Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-05-23
Astron.J.120:1175,2000
Astronomy and Astrophysics
Astrophysics
Accepted for publication by AJ. 10 pages of text plus 11 figures and 2 tables
Scientific paper
10.1086/301511
We have obtained an exceptionally high S/N, high resolution spectrum of the gravitationally lensed quasar Q1422+231 in order to investigate the metal enrichment of the IGM. A column density distribution function (CDDF) is determined for CIV, which is well fit by a power law with index 1.44 +/- 0.05. Once a correction for incompleteness is applied, we find that the CDDF is consistent with a power law down to log N(CIV) = 11.75, a factor of 10 more sensitive than previously determined. In order to determine whether the CIV enrichment extends to even lower column density HI clouds, we find that an analysis of individual pixel optical depths is more robust than the stacking technique. The results obtained from this optical depth method are compared with analyses of simulated spectra enriched with varying CIV enrichment recipes. From these simulations, we conclude that more CIV than is currently directly detected in Q1422+231 is required to reproduce the optical depths determined from the data, consistent with the conclusions drawn from consideration of the power law distribution. (Abridged)
Ellison Sara L.
Pettini Max
Schaye Joop
Songaila Antoinette
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