Metallicity evolution in quasars

Swayamtrupta Panda and Ewa Julia Skorek

Broad-band spectra of active galaxies contain a wide range of information that help reveal the nature and activity of the central continuum source and their immediate surroundings. Understanding the evolution of metals in the spectra of Active Galactic Nuclei (AGN) and linking them with the various fundamental black hole (BH) parameters, as for example, BH mass, the bolometric luminosity of the source, or its accreting power, can help address their connection to the growth of the BH across cosmic time. We investigate the role of selected metallicity indicators utilizing the rich spectroscopic database of emission lines covering a wide range in redshift in the recent spectroscopic data release of Sloan Digital Sky Survey (SDSS). We make careful filtering of the parent sample to prepare a pair of high-quality, redshift-dependent sub-samples and present the first results of the analysis here. To validate our findings from the simple correlations, we execute and evaluate the performance of a linear dimensionality reduction technique - principal component analysis (PCA), over our sub-samples. We also present the projection maps highlighting the primary drivers of the observed correlations. The projection maps also allow us to isolate peculiar sources of potential interest.

Proceedings of the Polish Astronomical Society, vol. 12, 72-75 (2022)

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