Automated physical classification in the SDSS DR10. A catalogue of candidate Quasars
Massimo Brescia, Stefano Cavuoti, Giuseppe Longo

TL;DR
This paper demonstrates that machine learning, specifically MLPQNA, can effectively classify astronomical objects in SDSS DR10 using photometric data, producing a large catalog of candidate quasars with high accuracy.
Contribution
The study applies a neural network approach to classify SDSS objects photometrically, creating a comprehensive quasar candidate catalog with high efficiency and purity.
Findings
Achieved 91.31% overall classification efficiency.
Produced a catalog of approximately 3.6 million quasar candidates.
Demonstrated effectiveness of machine learning in photometric classification.
Abstract
We discuss whether modern machine learning methods can be used to characterize the physical nature of the large number of objects sampled by the modern multi-band digital surveys. In particular, we applied the MLPQNA (Multi Layer Perceptron with Quasi Newton Algorithm) method to the optical data of the Sloan Digital Sky Survey - Data Release 10, investigating whether photometric data alone suffice to disentangle different classes of objects as they are defined in the SDSS spectroscopic classification. We discuss three groups of classification problems: (i) the simultaneous classification of galaxies, quasars and stars; (ii) the separation of stars from quasars; (iii) the separation of galaxies with normal spectral energy distribution from those with peculiar spectra, such as starburst or starforming galaxies and AGN. While confirming the difficulty of disentangling AGN from normal…
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