Abstract
We study the average absorption spectrum of the Damped Lyman Alpha system
(DLA) population at $z ~ 2.5$ by stacking normalized, rest-frame shifted
spectra of $27\,000$ DLAs from the Data Release 12 of the BOSS survey of
SDSS-III. We list measurements of the mean equivalent width of 50 individual
metal absorption lines in 5 intervals of DLA hydrogen column density $N_\rm
HI$, and overall mean equivalent widths for an additional 13 absorption
features from groups of strongly blended lines. We show that the mean
equivalent width of low-ionization lines increases with $N_HI$ as
expected, but this increase is much weaker or non-existent for high-ionization
lines. We develop a theoretical model to infer mean column densities from the
equivalent widths of partially saturated lines, based on the presence of
multiple absorption components observed in high-resolution spectra. We use this
model to infer mean column densities in DLAs of 14 low-ionization species, as
well as for AlIII, SIII, SiIII, CIV, SiIV, NV and OVI. In addition, we use an
approximate derivation for separating the contributions of several lines to
blended absorption features, and infer mean equivalent widths and column
densities from lines of the additional species NI, ZnII, CII$^*$, FeIII,
and SIV. These measurements do not suffer from the superposition of the Lyman
forests, owing to the large number of DLAs that are stacked. Several of these
mean column densities of metal lines in DLAs are obtained for the first time;
their values generally agree with measurements of individual DLAs from
high-resolution, high signal-to-noise ratio spectra when they are available.
Description
[1610.02711] The Mean Metal-line Absorption Spectrum of Damped Lyman Alpha Systems in BOSS
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