Qualifications
- PhD / DPhil (Leiden university)
Summary
I was appointed as a Lecturer in the Centre for Data Science, Artificial Intelligence and Modelling (DAIM) and the E. A. Milne Centre for Astrophysics at the University of Hull in November 2022.
Previously, I was a Postdoctoral Research Associate and Teaching Fellow at the Institute for Computational Cosmology, Durham University (2018 - 2022), and a Lindheimer postdoctoral fellow at Northwestern University (2016 - 2018). Prior to that, I completed my Ph.D. in Astrophysics at the University of Leiden under the supervision of Prof. Joop Schaye (2011 - 2015).
Book Chapter
The interplay between dust and radiation
Richings, A. (2024). The interplay between dust and radiation. In S. Bovino, & T. Grassi (Eds.), Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations (157-188). Elsevier. https://doi.org/10.1016/B978-0-32-391746-9.00015-8
Journal Article
Tests of subgrid models for star formation using simulations of isolated disc galaxies
Nobels, F. S. J., Schaye, J., Schaller, M., Ploeckinger, S., Chaikin, E., & Richings, A. J. (2024). Tests of subgrid models for star formation using simulations of isolated disc galaxies. Monthly notices of the Royal Astronomical Society, 532(3), 3299-3321. https://doi.org/10.1093/mnras/stae1390
Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry
Thompson, O. A., Richings, A. J., Gibson, B. K., Faucher-Giguère, C. A., Feldmann, R., & Hayward, C. C. (2024). Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry. Monthly notices of the Royal Astronomical Society, 532(2), 1948-1965. https://doi.org/10.1093/mnras/stae1486
Dense stellar clump formation driven by strong quasar winds in the FIRE cosmological hydrodynamic simulations
Mercedes-Feliz, J., Anglés-Alcázar, D., Oh, B. K., Hayward, C. C., Cochrane, R. K., Richings, A. J., Faucher-Giguère, C. A., Wellons, S., Terrazas, B. A., Moreno, J., Su, K. Y., & Hopkins, P. F. (2024). Dense stellar clump formation driven by strong quasar winds in the FIRE cosmological hydrodynamic simulations. Monthly notices of the Royal Astronomical Society, 530(3), 2795-2809. https://doi.org/10.1093/mnras/stae1021
158 μm emission as an indicator of galaxy star formation rate
Liang, L., Feldmann, R., Murray, N., Narayanan, D., Hayward, C. C., Angles-Alcázar, D., Bassini, L., Richings, A. J., Faucher-Giguère, C. A., Chung, D. T., Chan, J. Y., Tolgay, D., Çatmabacak, O., Kereš, D., & Hopkins, P. F. (2024). 158 μm emission as an indicator of galaxy star formation rate. Monthly notices of the Royal Astronomical Society, 528(1), 499-541. https://doi.org/10.1093/mnras/stad3792