https://nova.newcastle.edu.au/vital/access/ /manager/Index en-au 5 https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:25064 in vivo dosimetry, brachytherapy and auditing of radiotherapy practice. Recent developments of dosimeters that can be used for these purposes are discussed using spatial resolution and number of dimensions for measurement as sorting criteria. While dosimetry is ever evolving to address the needs of advancing applications of radiation in medicine two fundamental issues remain: the accuracy of the measurement from a scientific perspective and the importance to link the measurement to a clinically relevant question. This review aims to provide an update on both of these.]]> Wed 24 Nov 2021 15:51:37 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:47123 Wed 22 Mar 2023 19:02:39 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34514 Rₑ) and ellipticity (ϵₑ) are used to separate fast and slow rotators; there exists a good correspondence to regular and non-regular rotators, respectively, as also seen in earlier studies. We confirm that regular rotators show a strong h₃ versus V/σ anti-correlation, whereas quasi-regular and non-regular rotators show a more vertical relation in h₃ and V/σ. Motivated by recent cosmological simulations, we develop an alternative approach to kinematically classify galaxies from their individual h₃ versus V/σ signatures. Within the SAMI Galaxy Survey, we identify five classes of high-order stellar kinematic signatures using Gaussian mixture models. Class 1 corresponds to slow rotators, whereas Classes 2-5 correspond to fast rotators. We find that galaxies with similar λ_Rₑ - ϵₑ values can show distinctly different h₃ - V/σ signatures. Class 5 objects are previously unidentified fast rotators that show a weak h₃ versus V/σ anti-correlation. From simulations, these objects are predicted to be disk-less galaxies formed by gas-poor mergers. From morphological examination, however, there is evidence for large stellar disks. Instead, Class 5 objects are more likely disturbed galaxies, have counter-rotating bulges, or bars in edge-on galaxies. Finally, we interpret the strong anti-correlation in h₃ versus V/σ as evidence for disks in most fast rotators, suggesting a dearth of gas-poor mergers among fast rotators.]]> Wed 20 Mar 2019 13:17:45 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:32715 Wed 18 Jul 2018 16:19:36 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:39588 Wed 15 Jun 2022 12:47:02 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:47102 Wed 14 Dec 2022 09:51:28 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17106 Wed 11 Apr 2018 17:01:24 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:25165 Q calculations which show a much smaller difference between FFF and flattened beams than originally predicted. These results are explained by the inclusion of the added backscatter plates and build-up filters used in modern clinical FFF linacs, compared to a Monte Carlo model of an FFF linac in which the flattening filter is removed and no additional build-up or backscatter plate is added.]]> Wed 11 Apr 2018 16:42:22 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17103 Wed 11 Apr 2018 15:30:09 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17100 Wed 11 Apr 2018 15:17:45 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:20853 c, consistent with λeQ²/_s coupling. There is no change in dissipation associated with this high temperature transition, and no evidence in the elastic or anelastic behaviour for any secondary transition at ~920 K, thus supporting the thesis of a single high temperature transformation. Elastic stiffening is observed on cooling through T_N, in accordance with previous studies, and the excess elastic constant appears to scale with the square of the magnetic order parameter. The strains incurred at T_N are a factor of ~20 smaller than those at the structural transition, implying very weak λeQ²/_m coupling and a dominant contribution to the variation in the elastic constants from λeQ²/_m. The increased acoustic dissipation above T_N is consistent with an order–disorder process.]]> Wed 11 Apr 2018 15:07:37 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17105 Wed 11 Apr 2018 14:38:42 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:26435 Wed 11 Apr 2018 14:07:26 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17196 Wed 11 Apr 2018 13:31:39 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17002 Wed 11 Apr 2018 12:45:09 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:17163 98% of points passing a gamma analysis with 3%/3 mm criterion for all field sizes. The simulated anthropomorphic head phantom image shows macroscopic anatomical features and qualitatively agrees with the measured image. Results validate the suitability of the MC model for predicting EPID response in transit dosimetry.]]> Wed 11 Apr 2018 12:00:20 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:29911 Wed 11 Apr 2018 09:48:16 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:53719 Wed 10 Jan 2024 11:17:58 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:31828 Wed 09 Mar 2022 16:00:57 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34215 Wed 04 Sep 2019 12:18:12 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:35576 Wed 04 Sep 2019 11:32:47 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34656 Wed 04 Sep 2019 09:49:38 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:33990 Wed 04 Sep 2019 09:48:58 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:32482 Wed 04 Sep 2019 09:48:21 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34554 Wed 04 Sep 2019 09:48:05 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:33939 Wed 02 Mar 2022 14:26:19 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:47828 Wed 01 Feb 2023 13:08:00 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:47820 Wed 01 Feb 2023 10:33:49 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34305 Tue 26 Feb 2019 15:18:09 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:54371 Tue 20 Feb 2024 19:57:43 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:30491 Tue 20 Aug 2024 11:43:50 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:52556 Tue 17 Oct 2023 15:34:22 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:46341 Tue 14 Nov 2023 14:55:52 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34752 Tue 03 Sep 2019 18:31:15 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34083 ⊙), cold (12 K), and 3.6–70 μm IR dark clump (MM1) that has the potential to form high-mass stars. We observed this prestellar clump candidate with the Submillimeter Array (~3".5 resolution) and Jansky Very Large Array (~2farcs1 resolution) in order to characterize the early stages of high-mass star formation and to constrain theoretical models. Dust emission at 1.3 mm wavelength reveals five cores with masses ≤15 M_⊙. None of the cores currently have the mass reservoir to form a high-mass star in the prestellar phase. If the MM1 clump will ultimately form high-mass stars, its embedded cores must gather a significant amount of additional mass over time. No molecular outflows are detected in the CO (2-1) and SiO (5-4) transitions, suggesting that the SMA cores are starless. By using the NH₃ (1, 1) line, the velocity dispersion of the gas is determined to be transonic or mildly supersonic (ΔV_nt/ΔV_th ~ 1.1–1.8). The cores are not highly supersonic as some theories of high-mass star formation predict. The embedded cores are four to seven times more massive than the clump thermal Jeans mass and the most massive core (SMA1) is nine times less massive than the clump turbulent Jeans mass. These values indicate that neither thermal pressure nor turbulent pressure dominates the fragmentation of MM1. The low virial parameters of the cores (0.1–0.5) suggest that they are not in virial equilibrium, unless strong magnetic fields of ~1–2 mG are present. We discuss high-mass star formation scenarios in a context based on IRDC G028.23-00.19, a study case believed to represent the initial fragmentation of molecular clouds that will form high-mass stars.]]> Tue 03 Sep 2019 18:23:32 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:34944 + (1–0) line for the "blue asymmetry" spectroscopic signature of infall motion in a large sample of high-mass, dense molecular clumps observed to be at different evolutionary stages of star cluster formation according to their mid-infrared appearance. To quantify the degree of the line asymmetry, we measure the asymmetry parameter A=[formula could not be replicated], the fraction of the integrated intensity that lies to the blueshifted side of the systemic velocity determined from the optically thin tracer N₂H⁺ (1–0). For a sample of 1093 sources, both the mean and median of A are positive (A=0.0830 ± 010 and 0.065 ± 0.009, respectively) with high statistical significance, and a majority of sources (a fraction of 0.607 ± 0.015 of the sample) show positive values of A, indicating a preponderance of blue asymmetric profiles over red asymmetric profiles. Two other measures, the local slope of the line at the systemic velocity and the δv parameter of Mardones et al. (1997), also show an overall blue asymmetry for the sample, but with smaller statistical significance. This blue asymmetry indicates that these high-mass clumps are predominantly undergoing gravitational collapse. The blue asymmetry is larger (A ∼ 0.12) for the earliest evolutionary stages (quiescent, protostellar, and compact H ii region) than for the later H ii region (A ∼ 0.06) and photodissociation region (A ∼ 0) classifications.]]> Tue 03 Sep 2019 17:57:00 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:35015 Thu 30 May 2019 16:15:52 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:50497 Thu 27 Jul 2023 10:50:34 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:44459 Thu 13 Oct 2022 15:20:25 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:29622 Thu 09 Dec 2021 11:02:48 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:43126 Thu 02 Nov 2023 13:16:15 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:12924 n(r₁,...,r_n) = 1/π²[formula could not be replicated]. By virtue of striking connections with Jacobi ϑ-function values, we are able to develop new closed forms for certain values of the coordinates r_k, and extend such analysis to similar lattice sums. A primary result is that for rational x, y, the natural potential ⏀²(x, y) is 1/π log A where A is an algebraic number. Various extensions and explicit evaluations are given. Such work is made possible by number-theoretical analysis, symbolic computation and experimental mathematics, including extensive numerical computations using up to 20,000-digit arithmetic.]]> Sat 24 Mar 2018 10:37:10 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:31514 Sat 24 Mar 2018 08:44:17 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:15637 Sat 24 Mar 2018 08:23:45 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:9936 Sat 24 Mar 2018 08:14:17 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:11188 Sat 24 Mar 2018 08:13:36 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:11523 Sat 24 Mar 2018 08:10:22 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:10719 Sat 24 Mar 2018 08:09:48 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:12124 Sat 24 Mar 2018 08:08:54 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:11180 Sat 24 Mar 2018 08:08:26 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:20852 Sat 24 Mar 2018 08:02:54 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:18008 Sat 24 Mar 2018 07:56:16 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:19137 Sat 24 Mar 2018 07:55:54 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:20589 Sat 24 Mar 2018 07:55:35 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:19730 T_N = 946 ± 1 K is an example of a multiferroic transition which has both ferromagnetic (from canting of antiferromagnetically ordered spin moments) and ferroelastic (rhombohedral → monoclinic) character. By analogy with the improper ferroelastic transition in Pb₃(PO₄)₂, W and W' ferroelastic twin walls which are also 60° and 120° magnetic domain walls should develop. These have been tentatively identified from microstructures reported in the literature. The very low attenuation in the stability field of the C2/c structure in the polycrystalline sample used in the present study, in comparison with the strong acoustic dissipation reported for single crystal samples, implies, however, that the individual grains each consist of a single ferroelastic domain or that the twin walls are strongly pinned by grain boundaries. This absence of attenuation allows an intrinsic loss mechanism associated with the transition point to be seen and interpreted in terms of local coupling of shear strains with fluctuations which have relaxation times in the vicinity of ~10⁻⁸s. The first order [formula could not be replicated] (Morin) transition occurs through a temperature interval of coexisting phases but the absence of an acoustic loss peak suggests that the relaxation time for interface motion is short in comparison with the time scale of the applied stress (at ~0.1–1 MHz). Below the Morin transition a pattern of attenuation which resembles that seen below ferroelastic transitions has been found, even though the ideal low temperature structure cannot contain ferroelastic twins. This loss behavior is tentatively ascribed to the presence of local ferromagnetically ordered defect regions which are coupled locally to shear strains.]]> Sat 24 Mar 2018 07:53:45 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:21332 Sat 24 Mar 2018 07:52:48 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:20143 Sat 24 Mar 2018 07:51:36 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:21548 19 atoms per second per steradian. The beam performance was investigated using a conventional ion gauge and a stagnation detector, with the latter being used to produce beam flux profiles. The profile of the macroskimmed beam has been experimentally demonstrated to be strongly Gaussian.]]> Sat 24 Mar 2018 07:50:25 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:21546 Sat 24 Mar 2018 07:50:25 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:21551 Sat 24 Mar 2018 07:50:23 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:28067 Sat 24 Mar 2018 07:39:47 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:27970 Sat 24 Mar 2018 07:38:43 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:26384 Sat 24 Mar 2018 07:33:05 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:28541 Sat 24 Mar 2018 07:28:47 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:25899 Sat 24 Mar 2018 07:28:17 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:27483 Sat 24 Mar 2018 07:25:39 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:27721 Sat 24 Mar 2018 07:24:37 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:25150 Sat 24 Mar 2018 07:17:09 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:23365 1-xO, at the Néel temperature, T _N∼195K, is treated in terms of coupling between two macroscopic order parameters related to separate discrete instabilities. These each couple with a rhombohedral shear strain to give an indirect mechanism of linear (structural)quadratic (magnetic) coupling between them. Based on patterns of lattice parameter and magnetic ordering data from the literature, it appears that the overall behaviour matches the general pattern of linear-quadratic coupling for a system with two rather similar instability temperatures. At low pressures, the magnetic instability occurs at a higher temperature than the structural instability but the coupling results in a single phase transition dominated by the influence of the magnetic order parameter. For Fe _0.99O the magnetic order parameter, m, varies with temperature as ∼m ⁸σ(T _NT), while for Fe _0.94O the temperature dependence is of ∼m ⁴ or ∼m ². It is proposed that, with increasing pressure, there is a crossover of instability temperatures such that the structural instability occurs first at pressures above ∼13GPa. This would be expected to give rise to a first-order phase transition, as appears to occur, but magnetic ordering would still occur simultaneously if the coupling is sufficiently strong. Symmetry analysis and comparison with the behaviour of MnO shows that there are a number of different possible magnetically ordered structures which could be stabilized by pressure or non-hydrostatic stress to give topologically rich phase diagrams.]]> Sat 24 Mar 2018 07:16:30 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:23774 c ≈ 350 K. This matches the evolution of the intensity of the elastic central peak in neutron scattering spectra, and reflects the development of static (or quasistatic) polar nanoregions (PNRs) as if by a mean-field phase transition. Use of a Landau free energy expansion, which includes Γ̅₄ order parameter components to describe ferroelectric contributions and an R¹(+) order parameter to describe cation ordering together with their formal coupling with strain, then allows the pattern of elastic softening expected for a cubic → rhombohedral phase transition to be anticipated. The extent to which observed softening differs from this static mean-field pattern serves to highlight the additional roles of local heterogeneity and relaxation dynamics in determining the relaxor properties of PMN.]]> Sat 24 Mar 2018 07:13:21 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:24544 Sat 24 Mar 2018 07:11:33 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:49688 Mon 29 May 2023 11:08:53 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:44893 Mon 24 Oct 2022 15:42:26 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:47471 Mon 23 Jan 2023 11:05:51 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:12153 Mon 19 Aug 2024 10:32:19 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:47960 Mon 13 Feb 2023 14:42:01 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:55171 Mon 12 Aug 2024 08:13:22 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:49244 Mon 08 May 2023 10:21:31 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:39209 Arabidopsis epidermal peel were detected with or without exogenous application of mannose, fructose, glucose, and glucose-6-phosphate (G-6P). The results here showed that G-6P, but not glucose itself, induces stomatal closure in Arabidopsis. Furthermore, detection of stomatal apertures of Arabidopsis hexokinase loss of function with exogenous application of glucose showed that glucose induced stomatal closure was not due to osmotic pressure and it triggered guard cell ROS production depend on hexokinase activity. The effect of irradiance and G-6P on regulation of Arabidopsis stomatal aperture was investigated. The data obtained here indicated that G-6P induced changes of stomatal aperture depend on irradiance.]]> Fri 27 May 2022 10:20:29 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:49482 Fri 19 May 2023 15:49:16 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:43414 Fri 16 Sep 2022 14:31:25 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:33736 1V) and without (sCT) a one voxel body contour expansion included in the algorithm. This was to test whether this expansion was required for 1.5 T images. Both synthetic CT's were rigidly registered to the planning CT (pCT). A 6 MV Volumetric Modulated Arc Therapy plan was created on the pCT and recalculated on the sCT and sCT_1V The synthetic CT's dose distributions were compared to the dose distribution calculated on the pCT. The percentage dose difference at isocentre without the body contour expansion (sCT - pCT) was ΔD_sCT = (0.9 ± 0.8) % and with (sCT_1V-pCT) was ΔD_sCT1V = (-0.7 ± 0.7) % (mean ± one standard deviation). The sCT_1V; result was within one standard deviation of zero and agreed with the result reported previously using 3 T MR data. The sCT dose difference only agreed within two standard deviations. The mean ± one standard deviation gamma pass rate was Γ_sCT = 96.1 ± 2.9% for the sCT and Γ_sCT1V = 98.8 ± 0.5% for the sCT_1V (with 2% global dose difference and 2 mm distance to agreement gamma criteria). The one voxel body contour expansion improves the synthetic CT accuracy for MR images acquired at 1.5 T but requires the MR voxel size to be similar to the atlas MR voxel size. This study suggests that the atlas-based algorithm can be generalised to MR data acquired using a different field strength at a different centre.]]> Fri 14 Dec 2018 14:42:04 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:37227 Fri 11 Sep 2020 09:08:48 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:43003 Fri 09 Sep 2022 14:10:35 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:42981 0.999. EDLG results were analyzed as a difference relative to a baseline EDLG measurement for each machine, a metric we labeled the leaf offset constancy (LOC). The maximum change in LOC out of the 20 repeatability tests was −0.094 mm. The LOC QC process was found to be capable (Cpk > 1) for 4 machines using a ± 0.15 mm specification limit. LOC results showed that leaves may deviate from their reference positions at a level that approaches dosimetric significance for small stereotactic and highly modulated treatment fields, with average excursions measuring up to 0.21 mm for a Millennium MLC and 0.16 mm for a HD MLC. The effects of initialization, gantry angle, and common repairs are also reported.]]> Fri 09 Sep 2022 13:56:28 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:37313 Fri 02 Oct 2020 11:44:12 AEST ]]>