About

Massive galaxies are the first to form and the first to become quiescent, during a process called quenching in which the formation of new stars is shut down. Galaxy quenching is a key phase of galaxy evolution, but our physical understanding of it is still limited. In the Red Cardinal project we use the new James Webb Space Telescope, together with other space- and ground-based facilities, to investigate the stars, gas, dust, and supermassive black holes in distant galaxies, with the goal of understanding the key physical processes responsible for galaxy quenching.

The word cloud on the left was produced by NASA ADS using the Red Cardinal publications.

The Team

  • Sirio Belli (PI; Associate Professor) ORCID iD icon https://orcid.org/0000-0002-5615-6018
  • Letizia Bugiani (3rd-year PhD student)
  • Amir H. Khoram (3rd-year PhD student) ORCID iD icon https://orcid.org/0009-0009-6563-282X
  • Matteo Sapori (2nd-year PhD student)
  • Caterina Liboni (1st-year PhD student)

  • Additionally, we collaborate with a wide network of international colleagues. The graph on the right shows the author network for the Red Cardinal publications (from NASA ADS).

Publications

Here are some of the publications produced by Red Cardinal; the full list is available on the NASA ADS.