Zanisi, L.; Huertas-Company, M.; Lanusse, F.; Bottrell, C.; Pillepich, A.; Nelson, D.; Rodriguez-Gomez, V.; Shankar, F.; Hernquist, L.; Dekel, A. et al.; Margalef-Bentabol, B.; Vogelsberger, M.; Primack, J.: A deep learning approach to test the small-scale galaxy morphology and its relationship with star formation activity in hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society 501 (3), S. 4359 - 4382 (2021)

Dodelson, S.; Schmidt, F.: Modern cosmology. Academic Press, Cambridge, Massachusetts, US (2021), 494 S.

Dodelson, S.; Schmidt, F.: Modern cosmology. Academic Press, Cambridge, Massachusetts, US (2021), 494 S.

Supermassive Black Hole feedback in early type galaxies (Proceedings of the International Astronomical Union, 15/s359). 356nd Symposium of the International Astronomical Union: Galaxy Evolution and Feedback Across Different Environments, Bento Gonçalves, Brazil, 02. März 2020 - 06. März 2020. Cambridge University Press, Cambridge, UK (2021)

Establishing the impact of powerful AGN on their host galaxies (Proceedings of the International Astronomical Union, 15/s359). 356nd Symposium of the International Astronomical Union: Galaxy Evolution and Feedback Across Different Environments, Bento Gonçalves, Brazil, 02. März 2020 - 06. März 2020. Cambridge University Press, Cambridge, UK (2021)

Propagation of cosmic rays and their secondaries in the intracluster medium (Proceedings of the International Astronomical Union, 15/s359). 356nd Symposium of the International Astronomical Union: Galaxy Evolution and Feedback Across Different Environments, Bento Gonçalves, Brazil, 02. März 2020 - 06. März 2020. Cambridge University Press, Cambridge, UK (2021)

Feedback from quasars: The prevalence and impact of radio jets (Proceedings of the International Astronomical Union, 15/s356). 356nd Symposium of the International Astronomical Union: Nuclear Activity in Galaxies Across Cosmic Time , Addis Ababa, Ethiopia, 07. Oktober 2019 - 11. Oktober 2019. Cambridge University Press, Cambridge, UK (2021)

Pillepich, A.; Nelson, D.; Springel, V.; Pakmor, R.; Hernquist, L.; Vogelsberger, M.; Weinberger, R.; Genel, S.; Marinacci, F.; Torrey, P. et al.; Naiman, J.: The TNG50 Simulation: Highly-resolved galaxies in a large cosmological volume to the present day. In: Transactions of the High Performance Computing Center, Stuttgart (HLRS) 2019, S. 5 - 22 (Hg. Nagel, W. E.; Kröner, D. H.). High Performance Computing in Science and Engineering '19, Stuttgart, Germany . (2021)

Arras, P. A.: Radio interferometry with information field theory. Dissertation, 171 S., Ludwig Maximilians Universität München, München, Germany (2021)

Ayromlou, M.: Physical processes that determine the clustering of different types of galaxies on large scales. Dissertation, 130 S., Ludwig Maximilians Universität München, München, Germany (2021)

Enzi, W.: Astrophysical probes of dark matter: opportunities and challenges from a strong gravitational lensing perspective. Dissertation, 112 S., Ludwig Maximilians Universität München, München, Germany (2021)

Frank, P. F.: Approximate inference in astronomy. Dissertation, 166 S., Ludwig Maximilians Universität München, München, Germany (2021)

Kuuttila, J.: The observational characteristics of accreting white dwarfs and their connection to type Ia supernovae. Dissertation, 88 S., Ludwig Maximilians Universität München, München, Germany (2021)

Rathjen, T.-E.: Simulating the multi-phase interstellar medium and galactic outflows. Dissertation, 112 S., Ludwig Maximilians Universität München, München, Germany (2021)

Ding, S.: Multi-frequency imaging of HydraA using RESOLVE. Master, 53 S., Ludwig Maximilians Universität München, München, Germany (2021)

Lujan Niemeyer, M.: Lyman-alpha halos around high-redshift lyman-alpha emitting galaxies. Master, 93 S., Ludwig Maximilians Universität München, München, Germany (2021)

Guerdi, M.: Hamiltonian Monte Carlo. Bachelor, 32 S., Ludwig Maximilians Universität München, München, Germany (2021)

Springel, V.; Haemmerle, H.; Depner, M.: Annual Report 2020. (2021), 76 S.