The role of Accelerometry in the Conservation of two Coastal Marine Vertebrates

This thesis advances the understanding of the spatial and behavioural ecology of two endangered species, basking sharks (Cetorhinus maximus) and green turtles (Chelonia mydas) at their coastal foraging sites while highlighting the pragmatic application of biologging technology in informing conservation. Chapter 1 of this thesis is a general introduction to tracking technologies, covering how the advancements of biologging have revolutionised the field of ecology, with an emphasis on how accelerometers can be used in conservation. Chapters 2 explores the use of accelerometers on three basking sharks in the western Scottish Isles to understand their fine-scale behaviour. I present early evidence of potential behavioural lateralisation, and the first direct records of 67 breaches over 41 days, with sharks breaching on average twice a day, both during night and day and increasing energy expenditure by at least 30 times to breach. While the function of breaching remains unclear, owing to its energetic cost, breaching is likely to have an important fitness function. In Chapter 3, accelerometers were deployed on 16 juvenile green turtles in The Bahamas to investigate the behavioural and energetic costs of translocation. Turtles rehomed in as little as 15 hours following translocation of 4 km and allocated twice as much time to energetically demanding behaviours compared to resident turtles at their foraging grounds, highlighting that translocation is not a suitable conservation practice for sea turtles. Chapter 4 summarises both data chapters and discusses how their findings provide further evidence of how tracking technologies can be ideal tools for conservation practitioners by monitoring animal movement, behaviour and health as well as assisting with the designation of protected areas by identifying important life history events. Chapter 4 concludes on the challenges and limitations of the thesis as well as the future directions in the use of tracking technologies in conservation ecology

Effector-mediated partial and nonhost disease resistance in wheat

Plants are considered to have three major forms of resistance against pathogen infection. The first is ‘non host resistance’, which operates broadly at the species level, meaning all members of a plant species generally resist all members of the would-be pathogen species. The other two systems operate at the ‘host’ level. ‘Qualitative host resistance’ is seen when an individual plant cultivar (or genotype)completely resists attempted attack by an individual pathogen strain, whilst ‘partial resistance’ is when a plant cannot completely defend itself. Each of these systems have some underlying molecular principles which will be outlined later. In this issue of New Phytologist, Meile et al.(2023; pp. 1562–1577) describe a novel mechanism by which both partial and non host resistance can be achieved in wheat facing the fungal pathogen Zymoseptoria tritici and its closely related species

Previous bottlenecks and future solutions to dissecting the Zymoseptoria tritici -wheat host-pathogen interaction

AbstractZymoseptoria tritici (previously Mycosphaerella graminicola, teleomorph, Septoria tritici, anamorph) causes Septoria tritici blotch, one of the most economically important diseases of wheat (Triticum aestivum). The host pathogenic interaction, as currently understood, is intriguing, and may distinguish Z. tritici from many of the current models for plant pathogenic fungi. Many important questions remain which require a deeper understanding including; the nature and biological significance of the characteristic long latent periods of symptomless plant infection; how/why the fungus then effectively transitions from this to cause disease and reproduce? Elements of this transition currently resemble a putative “hijack” on plant defence but how is Z. tritici able to do this without any form of plant cell penetration? This commentary provides a summary of the recent history of research into the host-pathogen interaction, whilst highlighting some of the challenges going forwards, which will be faced by improved technologies and a growing research community

Ingot Hard Red Spring Wheat

This bulletin provides a brief overview of Ingot Hard Red Spring Wheat. Information regarding its origin, disease resistance, and other traits is provided

Oxen Hard Red Spring Wheat

This bulletin provides a brief overview of Oxen Hard Red Spring Wheat. Information regarding its origin, disease resistance, and other traits is provided

Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy

Numerical studies indicate that uncertainties in the treatment of baryonic physics can affect predictions for shear power spectra at a level that is significant for forthcoming surveys such as DES, SNAP, and LSST. Correspondingly, we show that baryonic effects can significantly bias dark energy parameter measurements. Eliminating such biases by neglecting information in multipoles beyond several hundred leads to weaker parameter constraints by a factor of approximately 2 to 3 compared with using information out to multipoles of several thousand. Fortunately, the same numerical studies that explore the influence of baryons indicate that they primarily affect power spectra by altering halo structure through the relation between halo mass and mean effective halo concentration. We explore the ability of future weak lensing surveys to constrain both the internal structures of halos and the properties of the dark energy simultaneously as a first step toward self calibrating for the physics of baryons. This greatly reduces parameter biases and no parameter constraint is degraded by more than 40% in the case of LSST or 30% in the cases of SNAP or DES. Modest prior knowledge of the halo concentration relation greatly improves even these forecasts. Additionally, we find that these surveys can constrain effective halo concentrations near m~10^14 Msun/h and z~0.2 to better than 10% with shear power spectra alone. These results suggest that inferring dark energy parameters with measurements of shear power spectra can be made robust to baryonic effects and may simultaneously be competitive with other methods to inform models of galaxy formation. (Abridged)Comment: 18 pages, 11 figures. Minor changes reflecting referee's comments. Results and conclusions unchanged. Accepted for publication in Physical Review