Traditional foods are increasingly being incorporated into modern diets. This is largely driven by consumers seeking alternative food sources that have superior nutritional and functional properties. Within Australia, Aboriginal and Torres Strait Islander peoples are looking to develop their traditional foods for commercial markets. However, supporting evidence to suggest these foods are safe for consumption within the wider general population is limited. At the 2022 NSA conference a keynote presentation titled ‘Decolonising food regulatory frameworks to facilitate First Peoples food sovereignty’ was presented. This presentation was followed by a manuscript titled ‘Decolonising food regulatory frameworks: Importance of recognising traditional culture when assessing dietary safety of traditional foods’, which was published in the conference proceedings journal(1). These pieces examined the current regulatory frameworks that are used to assess traditional foods and proposed a way forward that would allow Traditional Custodians to successfully develop their foods for modern markets. Building upon the previously highlighted works, this presentation will showcase best practice Indigenous engagement and collaboration principles in the development of traditionally used food products. To achieve this, we collaborated with a collective of Gamilaraay peoples who are looking to reignite their traditional grain practices and develop grain-based food products. To meet the current food safety regulatory requirements, we needed to understand how this grain would fit into modern diets, which included understanding the history of use, elucidating the nutritional and functional properties that can be attributed to the grain, and developing a safety dossier(2) so that the Traditional Custodians can confidently take their product to market. To aid the Traditional Custodians in performing their due diligence, we have systemically analysed the dietary safety of the selected native grain and compared it side-by-side with commonly consumed wheat in a range of in vitro bioassays and chemical analyses. From a food safety perspective, we show that the native grain is equivalent to commonly consumed wheat. The native grain has been shown to be no more toxic than wheat within our biological screening systems. Chemical analysis showed that the level of contaminants are below tolerable limits, and we were not able to identify any chemical classes of concern. Our initial findings support the history of safe use and suggest that the tested native grain species would be no less safe than commonly consumed wheat. This risk assessment and previously published nutritional study(3) provides an overall indication that the grain is nutritionally superior and viable for commercial development. The learnings from this project can direct the future risk assessment of traditional foods and therefore facilitate the safe market access of a broader range of traditionally used foods. Importantly, the methods presented are culturally safe and financially viable for the small businesses hoping to enter the market.

The optimal management of bacteriuria/pyuria of clinically undetermined significance (BPCUS) is unknown. Among 220 emergency department patients prescribed antibiotics for BPCUS, we found frequent readmissions, which were mitigated by outpatient follow-up visits. Observation and follow-up for an unknown diagnosis should be emphasized over antibiotics due to high likelihood of readmissions.

Anguillicoloides crassus is an invasive nematode parasite of the critically endangered European eel, Anguilla anguilla, and possibly one of the primary drivers of eel population collapse, impacting many features of eel physiology and life history. Early detection of the parasite is vital to limit the spread of A. crassus, to assess its potential impact on spawning biomass. However accurate diagnosis of infection could only be achieved via necropsy. To support eel fisheries management we developed a rapid, non-lethal, minimally invasive and in situ DNA-based method to infer the presence of the parasite in the swim bladder. Screening of 131 wild eels was undertaken between 2017 and 2019 in Ireland and UK to validate the procedure. DNA extractions and PCR were conducted using both a Qiagen Stool kit and in situ using Whatman qualitative filter paper No1 and a miniPCR DNA Discovery-System™. Primers were specifically designed to target the cytochrome oxidase mtDNA gene region and in situ extraction and amplification takes approximately 3 h for up to 16 individuals. Our in-situ diagnostic procedure demonstrated positive predictive values at 96% and negative predictive values at 87% by comparison to necropsy data. Our method could be a valuable tool in the hands of fisheries managers to enable infection control and help protect this iconic but critically endangered species.

In this era of spatially resolved observations of planet-forming disks with Atacama Large Millimeter Array (ALMA) and large ground-based telescopes such as the Very Large Telescope (VLT), Keck, and Subaru, we still lack statistically relevant information on the quantity and composition of the material that is building the planets, such as the total disk gas mass, the ice content of dust, and the state of water in planetesimals. SPace Infrared telescope for Cosmology and Astrophysics (SPICA) is an infrared space mission concept developed jointly by Japan Aerospace Exploration Agency (JAXA) and European Space Agency (ESA) to address these questions. The key unique capabilities of SPICA that enable this research are (1) the wide spectral coverage $10{-}220\,\mu\mathrm{m}$ , (2) the high line detection sensitivity of $(1{-}2) \times 10^{-19}\,\mathrm{W\,m}^{-2}$ with $R \sim 2\,000{-}5\,000$ in the far-IR (SAFARI), and $10^{-20}\,\mathrm{W\,m}^{-2}$ with $R \sim 29\,000$ in the mid-IR (SPICA Mid-infrared Instrument (SMI), spectrally resolving line profiles), (3) the high far-IR continuum sensitivity of 0.45 mJy (SAFARI), and (4) the observing efficiency for point source surveys. This paper details how mid- to far-IR infrared spectra will be unique in measuring the gas masses and water/ice content of disks and how these quantities evolve during the planet-forming period. These observations will clarify the crucial transition when disks exhaust their primordial gas and further planet formation requires secondary gas produced from planetesimals. The high spectral resolution mid-IR is also unique for determining the location of the snowline dividing the rocky and icy mass reservoirs within the disk and how the divide evolves during the build-up of planetary systems. Infrared spectroscopy (mid- to far-IR) of key solid-state bands is crucial for assessing whether extensive radial mixing, which is part of our Solar System history, is a general process occurring in most planetary systems and whether extrasolar planetesimals are similar to our Solar System comets/asteroids. We demonstrate that the SPICA mission concept would allow us to achieve the above ambitious science goals through large surveys of several hundred disks within $\sim\!2.5$ months of observing time.

Carbon-rich dust is known to form in the atmosphere of the semiregular variable star R Sculptoris. Such stardust, as well as the molecules and gas produced during the lifetime of the star, will be spread into the Galaxy via the mass-loss process. Probing this process is crucial to understand the chemical enrichment of the Galaxy. R Scl was observed using the ESO/VLTI MATISSE instrument in December 2018. Here we show the first images of the star between 3 and 10 R*. Using the complementary MIRA 3D image reconstruction and the RHAPSODY 1D intensity profile reconstruction code, we reveal the location of molecules and dust in the close environment of the star. Indeed, the C2H2 and HCN molecules are spatially located between 1 and 3.4 R* which is much closer to the star than the location of the dust. The R Scl spectrum is fitted by molecules and a dust mixture of 90% of amorphous carbon and 10% of silicone carbide. The inner boundary of the dust envelope is estimated by DUSTY at about 4.6 R*. We derive a mass-loss rate of 1.2 ± 0.4 × 10−6M⊙ yr−1however no clear SiC forming region has been detected in the MATISSE data.