Semi-supervised Spectral Classification of DESI White Dwarfs by Dimensionality Reduction
Xander Byrne, Amy Bonsor, Laura K. Rogers, Christopher J. Manser

TL;DR
This paper demonstrates how dimensionality reduction can effectively classify and visualize white dwarf spectra in large spectroscopic surveys, identifying features missed by visual inspection and enabling rapid, low-contamination sample selection.
Contribution
It introduces a semi-supervised spectral classification method using dimensionality reduction to analyze large spectroscopic datasets like DESI, improving classification accuracy and efficiency.
Findings
Successfully separates white dwarf spectral classes in DESI data
Achieves 90% recall for helium features and 100% for cataclysmic variables
Enables rapid, low-contamination sample selection from large datasets
Abstract
As a new generation of large-sky spectroscopic surveys comes online, the enormous data volume poses unprecedented challenges in classifying spectra. Modern unsupervised techniques have the power to group spectra based on their dominant features, circumventing the complete reliance on training data suffered by supervised methods. We outline the use of dimensionality reduction to generate a 2D map of the structure of an intermediate-resolution spectroscopic dataset. This technique efficiently separates white dwarfs of different spectral classes in the Dark Energy Spectroscopic Instrument's Early Data Release (DESI EDR), identifying spectral features that had been missed even by visual classification. By focusing the method on particular spectral regions, we identify white dwarfs with helium features at 90 per cent recall, and cataclysmic variables at 100 per cent recall, illustrating…
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Taxonomy
TopicsInfrared Target Detection Methodologies · Astronomy and Astrophysical Research · Optical Systems and Laser Technology
