The CORALS Survey I: New Estimates of the Number Density and Gas Content of Damped Lyman Alpha Systems Free from Dust Bias

Abstract

(Abridged) We present the first results from the Complete Optical and Radio Absorption Line System (CORALS) survey. We have compiled a homogeneous sample of radio-selected QSOs from the Parkes Catalogue and searched for damped Lyman alpha systems (DLAs) towards every target, irrespective of its optical magnitude. This approach circumvents selection effects -- particularly from intervening dust -- which have long been suspected to affect DLA surveys in optically-selected, magnitude-limited QSO samples. The CORALS data set consists of 66 z_em > 2.2 QSOs in which 22 DLAs with absorption redshifts 1.8 < z_abs < z_em have been identified over a total redshift interval Delta z = 55.46. In this first paper of the CORALS series we describe the sample, present intermediate resolution spectroscopy and determine the population statistics of DLAs. We deduce a value of the neutral gas mass density traced by DLAs (expressed as a fraction of the closure density) log Omega_DLA h = -2.59^{+0.17}_{-0.24}, and a number density of DLAs per unit redshift n(z) = 0.31^{+0.09}_{-0.08}, both at a mean redshift <z> = 2.37. Taking into account the errors, we conclude that dust-induced bias in previous surveys may have led to an underestimate of these quantities by at most a factor of two and we have not uncovered a previously unrecognised population of high column density DLAs in front of faint QSOs.

25 pages, accepted for publication in A&A

References in corpus (2)

• Absorption Systems in the Spectra of 66 z > 4 Quasars
• UVES observations of a damped Ly-alpha system at z_abs = 4.466 towards the quasar APM BR J0307-4945

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