| The relation between galaxy morphology and colour in the EAGLE simulation CA Correa, J Schaye, B Clauwens, RG Bower, RA Crain, M Schaller, ... Monthly Notices of the Royal Astronomical Society: Letters 472 (1), L45-L49, 2017 | 98 | 2017 |
| The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE ACR Thob, RA Crain, IG McCarthy, M Schaller, CDP Lagos, J Schaye, ... Monthly Notices of the Royal Astronomical Society 485 (1), 972-987, 2019 | 88 | 2019 |
| The new semi-analytic code GalICS 2.0–reproducing the galaxy stellar mass function and the Tully–Fisher relation simultaneously A Cattaneo, J Blaizot, JEG Devriendt, GA Mamon, E Tollet, A Dekel, ... Monthly Notices of the Royal Astronomical Society 471 (2), 1401-1427, 2017 | 38 | 2017 |
| Generating synthetic star catalogs from simulated data for next-gen observatories with py-ananke ACR Thob, RE Sanderson, AP Eden, F Nikakhtar, N Panithanpaisal, ... arXiv preprint arXiv:2312.02268, 2023 | | 2023 |
| Resolved Stars in Nearby Galaxies with the HLWAS W Benjamin, K McQuinn, R Sanderson, A Thob, E Bell, K Johnston, ... | | 2023 |
| Generating mock Euclid and Roman surveys of stellar halos of simulated nearby galaxies using the py-ananke pipeline A Thob European Astronomical Society Annual Meeting 2023, 2023 | | 2023 |
| RomAndromeda: The Roman Survey of the Andromeda Halo A Dey, J Najita, C Filion, JJ Han, S Pearson, R Wyse, ACR Thob, ... arXiv preprint arXiv:2306.12302, 2023 | | 2023 |
| Finding extragalactic self-obscured massive evolved stars for the era of Webb and Roman A Thob American Astronomical Society Meeting #241 55 (2), 452.06, 2023 | | 2023 |
| The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in simulated galaxies ACR Thob PQDT-Global, 2019 | | 2019 |
| The relationship between the morphology and kinematics of EAGLE galaxies ACR Thob, RA Crain, IG McCarthy European Week of Astronomy and Space Science 2018, 2018 | | 2018 |
