Stefano Andreon Homepage

I am first astronomer of INAF-Osservatorio Astronomico di Brera, President of the Astroinformatics and Astrostatistics Commission of the International Astronomical Union, Vice-President of the International Astrostatistics Association, chair of the IAU-IAA Astrostatistics and Astroinformatics seminar series, director of the INAF (summer) Astrostatistics school, and Honorary professor of the Shandong University.

My main interest is understanding how clusters of galaxies and galaxies in clusters evolve from an observational point of view and using Bayesian methods that I teach (so far at 14 universities spread in 7 countries). My top three most cited papers address the mass dependency and scatter of the stellar and gas fractions, the scaling between richness and mass, and the evolution of faint galaxies on the red-sequence. I discovered the most distant galaxy cluster for over a decade, JKCS041 at z=1.803 (currently the second most distant). I was one of the first astronomers using artificial intelligence tools (neural networks, self organizing maps) for photometric redshift and object detection at the end of the 90's and, starting from 2005, bayesian methods for many astrophysical applications (luminosity and mass function, velocity dispersion, quenched fraction, galaxy and cluster scaling relations, x-ray and optical analysis of galaxy clusters, etc). I'm lead author of Bayesian Methods for the Physical Sciences book. I'm presently deeply involved with the Euclid mission (awarded Euclid Builder status in 2023 for "extraordinary efforts on activity critical to the success of Euclid" mission). As a Euclid team member, I was awarded the 2024 Space Achievement Award. In 2016, I was awarded the status of  IAA fellow. Listed in the Italian Top Scientists and in the 2023 list of Highly Cited Researchers by Elsevier.

My data science interests can be found here.

In the past, I was deeply involved with the VIDEO survey, and with its successor, VEILS. Earlier, I was at INAF-Osservatorio Astronomico di Capodimonte, and I taught information science at the Milan University. I was a member of the XMM-LSS project, where I lead the (cluster) identification working group, and I was PI of the VST-OAC survey.
cover of Bayesian Methods For the Physical Sciences
My latest book

true color image of the most distant cluster known
The redshift-holder cluster of galaxies JKCS041 at z=1.803 I co-discovered