical images, outperforming previous estimators and providing interpretability through Grad-CAM visualizations.
Findings
CNN accurately predicts HI mass fraction from optical images.
The morphology-HI connection is stable in low/intermediate-density environments.
The CNN outperforms previous estimators across multiple catalogs.
Abstract
A galaxy's morphological features encode details about its gas content, star formation history, and feedback processes, which play important roles in regulating its growth and evolution. We use deep convolutional neural networks (CNNs) to learn a galaxy's optical morphological information in order to estimate its neutral atomic hydrogen (HI) content directly from SDSS image cutouts. We are able to accurately predict a galaxy's logarithmic HI mass fraction, , by training a CNN on galaxies in the ALFALFA 40% sample. Using pattern recognition (PR), we remove galaxies with unreliable estimates. We test CNN predictions on the ALFALFA 100%, xGASS, and NIBLES catalogs, and find that the CNN consistently outperforms previous estimators. The HI-morphology connection learned by the CNN appears to be constant in low- to…
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