Insights into Quasar UV Spectra Using Unsupervised Clustering Analysis
Aycha Tammour, Sarah C. Gallagher, Mark Daley (U. of Western Ontario),, Gordon T. Richards (Drexel U.)

TL;DR
This study applies K-means clustering to quasar UV spectra from SDSS to identify natural groupings, revealing known correlations and offering insights into quasar physical conditions through unsupervised machine learning.
Contribution
The paper demonstrates the effectiveness of unsupervised clustering in analyzing quasar spectra, uncovering known correlations and providing a new approach for spectral data analysis.
Findings
Recovered known UV spectral correlations
Identified clusters based on C III] properties
Showed clustering effectiveness in spectral analysis
Abstract
Machine learning can provide powerful tools to detect patterns in multi-dimensional parameter space. We use K-means -a simple yet powerful unsupervised clustering algorithm which picks out structure in unlabeled data- to study a sample of quasar UV spectra from the Quasar Catalog of the 10th Data Release of the Sloan Digital Sky Survey of Paris et al. (2014). Detecting patterns in large datasets helps us gain insights into the physical conditions and processes giving rise to the observed properties of quasars. We use K-means to find clusters in the parameter space of the equivalent width (EW), the blue- and red-half-width at half-maximum (HWHM) of the Mg II 2800 A line, the C IV 1549 A line, and the C III] 1908 A blend in samples of Broad Absorption-Line (BAL) and non-BAL quasars at redshift 1.6-2.1. Using this method, we successfully recover correlations well-known in the UV regime…
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