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Home All issues Volume 444 / No 2 (December III 2005) A&A, 444 2 (2005) 461-479 Abstract
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Issue
A&A
Volume 444, Number 2, December III 2005
Page(s) 461 - 479
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20041570


A&A 444, 461-479 (2005)
DOI: 10.1051/0004-6361:20041570

The dust obscuration bias in damped Lyman $\alpha$ systems

G. Vladilo1 and C. Péroux2

1  Osservatorio Astronomico di Trieste - Istituto Nazionale di Astrofisica, Via Tiepolo 11, 34131 Trieste, Italy
    e-mail: vladilo@ts.astro.it
2  European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching-bei-München, Germany
    e-mail: cperoux@eso.org

(Received 1 July 2004 / Accepted 4 October 2005)

Abstract
We present a new study of the effects of quasar obscuration on the statistics of Damped Ly $\alpha$ (DLA) systems. We show that the extinction of any Galactic or extragalactic $\ion{H}{i}$ region, $A_\lambda$, increases linearly with the column density of zinc, with a turning point $\partial A_\lambda / \partial (\log N_\mathrm{Zn}) =1$, above which background sources are suddenly obscured. We derive a relation $A_\lambda=A_\lambda(N_\mathrm{H},Z,z)$ between the extinction of a DLA system and its $\ion{H}{i}$ column density, NH, metallicity, Z, fraction of iron in dust, fFe(Z), and redshift, z. From this relation we estimate the fraction of DLA systems missed as a consequence of their own extinction in magnitude-limited surveys. We derive a method for recovering the true frequency distributions of NH and Z in DLAs, fNH and fZ, using the biased distributions measured in the redshift range where the observations have sufficient statistics ( $1.8 \leq z \leq 3$). By applying our method we find that the well-known empirical thresholds of DLA column densities, $N_\mathrm{Zn} \la 10^{13.1}$ atoms cm-2 and $N_\ion{H}{i} \la 10^{22}$ atoms cm-2, can be successfully explained in terms of the obscuration effect without tuning of the local dust parameters. The obscuration has a modest effect on the distribution of quasar apparent magnitudes, but plays an important role in shaping the statistical distributions of DLAs. The exact estimate of the bias is still limited by the paucity of the data ($\simeq$40 zinc measurements at $1.8 \leq z \leq 3$). We find that the fraction of DLAs missed as a consequence of obscuration is ~30% to 50%, consistent with the results of surveys of radio-selected quasars. By modelling the metallicity distribution with a Schechter function we find that the mean metallicity can be $\sim $5 to 6 times higher than the value commonly reported for DLAs at $z \sim 2.3$.


Key words: ISM: dust, extinction -- galaxies: ISM -- galaxies: high-redshift -- quasars: absorption lines

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