About Me

Hello everyone and welcome to my personal webpage. I am Julien Drevon, and working for the European Southern Observatory (ESO) with a Fellow astronomer position since November 1st 2023.
Born the 2nd of November 1997 in Cannes (France), I have made my bachelor degrees and my master degree at the Universite Cote d'Azur at Nice (France). In October 2023, I obtained my PhD thesis under the supervision of Pierre CRUZALEBES and Florentin MILLOUR with the title: "Exploitation of the VLTI/MATISSE instrument: imagery of evolved stars." In addition to all the stellar evolution theory skills that I have learned during my PhD, I also dealed with interferometric data using the VLTI/MATISSE instrument to understand how to use them in order to locate the molecular and dust formation regions in the vicinity of evolved stars.
During my 2nd year of my PhD, I have been granted a studentship position at ESO Chile under the supervision of Claudia Paladini to develop new skills on stellar wind and dust formation around AGB stars.
After my PhD I moved to ESO-Chile for a reasearch fellowship position with duties as night astronomer (80 nights per year) at the Paranal Observatory for VLTI. In addition to my night astronomer position, I am also instrument fellow for the VLTI/MATISSE instrument and working on instrumental projects for the observatory. Recently I coded a new quality check script for the VLTI/MATISSE instrument to improve the robusteness of the grading procedure.
All of my skills can be divided into four different categories: i) current theoretical knowledge on stellar evolution and dust formation around evolved stars, ii) knowledge of infrared interferometric instruments, iii) calibration, processing, and analysis of interferometric data, and iv) programming and the creation of new codes for processing and analyzing interferometric data. My skills are currently being used to analyze data from the VLTI instruments and reconstruct images of structures located at the surface and in the close environments (a few stellar radii) within the molecular and dust envelopes of evolved stars. My goal is to identify the conditions and regions of dust and molecule formation to better constrain the mass-loss phenomenon and improve our understanding of the dust formation process.
Scientific keywords: evolved stars, AGB, red supergiants, dust formation, stellar wind, molecules, convection cells, photosphere, circumstellar envelope.
Technical keywords: infrared, interferometry, VLTI, image reconstruction, machine learning, big data, coding, Python, statistics, photometry, spectroscopy.