# Ionization driven intrinsic absorption line variability of BAL quasars   in the Stripe 82 region

**Authors:** M. Vivek

arXiv: 1904.02149 · 2019-04-10

## TL;DR

This study examines how intrinsic C IV absorption line variability in BAL quasars correlates with continuum flux changes, revealing that saturation effects influence the strength of this correlation.

## Contribution

It provides the first detailed analysis of the connection between absorption line variability and continuum flux changes in BAL quasars using multi-epoch SDSS and CRTS data.

## Key findings

- Weak correlation (ρ ~ 0.3) overall between absorption and continuum variability.
- Stronger correlation (ρ ~ 0.5) in high-SNR samples.
- Even stronger correlation (ρ ~ 0.6) in shallow trough sub-set.

## Abstract

We investigate the connection between the intrinsic C IV absorption line variability and the continuum flux changes of broad absorption line (BAL) quasars using a sample of 78 sources in the Stripe 82 region. The absorption trough variability parameters are measured using the archival multi-epoch spectroscopic data from the Sloan Digital Sky Survey (SDSS), and the continuum flux variability parameters are estimated from the photometric light curves obtained by the SDSS and the Catalina Real-Time Survey (CRTS) surveys. We find evidence for weak correlations (\rho ~ 0.3) between the intrinsic C IV absorption line variability and the quasar continuum variability for the final sample of 78 BAL quasars. The correlation strengths improve (\rho ~0.5) for the "high-SNR" sample sources that have higher spectral signal-to-noise ratio. Using two sub-sets of the high-SNR sample differing on the absorption trough depth, we find that the shallow trough sub-set shows an even stronger correlation (\rho ~ 0.6), whereas the deep trough sub-set does not show any correlation between the absorption line variability and the continuum variability. These results point to the important role of saturation effects in the correlation between the absorption line variability and the continuum variability of BAL quasars. Considering other effects that can also smear the correlation, we conclude that the actual correlation between the absorption line and continuum variability is even stronger.

## Full text

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## Figures

30 figures with captions in the complete paper: https://tomesphere.com/paper/1904.02149/full.md

## References

76 references — full list in the complete paper: https://tomesphere.com/paper/1904.02149/full.md

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Source: https://tomesphere.com/paper/1904.02149