Andreea Font

1. High-resolution synthetic UV–submm images for Milky Way-mass simulated galaxies from the ARTEMIS project, Camps, P., Kapoor, A. U., Trcka, A., Font, A. S., McCarthy, I. G., Trayford, J., Baes, M., 2022, MNRAS, 512, 2728 (pdf).

 

2. Merger-induced galaxy transformations in the ARTEMIS simulations, Dillamore, A. M., Belokurov, V., Font, A. S., McCarthy, I. G., MNRAS, in press (pdf)

​

3. Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations,

Font, A.S., McCarthy, I. G., Belokurov, V., Brown, S. T, Stafford, S. G., 2022, MNRAS, 511, 1544 (pdf)

​

4. Towards a universal model for the density profiles of dark matter haloes, Brown, S. T., McCarthy, I. G., Stafford, S. G., Font, A. S., 2022, MNRAS, 509, 5685 (pdf).

​

5. The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum, Acuto, A., McCarthy, I. G., Kwan, J., Salcido Negrete, J., Stafford, S. G., Font, A. S., 2021, MNRAS, 508, 3519 (pdf).

​

6. Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys? Stafford, S. G., McCarthy, I. G., Kwan, J., Brown, S. T., Font, A. S., Robertson, A., 2021, MNRAS, 508, 3519 (pdf)

​

7. Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?

Font, A.S., McCarthy, I. G., Belokurov, V., 2021, MNRAS, 416, 2802 (pdf).

​

​