Berg, T. A. M.T. A. M.BergEllison, S. L.S. L.EllisonProchaska, J. X.J. X.ProchaskaSánchez-Ramírez, R.R.Sánchez-RamírezLopez, S.S.LopezD'ODORICO, ValentinaValentinaD'ODORICOBecker, G.G.BeckerChristensen, L.L.ChristensenCUPANI, GuidoGuidoCUPANIDenney, K.K.DenneyWorseck, G.G.Worseck2020-12-232020-12-2320170035-8711http://hdl.handle.net/20.500.12386/29184The XQ-100 survey provides optical and near-infrared coverage of 36 blindly selected, intervening damped Lyman α systems (DLAs) at 2 < z<SUB>abs</SUB> < 4, simultaneously covering the Mg II doublet at λλ2796, 2803Å, and the Ly α transition. Using the XQ-100 DLA sample, we investigate the completeness of selecting DLA absorbers based on their Mg II rest-frame equivalent width (W<SUB>0</SUB>^{2796}) at these redshifts. Of the 29 DLAs with clean Mg II profiles, we find that six (20 per cent of DLAs) have W<SUB>0</SUB>^{2796} < 0.6 Å. The DLA incidence rate of W<SUB>0</SUB>^{2796} < 0.6 Å absorbers is a factor of ∼5 higher than what is seen in z ∼ 1 samples, indicating a potential evolution in the Mg II properties of DLAs with redshift. All of the W<SUB>0</SUB>^{2796} < 0.6 Å DLAs have low metallicities (-2.5 < [M/H] < -1.7), small velocity widths (v<SUB>90</SUB> < 50 km s<SUP>-1</SUP>), and tend to have relatively low N(H I). We demonstrate that the exclusion of these low W<SUB>0</SUB>^{2796} DLAs results in a higher mean N(H I) which in turn leads to an ∼7 per cent increase in the cosmological gas density of H I of DLAs at 2 < z<SUB>abs</SUB> < 4; and that this exclusion has a minimal effect on the H I-weighted mean metallicity.STAMPAenArticle10.1093/mnrasl/slw1852-s2.0-85022201432000403097500012https://academic.oup.com/mnrasl/article/464/1/L56/28910032017MNRAS.464L..56BFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_8 Formation and evolution of galaxies