# Quasars with PV broad absorption in BOSS data release 9

## TL;DR

This study identifies PV broad absorption in a significant fraction of BAL quasars from SDSS-III/BOSS DR9, revealing large column densities and partial coverage in quasar outflows, which are crucial for understanding feedback in galaxy evolution.

## Contribution

It presents the first large-scale survey of PV absorption in BAL quasars, significantly increasing known detections and providing new insights into outflow properties and their prevalence.

## Key findings

- PV absorption detected in 3.0-6.2% of BAL quasars
- PV presence correlates with stronger CIV and SiIV absorption
- Many PV detections imply large column densities and partial coverage

## Abstract

Broad absorption lines (BALs) found in a significant fraction of quasar spectra identify high-velocity outflows that might be present in all quasars and could be a major factor in feedback to galaxy evolution. Understanding the nature of these flows requires further constraints on their physical properties, including their column densities, for which well-studied BALs, such as CIV 1548,1551, typically provide only a lower limit because of saturation effects. Low-abundance lines, such as PV 1118,1128, indicate large column densities, implying outflows more powerful than measurements of CIV alone would indicate. We search through a sample of 2694 BAL quasars from the SDSS-III/BOSS DR9 quasar catalog for such absorption, and we identify 81 `definite' and 86 `probable' detections of PV broad absorption, yielding a firm lower limit of 3.0-6.2% for the incidence of such absorption among BAL quasars. The PV-detected quasars tend to have stronger CIV and SiIV absorption, as well as a higher incidence of LoBAL absorption, than the overall BAL quasar population. Many of the PV-detected quasars have CIV troughs that do not reach zero intensity (at velocities where PV is detected), confirming that the outflow gas only partially covers the UV continuum source. PV appears significantly in a composite spectrum of non-PV-detected BAL quasars, indicating that PV absorption (and large column densities) are much more common than indicated by our search results. Our sample of PV detections significantly increases the number of known PV detections, providing opportunities for follow-up studies to better understand BAL outflow energetics.