The Last Eight-Billion Years of Intergalactic CIV Evolution
Kathy L. Cooksey (1), Christopher Thom (2), J. Xavier Prochaska (1,3),, and Hsiao-Wen Chen (2) ((1) UC Santa Cruz; (2) U Chicago; (3) UCO/Lick, Observatory)

TL;DR
This study analyzes the evolution of intergalactic CIV absorbers over the last eight billion years using HST UV spectra, revealing a steady increase in mass density since z=5.
Contribution
It provides the first low-redshift survey of CIV doublets with detailed statistical analysis, extending the understanding of intergalactic metal evolution.
Findings
CIV absorber density has not evolved significantly since z=5.
The mass density of CIV has increased steadily from z=5 to 0.
The power-law distribution of column densities is characterized with specific parameters.
Abstract
We surveyed the HST UV spectra of 49 low-redshift quasars for z < 1 CIV candidates, relying solely on the characteristic wavelength separation of the doublet. After consideration of the defining traits of CIV doublets (e.g., consistent line profiles, other associated transitions, etc.), we defined a sample of 38 definite (group G = 1) and five likely (G = 2) doublets with rest equivalent widths W_r for both lines detected at >= 3 sigma. We conducted Monte-Carlo completeness tests to measure the unblocked redshift (dz) and co-moving pathlength (dX) over which we were sensitive to CIV doublets of a range of equivalent widths and column densities. The absorber line density of (G = 1+2) doublets is dN/dX = 4.1+0.7/-0.6 for log N(C^+3) >= 13.2, and dN/dX has not evolved significantly since z = 5. The best-fit power-law to the G = 1 frequency distribution of column densities f(N(C^+3)) =…
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