AstroMAE: Redshift Prediction Using a Masked Autoencoder with a Novel Fine-Tuning Architecture
Amirreza Dolatpour Fathkouhi, Geoffrey Charles Fox

TL;DR
AstroMAE introduces a novel masked autoencoder approach with a specialized fine-tuning architecture for redshift prediction, leveraging unlabeled SDSS images to improve accuracy and generalization in astronomical data analysis.
Contribution
This paper presents the first application of masked autoencoders to astronomical data, enhancing redshift prediction through pretraining on unlabeled images and a new fine-tuning architecture.
Findings
AstroMAE outperforms traditional CNN and vision transformer models.
Pretraining with masked autoencoders improves data understanding without labels.
The approach achieves superior accuracy in redshift prediction tasks.
Abstract
Redshift prediction is a fundamental task in astronomy, essential for understanding the expansion of the universe and determining the distances of astronomical objects. Accurate redshift prediction plays a crucial role in advancing our knowledge of the cosmos. Machine learning (ML) methods, renowned for their precision and speed, offer promising solutions for this complex task. However, traditional ML algorithms heavily depend on labeled data and task-specific feature extraction. To overcome these limitations, we introduce AstroMAE, an innovative approach that pretrains a vision transformer encoder using a masked autoencoder method on Sloan Digital Sky Survey (SDSS) images. This technique enables the encoder to capture the global patterns within the data without relying on labels. To the best of our knowledge, AstroMAE represents the first application of a masked autoencoder to…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Calibration and Measurement Techniques · Statistical and numerical algorithms
MethodsAttention Is All You Need · Softmax · Layer Normalization · Linear Layer · Dense Connections · Residual Connection · Multi-Head Attention · Vision Transformer
