${session.getAttribute("locale")} 5 Report by the ARPANSA Radiofrequency Expert Panel on review of radiofrequency health effects research: Scientific literature 2000 – 2012 Wed 16 Apr 2014 17:14:10 EST ]]> The role of metallurgical solid state phase transformations on the formation of residual stress in laser cladding and heating Wed 16 Apr 2014 15:43:12 EST ]]> Utilization and efficacy of internet-based eHealth technology in gastroenterology: a systematic review Wed 16 Apr 2014 15:15:08 EST ]]> Genetic variations in dopamine and inhibitory control: lack of influence on action restraint Wed 16 Apr 2014 14:55:36 EST ]]> For want of industry policy, our living standards are set to fall Wed 16 Apr 2014 14:47:13 EST ]]> For want of industry policy, our living standards are set to fall Wed 16 Apr 2014 14:47:12 EST ]]> Hubble Space Telescope spectra of the Type Ia supernova SN 2011fe: A tail of low-density, high-velocity material with Z<Zsolar Wed 16 Apr 2014 14:31:49 EST ]]> The thematic structure of passenger comfort experience and its relationship to the context features in the aircraft cabin Wed 16 Apr 2014 14:26:12 EST ]]> Cue-utilisation typologies and pilots' pre-flight and in-flight weather decision-making Wed 16 Apr 2014 14:26:11 EST ]]> The social economy in Australia: a research agenda Wed 16 Apr 2014 14:12:09 EST ]]> Modelling how much extra motorists pay on the road? A cross-sectional study of profit margins of unleaded petrol in Australia Wed 16 Apr 2014 13:58:09 EST ]]> Swarm planning: the development of a planning methodology to deal with climate adaptation Wed 16 Apr 2014 13:58:07 EST ]]> Sustained brain activation supporting stop-signal task performance Wed 16 Apr 2014 13:51:09 EST ]]> Mental fatigue effects on physical performance during running Wed 16 Apr 2014 13:44:08 EST ]]> As above, so below Wed 16 Apr 2014 13:23:09 EST ]]> Truth, justice and the American way Wed 16 Apr 2014 13:16:10 EST ]]> Clinical management of stalkers and stalking behaviors Wed 16 Apr 2014 12:41:08 EST ]]> Classification of stalkers Wed 16 Apr 2014 12:41:08 EST ]]> A guide to what works for depression in young people Wed 16 Apr 2014 12:34:08 EST ]]> Galaxy And Mass Assembly (GAMA): ugrizYJHK Sersic luminosity functions and the cosmic spectral energy distribution by Hubble type Wed 16 Apr 2014 10:51:23 EST ]]> Knowledge-based approaches in software documentation: A systematic literature review Wed 16 Apr 2014 10:31:14 EST ]]> Enhancing a search for traditional medicinal plants with anthelmintic action by using wild type and stress reporter Caenorhabditis elegans strains as screening tools Wed 16 Apr 2014 10:27:01 EST ]]> Spectroscopic confirmation of DES12C3a Wed 16 Apr 2014 10:21:21 EST ]]> 100 million years after the Big Bang Wed 16 Apr 2014 10:21:19 EST ]]> Maximum-likelihood fitting of the 6dFGS peculiar velocities Wed 16 Apr 2014 10:21:18 EST ]]> The Virgo Cluster Wed 16 Apr 2014 10:21:15 EST ]]> Cepheids in the Coma Cluster Wed 16 Apr 2014 10:21:13 EST ]]> The 6dFGS peculiar velocity field Wed 16 Apr 2014 10:21:11 EST ]]> A fair game for all? How community sports clubs in Australia deal with diversity Wed 16 Apr 2014 10:21:03 EST ]]> Molecular dynamics study of nanoconfined water flow driven by rotating electric fields under realistic experimental conditions Wed 16 Apr 2014 10:07:32 EST ]]> Lipid oxidation volatiles absent in milk after selected ultrasound processing Wed 16 Apr 2014 10:07:31 EST ]]> The colour of the dark side of the Moon Wed 16 Apr 2014 10:07:29 EST ]]> The thematic structure of passenger comfort experience and its relationship to the context features in the aircraft cabin Wed 16 Apr 2014 10:07:28 EST ]]> Isolating quantum coherence using coherent multi-dimensional spectroscopy with spectrally shaped pulses Wed 16 Apr 2014 10:07:26 EST ]]> Automatic analysis of corporate sustainability reports and intelligent scoring Wed 16 Apr 2014 10:07:23 EST ]]> The power of social television: Can social media build viewer engagement? A new approach to brain imaging of viewer immersion Wed 16 Apr 2014 10:07:22 EST ]]> One-dimensional modelling of upper ocean mixing by turbulence due to wave orbital motion Wed 16 Apr 2014 10:07:20 EST ]]> Robust Sliding Mode-Based Learning Control for Steer-by-Wire Systems in Modern Vehicles Wed 16 Apr 2014 10:07:16 EST ]]> Integration of carbon risks and opportunities in enterprise risk management systems: evidence from Australian firms Wed 16 Apr 2014 10:07:13 EST ]]> Driving during alcohol hangover among Dutch professional truck drivers Wed 16 Apr 2014 10:07:12 EST ]]> Development of thermal-electrochemical model for lithium ion 18650 battery packs in electric vehicles Wed 16 Apr 2014 08:57:16 EST ]]> A new lightweight and high performance AES S-box using modular design Wed 16 Apr 2014 08:57:12 EST ]]> The Australian academic profession in transition. An alternative futures interpretation Wed 16 Apr 2014 08:57:12 EST ]]> V4 LEAD: A comparative study of leadership excellence and ethics in Central Eastern Europe Tue 15 Apr 2014 18:50:11 EST ]]> GROW: Fundraising for social good - how to upskill, empower, and support your volunteers to raise money for your organisation [workshop] Tue 15 Apr 2014 17:04:21 EST ]]> Fundraising: professional development pathways [panel discussion] Tue 15 Apr 2014 16:48:57 EST ]]> Does retail petrol price respond asymmetrically to changes in its cost? Tue 15 Apr 2014 16:05:24 EST ]]> Concept to devices: from plasmonic light trapping to upscaled plasmonic solar modules [Invited] Tue 15 Apr 2014 15:34:09 EST ]]> Merging theory and practice through artefact and exegesis Tue 15 Apr 2014 14:52:10 EST ]]> Instruction/Poem Tue 15 Apr 2014 14:52:09 EST ]]> The effect of environmental uncertainty and risk on entry mode choice: an empirical examination of Australian organisations Tue 15 Apr 2014 14:41:14 EST ]]> Festivals as a celebration of Place: a case study of the Coranderrk Aboriginal Festival Tue 15 Apr 2014 14:24:10 EST ]]> Controversial new sciences in the media: content analysis of global reporting of nanotechnology during the last decade Tue 15 Apr 2014 14:17:09 EST ]]> Writing to affect change: creative writing courses in Australia Tue 15 Apr 2014 13:42:09 EST ]]> 'Inspired by Business': a case of mentoring among disadvantaged first year students Tue 15 Apr 2014 12:32:14 EST ]]> Emergency expatriate evacuation: literature and research Tue 15 Apr 2014 12:32:14 EST ]]> Three-dimensional parallel recording with a Debye diffraction-limited and aberration-free volumetric multifocal array Tue 15 Apr 2014 12:32:13 EST ]]> To thine own self be true? Authenticity among banking CEOs Tue 15 Apr 2014 12:32:12 EST ]]> Embodying ethics: the visual representation of banking CEOs Tue 15 Apr 2014 12:32:10 EST ]]> Human resources and expatriate evacuation: a conceptual model Tue 15 Apr 2014 12:32:10 EST ]]> Swarm planning for climate change: an alternative pathway for resilience Tue 15 Apr 2014 12:18:12 EST ]]> Dutch and Australian planning regimes: are they ready to face extreme climate impacts? Tue 15 Apr 2014 12:18:11 EST ]]> Towards a spatial planning framework for climate adaptation Tue 15 Apr 2014 12:18:10 EST ]]> Hotspot: climate-proof Groningen: final report Tue 15 Apr 2014 12:18:10 EST ]]> Artist with a cameraphone: a decade of mobile photography Tue 15 Apr 2014 11:57:12 EST ]]> Code: the Exhibition Tue 15 Apr 2014 11:57:11 EST ]]> On the connection between the intergalactic medium and galaxies: the H i–galaxy cross-correlation at z ≲ 1 50 per cent of ‘weak’ H i systems reside within galaxy voids (hence not correlated with galaxies), and are confined in dark matter haloes of masses smaller than those hosting ‘strong’ systems and/or galaxies. We speculate that H i systems within galaxy voids might still be evolving in the linear regime even at scales ≲2 Mpc.]]> Thu 17 Apr 2014 16:13:06 EST ]]> Large-scale structure in absorption: gas within and around galaxy voids 99 per cent confidence level, c.l.) of Lyα systems at the edges of galaxy voids with respect to a random distribution, on ∼5 h-1 Mpc scales. We find no significant difference in the number of systems inside voids with respect to the random expectation. We report differences between both column density (inline image) and Doppler parameter (inline image) distributions of Lyα systems found inside and at the edge of galaxy voids at the ≳98 and ≳90 per cent c.l., respectively. Low-density environments (voids) have smaller values for both inline image and inline image than higher density ones (edges of voids). These trends are theoretically expected and also found in Galaxies-Intergalactic Medium Interaction Calculation (GIMIC), a state-of-the-art hydrodynamical simulation. Our findings are consistent with a scenario of at least three types of Lyα systems: (1) containing embedded galaxies and so directly correlated with galaxies (referred to as 'halo-like'), (2) correlated with galaxies only because they lie in the same overdense large-scale structure (LSS) and (3) associated with underdense LSS with a very low autocorrelation amplitude (≈random) that are not correlated with luminous galaxies. We argue that the latter arise in structures still growing linearly from the primordial density fluctuations inside galaxy voids that have not formed galaxies because of their low densities. We estimate that these underdense LSS absorbers account for 25-30 ±6 per cent of the current Lyα population (inline image cm-2), while the other two types account for the remaining 70-75 ± 12 per cent. Assuming that only inline image cm-2 systems have embedded galaxies nearby, we have estimated the contribution of the 'halo-like' Lyα population to be ≈12-15 ± 4 per cent and consequently ≈55-60 ± 13 per cent of the Lyα systems to be associated with the overdense LSS.]]> Thu 17 Apr 2014 16:13:04 EST ]]> The VLT LBG Redshift Survey - III. The clustering and dynamics of Lyman-break galaxies at z ˜ 3 Thu 17 Apr 2014 16:13:04 EST ]]> Accurate indoor positioning technique using RSSI assisted inertial measurement Thu 17 Apr 2014 15:38:08 EST ]]> Trends of platelet inhibition in different clopidogrel pretreatment patterns in Malaysian patients undergoing elective percutaneous coronary intervention Thu 17 Apr 2014 15:38:07 EST ]]> A GIS-based environmental health information source for Malaysian context Thu 17 Apr 2014 15:38:06 EST ]]> PIVKA-II can be an ideal marker for monitoring the therapeutic efficacy of warfarin on atrial fibrilation patients Thu 17 Apr 2014 15:38:05 EST ]]> Relation of Plasma Thrombin concentration in patients with Atrial Fibrillation to differences in Warfarin Anticoagulation dosing: A prospective singlec centre study Thu 17 Apr 2014 15:38:04 EST ]]> The bivariate generalized variance |S| control chart with runs rules Thu 17 Apr 2014 15:38:03 EST ]]> De-colonisation or re-colonisation: contemporary social work and Indigenous Australians Thu 17 Apr 2014 15:17:02 EST ]]> Social work with Indigenous communities: a human rights approach, 2nd edition Thu 17 Apr 2014 15:04:05 EST ]]> Voyages of the damned Thu 17 Apr 2014 14:17:03 EST ]]> Effect of geogrids on interface shear strength properties of recycled crushed brick Thu 17 Apr 2014 12:08:02 EST ]]> Improvement of the biomedical properties of titanium using SMAT and thermal oxidation Thu 17 Apr 2014 12:08:01 EST ]]> Thank God, the city is complex Thu 17 Apr 2014 11:40:07 EST ]]> Are we listening? Thu 17 Apr 2014 11:40:06 EST ]]> City in advance: climate as trigger for adaptive planning Thu 17 Apr 2014 11:40:05 EST ]]> Advanced use of the urban metabolism model in rapidly changing cities Thu 17 Apr 2014 11:40:03 EST ]]> Development of a planning theory for wicked problems Thu 17 Apr 2014 11:40:03 EST ]]> The VLT LBG redshift survey - I. Clustering and dynamics of ≈1000 galaxies at z≈ 3 3 quasi-stellar objects (QSOs), allowing ≈21 000 2 < z < 3.5 galaxy candidates to be selected using the Lyman-break technique. We performed spectroscopic follow-up using VLT VIMOS, measuring redshifts for 1020 z > 2 Lyman-break galaxies and 10 z > 2 QSOs from a total of 19 VIMOS pointings. From the galaxy spectra, we observe a 625 ± 510 km s-1 velocity offset between the interstellar absorption and Lyman α emission-line redshifts, consistent with previous results. Using the photometric and spectroscopic catalogues, we have analysed the galaxy clustering at z≈ 3. The angular correlation function, w(θ), is well fitted by a double power law with clustering scalelength, r0= 3.19+0.32-0.54 h-1 Mpc and slope γ= 2.45 for r < 1 h-1 Mpc and r0= 4.37+0.43-0.55 h-1 Mpc with γ= 1.61 ± 0.15 at larger scales. Using the redshift sample we estimate the semiprojected correlation function, wp(σ), and, for a γ= 1.8 power law, find r0= 3.67+0.23-0.24 h-1 Mpc for the VLT sample and r0= 3.98+0.14-0.15 h-1 Mpc for a combined VLT+Keck sample. From ξ(s) and ξ(σ, π), and assuming the above ξ(r) models, we find that the combined VLT and Keck surveys require a galaxy pairwise velocity dispersion of ≈700 km s-1, higher than ≈400 km s-1 assumed by previous authors. We also measure a value for the gravitational growth rate parameter of β(z= 3) = 0.48 ± 0.17, again higher than that previously found and implying a low value for the bias of b= 2.06+1.1-0.5. This value is consistent with the galaxy clustering amplitude which gives b= 2.22 ± 0.16, assuming the standard cosmology, implying that the evolution of the gravitational growth rate is also consistent with Einstein gravity. Finally, we have compared our Lyman-break galaxy clustering amplitudes with lower redshift measurements and find that the clustering strength is not inconsistent with that of low-redshift L* spirals for simple 'long-lived' galaxy models.]]> Thu 17 Apr 2014 11:33:06 EST ]]> The VLT LBG redshift survey- II. Interactions between galaxies and the IGM at z∼ 3 Thu 17 Apr 2014 11:33:04 EST ]]> Through thick and thin - H I absorption in cosmological simulations 1018 cm-2, while the transition to fully neutral gas and conversion of H I to H2 steepen it around column densities of N H I = 1020.3 cm-2 and N H I = 1021.5 cm-2, respectively.]]> Thu 17 Apr 2014 11:33:03 EST ]]> Meta-analysis of on-the-road experimental studies of hypnotics: effects of time after intake, dose, and half-life 12 h) and both intermediate- and long-acting drugs caused significant impairment the morning after bedtime administration, whereas short acting hypnotics did not. Conclusions: These analyses indicate that the half-life, dose of the hypnotic, as well as time between treatment and driving, as measured by SDLP, all significantly impact the ability to drive a car after taking hypnotic drugs.]]> Thu 17 Apr 2014 09:20:10 EST ]]> War affected youth as consumers of microcredit: an application and extension of the Theory of Planned Behaviour Thu 17 Apr 2014 09:20:09 EST ]]> Morphologies of z ~ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity Thu 17 Apr 2014 09:20:08 EST ]]> Detection of Listeria in milk using non-targeted metabolic profiling of Listeria monocytogenes: a proof-of-concept application Thu 17 Apr 2014 09:20:07 EST ]]> Towards stellar effective temperatures and diameters at 1 per cent accuracy for future surveys Thu 17 Apr 2014 09:20:05 EST ]]> High-order clustering of WiggleZ galaxies Thu 17 Apr 2014 09:20:03 EST ]]> Ultracompact dwarfs in the Perseus Cluster: UCD formation via tidal stripping Thu 17 Apr 2014 09:20:03 EST ]]> Symposium Proceedings of Swinburne Professional Skills Forum: Providing Feedback to Students, Swinburne University of Technology, Melbourne, Australia, 9th December 2008 Thu 17 Apr 2014 08:45:10 EST ]]> Sustainability, gems and childcare: providing data enhance knowledge Thu 17 Apr 2014 08:45:08 EST ]]> The effectiveness of different wash hand basins in reducing the microbial load on the hands of food handlers Thu 17 Apr 2014 08:45:07 EST ]]> Addressing cultural diversity and food safety plans: the victorian experience Thu 17 Apr 2014 08:45:05 EST ]]> An assessment model for environmental health work-integrated learning placements Thu 17 Apr 2014 08:45:05 EST ]]>