The First Large Absorption Survey in H i (FLASH) is a large-area radio survey for neutral hydrogen in and around galaxies in the intermediate redshift range $0.4\lt z\lt1.0$, using the 21-cm H i absorption line as a probe of cold neutral gas. The survey uses the ASKAP radio telescope and will cover 24,000 deg$^2$ of sky over the next five years. FLASH breaks new ground in two ways – it is the first large H i absorption survey to be carried out without any optical preselection of targets, and we use an automated Bayesian line-finding tool to search through large datasets and assign a statistical significance to potential line detections. Two Pilot Surveys, covering around 3000 deg$^2$ of sky, were carried out in 2019-22 to test and verify the strategy for the full FLASH survey. The processed data products from these Pilot Surveys (spectral-line cubes, continuum images, and catalogues) are public and available online. In this paper, we describe the FLASH spectral-line and continuum data products and discuss the quality of the H i spectra and the completeness of our automated line search. Finally, we present a set of 30 new H i absorption lines that were robustly detected in the Pilot Surveys, almost doubling the number of known H i absorption systems at $0.4\lt z\lt1$. The detected lines span a wide range in H i optical depth, including three lines with a peak optical depth $\tau\gt1$, and appear to be a mixture of intervening and associated systems. Interestingly, around two-thirds of the lines found in this untargeted sample are detected against sources with a peaked-spectrum radio continuum, which are only a minor (5–20%) fraction of the overall radio-source population. The detection rate for H i absorption lines in the Pilot Surveys (0.3 to 0.5 lines per 40 deg$^2$ ASKAP field) is a factor of two below the expected value. One possible reason for this is the presence of a range of spectral-line artefacts in the Pilot Survey data that have now been mitigated and are not expected to recur in the full FLASH survey. A future paper in this series will discuss the host galaxies of the H i absorption systems identified here.

Objectives/Goals: This study assesses the feasibility of a human-to-swine lung transplant model for the evaluation of bioengineered organs. Given the critical organ shortage, this research explores bioengineered organs as a potential solution by evaluating early lung function, immune responses, and technical aspects to develop a model for bioengineered lungs. Methods/Study Population: The study employs a non-survival human-to-swine left lung transplant model in an immunosuppressed Yorkshire swine. A combination of cobra venom factor pretreated with methylprednisolone and Benadryl with scheduled dosing of tacrolimus and mycophenolate over a 24-hour period will be administered. The transplanted human lung is assessed over a 24-hour post-transplant period, with hourly pulmonary vein gas sampling and lung tissue resections. The proposed model will assess the immunological response of swine to human lung tissue as well as the efficacy of the immunosuppression model. Tissue samples are taken at intervals to evaluate for signs of rejection, cellular damage, and the overall function of the transplanted lung. All tissues are preserved in formaldehyde for subsequent immunohistology evaluation. Results/Anticipated Results: We anticipate a successful non-survival swine transplant model with pulmonary function sustained for the full 24-hour study using our proposed immunosuppression regimen. Initial testing with a standard human lung will lay the groundwork to assess the effectiveness of the human-to-swine transplant model. Hourly pulmonary vein gas analyses and tissue biopsies are expected to show minimal immune rejection, supported by the preoperative immunosuppression regimen. Early data indicate that the swine tolerates both the surgical procedure and immunosuppressive therapy well, with manageable hemodynamic stability. This model is expected to yield critical insights into lung viability and will identify areas for optimization for long-term survival studies to test the efficacy of bioengineered organs. Discussion/Significance of Impact: This non-survival swine model offers valuable insights into the acute-phase immune response and functional viability of human-to-swine lung transplant model. The findings will support the development of long-term survival models that will allow the evaluation of bioengineered organs based solely on their functionality as engineered organs.

Task-shared psychological treatments play a critical role in addressing the global mental health treatment gap, yet their integration into routine care requires further study. This study evaluated the causal association between an implementation factor of a task-shared psychological treatment and participant outcomes to strengthen the implementation-to-outcome link within global mental health. This secondary analysis utilized cohort data from the Program for Improving Mental Health Care (PRIME) implemented in Sehore, India where trained non-specialist health workers delivered treatment for depression and alcohol use disorder (AUD). Propensity scores and inverse probability of treatment weights examined the impact of mental health service users’ treatment attendance on users’ symptom severity (PHQ-9 scores for depression; AUDIT scores for AUD) at 3 and 12-month follow-ups. Among the 240 patients with depression, higher treatment session attendance led to 1.3 points lower PHQ-9 scores (vs. no attendance) and 2.4 points lower PHQ-9 scores (vs. low attendance) at 3 months, with no significant effects at 12 months. Among the 190 AUD patients, treatment session attendance did not have a significant impact on AUDIT scores. Our findings have implications for enhancing treatment session attendance among those with depression within task-shared psychological treatments.

Although the basic test for apprehended bias is now well-established in Australian law, its application continues to present difficulties. The basic test is whether a fair-minded lay observer with knowledge of the material objective facts might reasonably apprehend that the judicial or administrative decision-maker might not bring an impartial and unprejudiced mind to the resolution of the question at hand. It is equally well-established that, while the same objective test applies to judges as to tribunal members and other public decision-makers, the application and content of that test varies depending on the context, including differences in decision-making roles, functions, powers and processes.

The application of the test can be problematic and somewhat unpredictable. For example, despite the unqualified terms of the relevant parts of the High Court’s decision in Ebner, it now appears that, at least in the context of curial decision-making, the Ebner two-step test is not universal in its application.

Over the last three years the Commonwealth has enacted four statutes with the aim of overcoming some of the deficiencies which exist at common law in the reviewing of administrative action. These are the Administrative Appeals Tribunal Act 1975 (Cth), the Administrative Appeals Tribunal Amendment Act 1977 (Cth), the Ombudsman Act 1976 (Cth) and the Administrative Decisions (Judicial Review) Act 1977 (Cth). This article examines in detail the Administrative Decisions (Judicial Review) Act 1977 (Cth) in order to determine whether the common law rights and remedies have been improved.

The Magellanic Stream (MS), a tail of diffuse gas formed from tidal and ram pressure interactions between the Small and Large Magellanic Clouds (SMC and LMC) and the Halo of the Milky Way, is primarily composed of neutral atomic hydrogen (HI). The deficiency of dust and the diffuse nature of the present gas make molecular formation rare and difficult, but if present, could lead to regions potentially suitable for star formation, thereby allowing us to probe conditions of star formation similar to those at high redshifts. We search for $\text{HCO}^{+}$, HCN, HNC, and C$_2$H using the highest sensitivity observations of molecular absorption data from the Atacama Large Millimeter Array (ALMA) to trace these regions, comparing with HI archival data from the Galactic Arecibo L-Band Feed Array (GALFA) HI Survey and the Galactic All Sky Survey (GASS) to compare these environments in the MS to the HI column density threshold for molecular formation in the Milky Way. We also compare the line of sight locations with confirmed locations of stars, molecular hydrogen, and OI detections, though at higher sensitivities than the observations presented here.

We find no detections to a 3$\sigma$ significance, despite four sightlines having column densities surpassing the threshold for molecular formation in the diffuse regions of the Milky Way. Here we present our calculations for the upper limits of the column densities of each of these molecular absorption lines, ranging from $3 \times 10^{10}$ to $1 \times 10^{13}$ cm$^{-2}$. The non-detection of $\text{HCO}^{+}$ suggests that at least one of the following is true: (i) $X_{\text{HCO}^{+}{}, \mathrm{MS}}$ is significantly lower than the Milky Way value; (ii) that the widespread diffuse molecular gas observed by Rybarczyk (2022b, ApJ, 928, 79) in the Milky Way’s diffuse interstellar medium (ISM) does not have a direct analogue in the MS; (iii) the HI-to-$\text{H}_{2}$ transition occurs in the MS at a higher surface density in the MS than in the LMC or SMC; or (iv) molecular gas exists in the MS, but only in small, dense clumps.

There is an increasing emphasis worldwide on breeding wheat cultivars with higher biomass and grain yield, whilst reducing excessive input of N fertilizers. Modern plant breeding has narrowed the genetic base of bread wheat, so exploring new sources of genetic variation for leaf photosynthesis traits and biomass to underpin grain yield improvement has become necessary. Our objectives were to quantify the genetic variability in a range of landrace-derived lines and elite bread wheat genotypes in flag-leaf photosynthesis traits, biomass and N-use efficiency for potential application in pre-breeding. Sixteen bread wheat genotypes including elite spring wheat cultivar Paragon × landrace crosses were tested in two field experiments in the UK. Averaging across years, pre-anthesis flag-leaf photosynthesis rate ranged amongst genotypes from 26.0 to 31.5 μmol/m2/s (P < 0.001) and post-anthesis from 14.2 to 18.6 μmol/m2/s (P < 0.001). Two landrace-derived lines had greater post-anthesis flag-leaf photosynthesis rate (P < 0.001) than their elite parent Paragon. There was a trend for a positive correlation among genotypes between post-anthesis flag-leaf photosynthesis rate and biomass (r = 0.47, P = 0.06). Two landrace derivatives showed higher post-anthesis flag-leaf stomatal conductance than Paragon. Our results indicated that introgression of traits from wider germplasm into elite UK modern wheat germplasm offers scope to raise flag-leaf photosynthetic rate and biomass.

Early life stress (ELS) and a Western diet (WD) promote mood and cardiovascular disorders, however, how these risks interact in disease pathogenesis is unclear. We assessed effects of ELS with or without a subsequent WD on behaviour, cardiometabolic risk factors, and cardiac function/ischaemic tolerance in male mice. Fifty-six new-born male C57BL/6J mice were randomly allocated to a control group (CON) undisturbed before weaning, or to maternal separation (3h/day) and early (postnatal day 17) weaning (MSEW). Mice consumed standard rodent chow (CON, n = 14; MSEW, n = 15) or WD chow (WD, n = 19; MSEW + WD, n = 19) from week 8 to 24. Fasted blood was sampled and open field test and elevated plus maze (EPM) tests undertaken at 7, 15, and 23 weeks of age, with hearts excised at 24 weeks for Langendorff perfusion (evaluating pre- and post-ischaemic function). MSEW alone transiently increased open field activity at 7 weeks; body weight and serum triglycerides at 4 and 7 weeks, respectively; and final blood glucose levels and insulin resistance at 23 weeks. WD increased insulin resistance and body weight gain, the latter potentiated by MSEW. MSEW + WD was anxiogenic, reducing EPM open arm activity vs. WD alone. Although MSEW had modest metabolic effects and did not influence cardiac function or ischaemic tolerance in lean mice, it exacerbated weight gain and anxiogenesis, and improved ischaemic tolerance in WD fed animals. MSEW-induced increases in body weight (obesity) in WD fed animals in the absence of changes in insulin resistance may have protected the hearts of these mice.

We present the first unbiased survey of neutral hydrogen absorption in the Small Magellanic Cloud. The survey utilises pilot neutral hydrogen observations with the Australian Square Kilometre Array Pathfinder telescope as part of the Galactic Australian Square Kilometre Array Pathfinder neutral hydrogen project whose dataset has been processed with the Galactic Australian Square Kilometre Array Pathfinder-HI absorption pipeline, also described here. This dataset provides absorption spectra towards 229 continuum sources, a 275% increase in the number of continuum sources previously published in the Small Magellanic Cloud region, as well as an improvement in the quality of absorption spectra over previous surveys of the Small Magellanic Cloud. Our unbiased view, combined with the closely matched beam size between emission and absorption, reveals a lower cold gas faction (11%) than the 2019 ATCA survey of the Small Magellanic Cloud and is more representative of the Small Magellanic Cloud as a whole. We also find that the optical depth varies greatly between the Small Magellanic Cloud’s bar and wing regions. In the bar we find that the optical depth is generally low (correction factor to the optically thin column density assumption of $\mathcal{R}_{\mathrm{HI}} \sim 1.04$) but increases linearly with column density. In the wing however, there is a wide scatter in optical depth despite a tighter range of column densities.

The Rapid ASKAP Continuum Survey (RACS) is the first large-area survey to be conducted with the full 36-antenna Australian Square Kilometre Array Pathfinder (ASKAP) telescope. RACS will provide a shallow model of the ASKAP sky that will aid the calibration of future deep ASKAP surveys. RACS will cover the whole sky visible from the ASKAP site in Western Australia and will cover the full ASKAP band of 700–1800 MHz. The RACS images are generally deeper than the existing NRAO VLA Sky Survey and Sydney University Molonglo Sky Survey radio surveys and have better spatial resolution. All RACS survey products will be public, including radio images (with $\sim$ 15 arcsec resolution) and catalogues of about three million source components with spectral index and polarisation information. In this paper, we present a description of the RACS survey and the first data release of 903 images covering the sky south of declination $+41^\circ$ made over a 288-MHz band centred at 887.5 MHz.

This work investigated the photophysical pathways for light absorption, charge generation, and charge separation in donor–acceptor nanoparticle blends of poly(3-hexylthiophene) and indene-C60-bisadduct. Optical modeling combined with steady-state and time-resolved optoelectronic characterization revealed that the nanoparticle blends experience a photocurrent limited to 60% of a bulk solution mixture. This discrepancy resulted from imperfect free charge generation inside the nanoparticles. High-resolution transmission electron microscopy and chemically resolved X-ray mapping showed that enhanced miscibility of materials did improve the donor–acceptor blending at the center of the nanoparticles; however, a residual shell of almost pure donor still restricted energy generation from these nanoparticles.

Across the globe, there has been a marked increase in longevity, but significant inequalities remain. These are exacerbated by inadequate access to proper nutrition and health care services and to reliable information to make the decisions related to nutrition and health care. Many in economically developing as well as developed societies are plagued with the double-burden of energy excess and undernutrition. This has resulted in mental and physical deterioration, increased non-communicable disease rates, lost productivity, increased medical costs and reduced quality of life. While adequate nutrition is fundamental to good health at all stages of the life course, the impact of diet on prolonging good quality of life during ageing remains unclear. For progress to continue, there is need for new and/or innovative approaches to promoting health as individuals age, as well as qualitative and quantitative biomarkers and other accepted tools that can measure improvements in physiological integrity throughout life. A framework for progress has been proposed by the World Health Organization in their Global Strategy and Action Plan on Ageing and Health. Here, we focused on the impact of nutrition within this framework, which takes a broad, person-centred emphasis on healthy ageing, stressing the need to better understand each individual's intrinsic capacity, their functional abilities at various life stages, and the impact of their mental, and physical health, as well as the environments they inhabit.