Damped Lyα Systems at z<1.65: The Expanded Sloan Digital Sky Survey Hubble Space Telescope Sample
Turnshek, David A.; Rao, Sandhya M.; Nestor, Daniel B.
United States
Abstract
We present results of our Hubble Space Telescope Cycle 11 survey for low-redshift (z<1.65) damped Lyα (DLA) systems in the UV spectra of quasars selected from the Sloan Digital Sky Survey (SDSS) Early Data Release. These quasars have strong intervening Mg II-Fe II systems that are known signatures of high column density neutral gas. In total, including our previous surveys, UV observations of Lyα absorption in 197 Mg II systems with z<1.65 and rest equivalent width (REW) Wλ27960>=0.3 Å have now been obtained. The main results are as follows: (1) The success rate of identifying DLAs in a Mg II sample with Wλ27960>=0.5 Å and Fe II Wλ26000>=0.5 Å is 36%+/-6% and increases to 42%+/-7% for systems with Wλ27960/Wλ26000<2 and Mg I Wλ28520>0.1 Å. (2) The mean H I column density of Mg II systems with 0.3 Å<=Wλ27960<0.6 Å is =(9.7+/-2.2)×1018 cm-2. For the larger REW systems in our sample, =(3.5+/-0.7)×1020 cm-2. (3) The DLA incidence per unit redshift for 0<z<5 is nDLA(z)=n0(1+z)γ, where n0=0.044+/-0.005 and γ=1.27+/-0.11. This parameterization is consistent with no evolution for z<~2 (ΩΛ=0.7, ΩM=0.3) but exhibits significant evolution for z>~2. (4) The cosmological neutral gas mass density due to DLAs is constant in the redshift interval 0.5<z<5.0 to within the uncertainties, ΩDLA~1×10-3. This is larger than Ωgas(z=0) by a factor of ~2. (5) The slope of the H I column density distribution does not change significantly with redshift. However, the low-redshift distribution is marginally flatter due to the higher fraction of high column density systems in our sample. (6) Finally, using the precision of Mg II survey statistics, we show that under the assumption of constant DLA fraction and H I column density suggested by our current sample, there may be evidence of a decreasing ΩDLA from z=0.5 to 0.
Based on data obtained from the Sloan Digital Sky Survey (SDSS) and on observations made with the Hubble Space Telescope (HST) operated by STScI-AURA for NASA.