This review summarizes findings from studies in companion animals with chronic diseases receiving omega-3 supplementation. Investigated conditions included dermatopathies (dogs n=7), osteoarthritis (dogs n=7, cats n=2), cardiovascular diseases (dogs n=7), dyslipidaemias (dogs n=1), gastroenteropathies (dogs n=2), chronic kidney disease (dogs n=2, cats n=3), cognitive impairment (dogs n=4, cats n=1), and behavioural disorders (dogs n=3). When possible, dosages were standardized to mg/kg using available data on food intake and EPA/DHA concentrations. The minimum and maximum ranges of EPA and DHA, along with their ratios, were as follows: for dermatology 0.99–43 mg/kg EPA and 0.66–30 mg/kg DHA (ratio 1.4–3.4); for osteoarthritis 48–100 mg/kg EPA and 20–32 mg/kg DHA (ratio 1.5–3.4); cardiology 27–54.2 mg/kg EPA and 18–40.6 mg/kg DHA (ratio 1.3–1.5); dyslipidaemia 58.8 mg/kg EPA and 45.4 mg/kg DHA (ratio 1.3); cognition (1/5 studies) 225 mg/kg EPA and 90 mg/kg DHA (ratio 2.5); behaviour (1/3) 31 mg/kg EPA and 45 mg/kg DHA (ratio 0.7). Nephrology and oncology studies lacked sufficient data for calculation. Gastrointestinal diseases do not appear to benefit from omega-3 supplementation, likely due to inflammation-related malabsorption, although few adverse effects were reported in dogs. Other enteropathy studies were low-quality (case reports/series). The lowest omega-6/omega-3 ratio with anti-inflammatory effect was 1:3.75; the highest was 5.5:1. In conclusion, the reviewed EPA and DHA doses appear effective for atopic dermatitis, osteoarthritis, cardiac disease, hyperlipidaemia, and cognitive and behavioural disorders. Further research is needed to clarify efficacy in gastrointestinal and oncological conditions.

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 < z < 1.0, 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 deg2 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 deg2 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 < z < 1. The detected lines span a wide range in H i optical depth, including three lines with a peak optical depth τ > 1, 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 deg2 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.

The Australian SKA Pathfinder (ASKAP) offers powerful new capabilities for studying the polarised and magnetised Universe at radio wavelengths. In this paper, we introduce the Polarisation Sky Survey of the Universe’s Magnetism (POSSUM), a groundbreaking survey with three primary objectives: (1) to create a comprehensive Faraday rotation measure (RM) grid of up to one million compact extragalactic sources across the southern ∼ 50 per cent of the sky (20,630 deg2); (2) to map the intrinsic polarisation and RM properties of a wide range of discrete extragalactic and Galactic objects over the same area; and (3) to contribute interferometric data with excellent surface brightness sensitivity, which can be combined with single-dish data to study the diffuse Galactic interstellar medium. Observations for the full POSSUM survey commenced in May 2023 and are expected to conclude by mid-2028. POSSUM will achieve an RM grid density of around 30–50 RMs per square degree with a median measurement uncertainty of ∼1 rad m−2. The survey operates primarily over a frequency range of 800–1088 MHz, with an angular resolution of 20″ and a typical RMS sensitivity in Stokes Q or U of 18 μJy beam−1. Additionally, the survey will be supplemented by similar observations covering 1296–1440 MHz over 38 per cent of the sky. POSSUM will enable the discovery and detailed investigation of magnetized phenomena in a wide range of cosmic environments, including the intergalactic medium and cosmic web, galaxy clusters and groups, active galactic nuclei and radio galaxies, the Magellanic System and other nearby galaxies, galaxy halos and the circumgalactic medium, and the magnetic structure of the Milky Way across a very wide range of scales, as well as the interplay between these components. This paper reviews the current science case developed by the POSSUM Collaboration and provides an overview of POSSUM’s observations, data processing, outputs, and its complementarity with other radio and multi-wavelength surveys, including future work with the SKA.

We undertake a comprehensive investigation into the distribution of in situ stars within Milky Way-like galaxies, leveraging TNG50 simulations and comparing their predictions with data from the H3 survey. Our analysis reveals that 28% of galaxies demonstrate reasonable agreement with H3, while only 12% exhibit excellent alignment in their profiles, regardless of the specific spatial cut employed to define in situ stars. To uncover the underlying factors contributing to deviations between TNG50 and H3 distributions, we scrutinize correlation coefficients among internal drivers(e.g., virial radius, star formation rate [SFR]) and merger-related parameters (such as the effective mass-ratio, mean distance, average redshift, total number of mergers, average spin-ratio and maximum spin alignment between merging galaxies). Notably, we identify significant correlations between deviations from observational data and key parameters such as the median slope of virial radius, mean SFR values, and the rate of SFR change across different redshift scans. Furthermore, positive correlations emerge between deviations from observational data and parameters related to galaxy mergers. We validate these correlations using the Random Forest Regression method. Our findings underscore the invaluable insights provided by the H3 survey in unravelling the cosmic history of galaxies akin to the Milky Way, thereby advancing our understanding of galactic evolution and shedding light on the formation and evolution of Milky Way-like galaxies in cosmological simulations.

We present the Evolutionary Map of the Universe (EMU) survey conducted with the Australian Square Kilometre Array Pathfinder (ASKAP). EMU aims to deliver the touchstone radio atlas of the southern hemisphere. We introduce EMU and review its science drivers and key science goals, updated and tailored to the current ASKAP five-year survey plan. The development of the survey strategy and planned sky coverage is presented, along with the operational aspects of the survey and associated data analysis, together with a selection of diagnostics demonstrating the imaging quality and data characteristics. We give a general description of the value-added data pipeline and data products before concluding with a discussion of links to other surveys and projects and an outline of EMU’s legacy value.

The quasi-geostrophic two-layer model is a widely used tool to study baroclinic instability in the ocean. One instability criterion for the inviscid two-layer model is that the potential vorticity (PV) gradient must change sign between the layers. This has a well-known implication if the model includes a linear bottom slope: for sufficiently steep retrograde slopes, instability is suppressed for a flow parallel to the isobaths. This changes in the presence of bottom friction as well as when the PV gradients in the layers are not aligned. We derive the generalised instability condition for the two-layer model with non-zero friction and arbitrary mean flow orientation. This condition involves neither the friction coefficient nor the bottom slope; even infinitesimally weak bottom friction destabilises the system regardless of the bottom slope. We then examine the instability characteristics as a function of varying slope orientation and magnitude. The system is stable across all wavenumbers only if friction is absent and if the planetary, topographic and stretching PV gradients are aligned. Strong bottom friction decreases the growth rates but also alters the dependence on bottom slope. In conclusion, the often mentioned stabilisation by steep bottom slopes in the two-layer model holds only in very specific circumstances, thus probably plays only a limited role in the ocean.

Cardiometabolic pregnancy complications, including gestational diabetes mellitus (GDM), hypertensive disorders of pregnancy (HDP), intrauterine growth restriction (IUGR) and preterm birth (PTB) are prevalent pregnancy complications that adversely affect maternal and neonatal health during pregnancy, and increase women’s risk of future type 2 diabetes mellitus (T2DM) and cardiovascular disease (CVD)1–5. Pregnancy and postpartum, including intrapartum periods, are critical windows of opportunity to deliver care to support sustained behaviour change(6). There is currently a gap in lifestyle (diet and physical activity) interventions specific to cardiometabolic disease risk awareness and prevention during and following pregnancy(5,7). These are key life stages where early risk factors for cardiometabolic disease may present, women are actively engaged in the healthcare system and their health priorities are shifting as they transition into parenthood. Early intervention in pregnancy may enable commencement of pharmacological and/or lifestyle intervention to reduce the risk or severity of cardiometabolic pregnancy complications(8), whereas postpartum intervention may enable commencement of sustainable lifestyle change for reduction of long-term cardiometabolic risks(9). There are a range of settings where pregnant and postpartum women receive healthcare, including hospitals, primary care clinics, community health institutions and online platforms(8,10,11). The optimum timing and setting to deliver an intervention to these high-risk women is not known. Designing interventions to align with the needs and priorities of stakeholders is a critical first step in developing an acceptable intervention. The aims of this research were to explore stakeholder perspectives and prioritise the optimal timing and setting to deliver a lifestyle intervention to improve long-term cardiometabolic health amongst women at high-risk of or diagnosed with a cardiometabolic pregnancy complication. An embedded mixed-methods research design was utilised. Facilitator-led workshops were used to prioritise the preferred timing (pregnancy or postpartum) and setting (hospital, general practice, community health program, maternal and child health services or online) for an intervention. Women with prior GDM, HDP, IUGR and/or PTB (n = 9), and research partners (n = 15) (obstetricians, endocrinologists, community health representatives, researchers, midwife, general practitioner, dietitian) participated. Workshops were audio recorded, transcribed verbatim and thematically analysed using template analysis. Online polls were used to assess participants preferred timing and setting for an intervention. Women preferred a postpartum intervention delivered online, whereas research partners preferred a pregnancy intervention delivered via hospital antenatal care. Both groups suggested commencing interventions during pregnancy and continuing postpartum. Participants recommended ensuring interventions consider healthcare system barriers to intervention delivery, equity and sustainment, as well as consumer-specific barriers to intervention engagement and lifestyle change during pregnancy and postpartum. Commencing patient-centred interventions during pregnancy and continuing postpartum should be considered to support continuity of care and improve health outcomes across both life stages for this high-risk group of women.

Cardiometabolic pregnancy complications (gestational diabetes mellitus (GDM), hypertensive disorders of pregnancy (HDP), intrauterine growth restriction (IUGR), preterm birth (PTB)) present a unique sex-specific risk factor for future cardiometabolic disease(1–5). Lifestyle modifications and healthful behaviour change (diet and physical activity), which can be supported by the delivery of evidence-based lifestyle interventions, are important factors in modifying risks of cardiometabolic conditions(2,6,7). Pregnancy and postpartum present unique windows of opportunity to intervene and prevent or delay the onset of cardiometabolic pregnancy complications and future cardiometabolic disease(2,8). Co-design considers the end-users wants, needs, preferences, characteristics and abilities throughout the entirety of the design process(9,10). Co-design processes engage women with lived experience alongside other key stakeholders including; community organisations, healthcare professionals, primary healthcare and health promotion experts14. In line with patient-centred care it offers the opportunity to design lifestyle interventions that are adapted to suit end-users, in the hope of increasing uptake, engagement, implementation success and sustainability(11). This study aims to co-design and explore stakeholders’ perspectives of the acceptability and feasibility of a lifestyle and screening intervention to reduce cardiometabolic risk amongst women at risk of or diagnosed with a cardiometabolic pregnancy complication. A descriptive qualitative research design was utilised. Two 2-hour co-design group workshops and a series of one-on-one semi-structured interviews were conducted with women with prior GDM, HDP, IUGR and/or PTB (n = 11), and research partners (obstetricians, endocrinologists, community health representatives, researchers, midwives, general practitioners, dietitians) (n = 14). Participants were provided with an overview of a potential lifestyle intervention, discussed the acceptability of each intervention component (outlined by the TIDieR framework; brief name, why, what, who provided, how, where, when and how much, tailoring, modifications, how well(12)), and the feasibility of implementation (outlined by the Theoretical Framework of Acceptability(13) and the APEASE criteria for intervention design(14)). Workshops and interviews were audio recorded, transcribed and analysed using template analysis. Analysis highlighted 10 key themes. Participants recommended the intervention is holistic, user-friendly, empowering, empathetic, patient-centred and culturally sensitive. Participants highlighted the importance of good risk communication, focusing on a positive, healthy pregnancy as opposed to risk reduction. Participants recommended providing additional resources and access to health services to complement intervention content. Participants suggested the intervention be delivered by female healthcare professionals from a range of cultural backgrounds with expertise in cardiometabolic pregnancy complications and postpartum management. Participants discussed the importance and value of the proposed intervention in filling what was perceived as a current healthcare gap for women at risk and diagnosed with cardiometabolic conditions during and following pregnancy. Engaging stakeholders to co-design an intervention that aligns with women’s and the healthcare system’s preferences, needs and priorities will support the development of an acceptable intervention for implementation in a real-world setting.

Microbial mineral weathering has been predominantly investigated at shallow depths in humid and tropical environments. Much less is understood about its role in the deeper subsurface of arid and semi-arid environments where microbial weathering is limited by the availability of water and energy sources for microbial metabolism. However, the deep subsurface in these climate zones may host a microbial community that thrives on weathering of iron (Fe)-bearing minerals that serve as electron donors or acceptors.

To investigate the role of microorganisms in weathering of Fe-bearing minerals in a dry climate, we recovered a >80 m deep weathering profile in a semi-arid region of the Chilean Coastal Cordillera. The bedrock is rich in Fe-bearing minerals (hornblende, biotite, chlorite, magnetite and hematite) but lacks detectable organic carbon. We evaluated the bioavailability of Fe(III)-bearing minerals that may serve as an electron acceptor for Fe(III)-reducing microorganisms. Using geochemical, mineralogical and cultivation-based methods, we found enhanced Fe bioavailability and more in vitro microbial Fe(III) reduction at increased depth. We obtained an Fe(III)-reducing enrichment culture from the deepest weathered rock found at 77 m depth. This enrichment culture is capable of reducing ferrihydrite (up to 0.6 mM d–1) using lactate or dihydrogen as an electron donor and grows at circumneutral pH. The main organism in the enrichment culture is the spore-forming Desulfotomaculum ruminis (abundance of 98.5%) as revealed by 16S rRNA gene amplicon sequencing.

Our findings provide evidence for a microbial contribution to the weathering of Fe-bearing minerals in semi-arid environments. While microorganisms are probably not contributing to the weathering of Fe(II)-bearing silicate minerals, they are most likely of importance regarding reductive dissolution of secondary weathering products. The Fe(III) reduction quantified in this weathering profile by the in situ microbial community suggests that microorganisms are active weathering agents in semi-arid climates.

Parasite biodiversity is underestimated or unknown in many regions, yet information on parasites is critical to understanding ecosystem structure and how this will change into the future. Understanding the diversity and role of parasites is especially important in regions exposed to anthropogenic pressures, such as aquatic ecosystems, as their interactions with other stressors can either exacerbate or mediate negative impacts. Water scarcity in the Brazilian semi-arid has led to a proliferation of reservoirs for human use. These artificial waterbodies host a diversity of taxa, including a large number of fish species; however, fish parasite diversity remains undocumented. This study investigated the parasitological diversity of fishes from reservoirs in the Paraíba and Mamanguape River basins in the Caatinga domain, Brazil – one of the most populated semi-arid regions worldwide. Eight reservoirs were studied, with fish sampled across the two phases of the hydrological cycle (dry and rainy seasons) using gillnets, cast nets, and trawl nets. Endo- and ecto-parasites were identified and enumerated, and parasitological indices (prevalence, intensity, and abundance) were calculated. In total, 1,170 individuals of 21 fish species were examined. Of these individuals, 42% were parasitized with at least one of 54 parasite taxa. We recorded 32 new geographical occurrences of parasites and 23 new fish-parasite interactions, expanding our understanding of ichthyoparasite diversity in the Brazilian semi-arid. Moving forward, it is important to develop knowledge around how anthropogenic changes (e.g., biological invasions, climate, and land use change) influence host-parasite structure and dynamics and ecosystem functioning in these ecosystems.

Rainfall is the main driving factor for soil-active herbicides, influencing their incorporation, leaching, and absorption. Studies were conducted to determine the effects of simulated rainfall and hexazinone application rates on giant smutgrass [Sporobolus indicus (L.) R. Br. var. pyramidalis (P. Beauv.) Veldkamp] control and the impacts of application timing and rates on S. indicus var. pyramidalis in the field. Greenhouse experiments were established in Florida between 2017 and 2018, comprising hexazinone application rates of 0.56 and 1.12 kg ai ha−1, and seven simulated rainfall accumulation volumes (0, 6, 12, 25, 50, 100, and 200 mm), distributed in a completely randomized design with four replicates and a non-treated control. Field experiments were conducted in a split-plot arrangement, wherein main plots were application timings at 1-wk intervals, subplots were two hexazinone application rates (0.56 and 1.12 kg ha−1) and a non-treated control, distributed in a randomized complete block design, with four replicates. In the greenhouse experiment, 49 and 92 mm were required to obtain 50% visual control and 35 and 82 mm to reduce biomass by 50% for hexazinone rates of 0.56 and 1.12 kg ai ha−1, respectively. Field experiments showed that hexazinone peak efficacy was from mid-June to mid-August when applications were followed by 10 to 75 mm of rainfall during the first 7 d after treatment. The recommended rate of hexazinone at 1.12 kg ai ha−1 should be applied, as it has an extended window of optimum application timing.