All Outputs (7)

Embedded software of the KM3NeT central logic board (2023)
Journal Article
Aiello, S., Albert, A., Alves Garre, S., Aly, Z., Ambrosone, A., Ameli, F., …Zywucka, N. (2024). Embedded software of the KM3NeT central logic board. Computer Physics Communications, 296, Article 109036. https://doi.org/10.1016/j.cpc.2023.109036

The KM3NeT Collaboration is building and operating two deep sea neutrino telescopes at the bottom of the Mediterranean Sea. The telescopes consist of latices of photomultiplier tubes housed in pressure-resistant glass spheres, called digital optical... Read More about Embedded software of the KM3NeT central logic board.

The limitations of Rankine-Hugoniot jump conditions for estimating infall velocity during a minor galaxy cluster merger. (2023)
Thesis
Huntley, M. L.-R. The limitations of Rankine-Hugoniot jump conditions for estimating infall velocity during a minor galaxy cluster merger. (Thesis). University of Hull. https://hull-repository.worktribe.com/output/4425365

Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields (2023)
Journal Article
Keegans, J. D., Pignatari, M., Stancliffe, R. J., Travaglio, C., Jones, S., Gibson, B. K., …Few, G. (2023). Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields. Astrophysical Journal Supplement, 268(1), Article 8. https://doi.org/10.3847/1538-4365/ace102

Type Ia supernova explosions (SN Ia) are fundamental sources of elements for the chemical evolution of galaxies. They efficiently produce intermediate-mass (with Z between 11 and 20) and iron group elements - for example, about 70% of the solar iron... Read More about Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields.

On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation (2023)
Journal Article
Singh, A., Park, C., Choi, E., Kim, J., Jun, H., Gibson, B. K., …Snaith, O. (2023). On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation. The Astrophysical journal, 953(1), Article 64. https://doi.org/10.3847/1538-4357/acdd6b

We use the Horizon Run 5 cosmological simulation to study the effect of galaxy intrinsic properties and the local environment on active galactic nuclei (AGNs) characterized by their threshold of the accretion rate. We select galaxies in the stellar m... Read More about On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation.

The chemical evolution of the solar neighbourhood for planet-hosting stars (2023)
Journal Article
Pignatari, M., Trueman, T. C., Womack, K. A., Gibson, B. K., Côte, B., Turrini, D., …Lugaro, M. (2023). The chemical evolution of the solar neighbourhood for planet-hosting stars. Monthly notices of the Royal Astronomical Society, 524(4), 6295-6330. https://doi.org/10.1093/mnras/stad2167

Theoretical physical-chemical models for the formation of planetary systems depend on data quality for the Sun's composition, that of stars in the solar neighbourhood, and of the estimated 'pristine' compositions for stellar systems. The effective sc... Read More about The chemical evolution of the solar neighbourhood for planet-hosting stars.

Modelling the Chemical Evolution of the Milky Way: Short-lived Radioactive Isotopes from AGB Stars and the impact of SNe Ia (2023)
Thesis
Trueman, T. Modelling the Chemical Evolution of the Milky Way: Short-lived Radioactive Isotopes from AGB Stars and the impact of SNe Ia. (Thesis). University of Hull. https://hull-repository.worktribe.com/output/4366004

Inhomogeneous Galactic chemical evolution: modelling ultra-faint dwarf galaxies of the Large Magellanic Cloud (2023)
Journal Article
Alexander, R. K., Vincenzo, F., Ji, A. P., Richstein, H., Jordan, C. J., & Gibson, B. K. (2023). Inhomogeneous Galactic chemical evolution: modelling ultra-faint dwarf galaxies of the Large Magellanic Cloud. Monthly notices of the Royal Astronomical Society, 522(4), 5415-5433. https://doi.org/10.1093/mnras/stad1312

Ultra-faint dwarf galaxies (UFDs) are among the oldest and most metal-poor galaxies in the cosmos, observed to contain no gas and a high dark matter mass fraction. Understanding the chemical abundance dispersion in such extreme environments could she... Read More about Inhomogeneous Galactic chemical evolution: modelling ultra-faint dwarf galaxies of the Large Magellanic Cloud.