The SCUBA 8-mJy survey – II. Multiwavelength analysis of bright submillimetre sources

We present the results of a multiwavelength study of the 19 most significant submillimetre (submm) sources detected in the SCUBA 8-mJy survey. As described in Scott et al. , this survey covers ≃260 arcmin² using the submillimetre camera SCUBA, to a limiting source detection limit   S _850 μm≃8 mJy  . One advantage of this relatively bright flux-density limit is that accurate astrometric positions are potentially achievable for every source using existing radio and/or millimetre-wave interferometers. However, an associated advantage is that spectral energy distribution (SED) based redshift constraints should be more powerful than in fainter submm surveys. Here we therefore exploit the parallel SCUBA 450-μm data, in combination with existing radio and Infrared Space Observatory ( ISO ) data at longer and shorter wavelengths to set constraints on the redshift of each source. We also analyse new and existing optical and near-infrared imaging of our SCUBA survey fields to select potential identifications consistent with these constraints. Our derived SED-based redshift constraints, and the lack of statistically significant associations with even moderately bright galaxies allow us to conclude that all 19 sources lie at   z >1  , and at least half of them apparently lie at   z >2  .     

Late Devensian evolution of the marine offshore environment of western Scotland

Offshore boreholes from the outer Firth of Clyde and from the Sea of the Hebrides passed through marine deposits of Holocene, Loch Lomond Stadial (LLS) and Windermere Interstadial (WI) age, but it is likely that older, probably Dimlington Stadial (DS) strata, now removed by erosion, were formerly present at the entrance to the Firth of Clyde. The late-glacial environment was one of very rapid deposition punctuated by erosive episodes. Reworking and redeposition led to the mixing of otherwise incompatible warm, shallow-water and cold, offshore faunas, particularly during a ‘warm’ event towards the end of the WI. The latter is correlated with Greenland Interstadial GI1a, but no evidence has been found for climatic ameliorations corresponding to GI1c and GI1e earlier in the Wl. A less cold interval at the end of the LLS may be coeval with climatic changes in Norway and the Shetland–Faroe Channel. Glacier ice disappeared from the outer Firth of Clyde before the close of the DS, and the Glasgow area was deglaciated across the DS/WI transition. The borehole evidence for the timing of deglaciation in the Sea of the Hebrides is inconclusive.     

Multilevel samplers as microcosms to assess microbial response to biostimulation

Passive multilevel samplers (MLS) containing a solid matrix for microbial colonization were used as in situ microcosms in conjunction with a push-pull biostimulation experiment designed to promote biological U(VI) and Tc(VII) reduction. MLS were deployed at 24 elevations in the injection well and two downgradient wells to investigate the spatial variability in microbial community composition and growth prior to and following biostimulation. The microbial community was characterized by real-time quantitative polymerase chain reaction (Q-PCR) quantification of bacteria, NO(3)(-)-reducing bacteria (nirS and nirK), delta-proteobacteria, Geobacter sp., and methanogens (mcrA). Pretest cell densities were low overall but varied substantially with significantly greater bacterial populations detected at circumneutral pH (t-test, alpha= 0.05), suggesting carbon substrate and low pH limitations of microbial activity. Although pretest cell densities were low, denitrifying bacteria were dominant members of the microbial community. Biostimulation with an ethanol-amended ground water resulted in concurrent NO(3)(-) and Tc(VII) reduction, followed by U(VI) reduction. Q-PCR analysis of MLS revealed significant (1 to 2 orders of magnitude, Mann-Whitney U-test, alpha= 0.05) increases in cell densities of bacteria, denitrifiers, delta-proteobacteria, Geobacter sp., and methanogens in response to biostimulation. Traditionally, characterization of sediment samples has been used to investigate the microbial community response to biostimulation; however, collection of sediment samples is expensive and not conducive to deep aquifers or temporal studies. The results presented demonstrate that push-pull tests with passive MLS provide an inexpensive approach to determine the effect of biostimulation on contaminant concentrations, geochemical conditions, and the microbial community composition and function.     

Floodplain construction by recent,rapid vertical accretion: Waipaoa River,New Zealand

The rate of vertical accretion (typically 14–18 mm h⁻¹) during eight floods in the Waipaoa River basin, with recurrence intervals of 5 to 60 years, was determined by relating the floodplain stratigraphy at McPhail's bend to the 1948–1995 flood history. Overbank deposits remaining after a flood that occurred in March 1996 suggest a rate of vertical accretion of 15 mm h⁻¹. By contrast, because the flow velocity across the floodplain was too high to permit deposition from suspension, during the record flood of March 1988 the rate of vertical accretion was only 6 mm h⁻¹. The sequence of deposition is highly discontinuous, and the rapid vertical accretion is a response to a late 19th to early 20th century phase of deforestation in the headwaters that probably initiated a far greater change in suspended sediment yield than in discharge. Cross-section surveys conducted since 1948 indicate that the high suspended sediment load of the Waipaoa River also promoted in-channel deposition, which effected a progressive reduction in bankfull channel width although, due to the overbank deposition, channel capacity remained constant. © 1998 John Wiley & Sons, Ltd.     

The spectrum of multiply ionized iron between 10 and 17 Å

Valency and inner shell transitions in multiply ionized iron have been excited in the transient pinch of a Plasma Focus discharge. Hartree-Fock calculations have been made to identify the levels involved and a comparison is made with observations of solar flares.