2005MNRAS.364..319B

At redshifts larger than 2, a large fraction (80 per cent) of the metals is apparently as yet undetected. We use a sample of submillimetre-selected galaxies (SMGs) with molecular gas and dynamical mass measurements from the literature in order to put constraints on the contribution of such galaxies to the total metal budget. Compared with Lyman break galaxies (LBGs), for example, SMGs are rarer (by a factor of 10 or more), but contain much more gas and are more metal-rich. We estimate that SMGs brighter than 3mJy contain only ≲9 per cent of the metals, when we combine the observed dynamical masses (<M_dyn>∼ fewx10¹¹M_☉), number density (n≃ 10^–4/Mpc3), observed gas metallicity (Z≃ 1-2Z_☉), and observed gas fractions (f_gas~ 40 per cent), assuming a molecular to neutral hydrogen ratio of 1. Including SMGs fainter than 3mJy, we estimate that SMGs contain about ≤15 per cent of the metals, where our incompleteness correction is estimated from the dust mass function. Our results are strong upper limits, given that high gas fractions and high overall metallicity are mutually exclusive. In summary, SMGs make a significant contribution to the metal budget (≲15 per cent) but not sufficient to solve the `missing metal problem'. A consequence of our results is that SMGs can only add ~3.5 per cent to Ω_DLA, and cannot be the source of a significant population of dusty DLAs.