Please be advised that two PhD thesis are available at INAF – IASF Milano for the PhD program in Physics, Astrophysics and Applied Physics at the University of Milan. Potentially interested candidates are encouraged to contact the relevant contacts.
Galaxy Evolution and AGN Across Cosmic Time with Next-Generation Spectroscopic Surveys
This PhD project focuses on understanding how galaxies assemble their stellar mass across cosmic time and assessing the impact of Active Galactic Nuclei (AGN) on star formation and galaxy evolution. The candidate will address these questions through the analysis of large spectroscopic survey datasets spanning a broad redshift range, from the local Universe to the epoch of peak cosmic star formation. A central component of the project will be the exploitation of data from MOONRISE, one of the flagship extragalactic spectroscopic surveys with the new VLT/MOONS facility, starting in early 2027. MOONRISE will provide an unprecedented near-infrared spectroscopic dataset to investigate galaxy assembly, stellar populations, chemical enrichment, black holes fundamental properties and their connection with the host galaxy. Depending on the candidate’s interests, the project may also incorporate complementary data from Euclid and previous spectroscopic surveys, as well as opportunities to contribute to preparatory activities for future facilities such as MOSAIC on the ELT. The candidate will join a dynamic and internationally active team involved in leading roles in major collaborations including MOONS, Euclid, and MOSAIC, gaining direct experience in large survey science and advanced data analysis.
Contact person: Adriana Gargiulo, Susanna Bisogni, Chiara Mancini, Giustina Vietri, Marco Scodeggio
Astrophysics of Galaxy Clusters and Groups
This PhD program offers the opportunity to investigate the most massive gravitationally bound structures in the Universe, focusing on the complex physics of the Intracluster and Intragroup Medium. Candidates can choose to specialize in one or more core research areas, including the thermodynamical properties of the diffuse plasma, the metal enrichment history of massive halos, or the impact of non-thermal processes. Projects may also focus on precise mass measurements and the calibration of scaling relations, which are vital for constraining cosmological models. Furthermore, students could contribute to the next generation of X-ray missions by developing innovative analysis techniques and strategies to mitigate instrumental background, ensuring high-sensitivity science for future observatories. This program bridges fundamental plasma physics with cutting-edge observational cosmology and mission-driven science.
Contact persons: Mariachiara Rossetti, Fabio Gastaldello, Lorenzo Lovisari, Silvano Molendi, Simona Ghizzardi