Estimating Cluster Masses from SDSS Multi-band Images with Transfer Learning
Sheng-Chieh Lin, Yuanyuan Su, Gongbo Liang, Yuanyuan Zhang, Nathan, Jacobs, Yu Zhang

TL;DR
This paper introduces a transfer-learning deep neural network approach to estimate galaxy cluster masses from SDSS images, achieving accuracy comparable to existing methods and demonstrating the potential of deep learning for large-scale astrophysical surveys.
Contribution
The paper presents a novel semi-supervised transfer-learning model that estimates cluster masses from SDSS images using real observational data, improving accuracy and interpretability.
Findings
Achieved a mean absolute error of 0.232 dex in mass estimation
Performance comparable to redMaPPer with 0.192 dex error
Demonstrated interpretability with gradient and activation mapping
Abstract
The total masses of galaxy clusters characterize many aspects of astrophysics and the underlying cosmology. It is crucial to obtain reliable and accurate mass estimates for numerous galaxy clusters over a wide range of redshifts and mass scales. We present a transfer-learning approach to estimate cluster masses using the ugriz-band images in the SDSS Data Release 12. The target masses are derived from X-ray or SZ measurements that are only available for a small subset of the clusters. We designed a semi-supervised deep learning model consisting of two convolutional neural networks. In the first network, a feature extractor is trained to classify the SDSS photometric bands. The second network takes the previously trained features as inputs to estimate their total masses. The training and testing processes in this work depend purely on real observational data. Our algorithm reaches a mean…
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