معرفی
Professor Peter Schilke is a distinguished astrophysicist at the University of Cologne's Institute of Physics I, where he has been faculty since March 2009. He serves as chair of the Bachelor of Science Examination Board and leads an active research group focused on high-mass star formation and astrochemistry. His work involves advanced observational techniques across multiple wavelengths and sophisticated modeling approaches.
- PhD from University of Bonn (1992)
- Research Fellow at Caltech (1992-1995)
- Postdoc at I. Physikalisches Institut (1995-1997)
- Scientist at Max-Planck-Institut for Radioastronomy (1997-2009)
Professor Schilke's research focuses on the formation processes of high-mass stars, astrochemistry, and the evolution of molecular clouds. His work particularly emphasizes the modeling of observational data to understand physical and chemical processes in star-forming regions. He investigates how material is transported from large-scale molecular clouds to dense cores, how feedback mechanisms from newly-born stars affect this process, and how chemistry evolves from the diffuse interstellar medium to dense star-forming regions. His group has expanded studies to include clusters surrounding high-mass stars and extragalactic star formation in the Large Magellanic Cloud.
Analysis of his recent publications reveals a strong focus on large-scale observational programs, particularly the ALMAGAL survey using ALMA to study high-mass protocluster formation across the Galaxy. His work combines observations from multiple facilities including ALMA, APEX, IRAM instruments, SOFIA, and SMA. The research spans both observational and computational approaches, with significant emphasis on developing software tools for data analysis and modeling.
- Albertus-Magnus teaching award in physics (2020)
Professor Schilke actively mentors PhD students, with current advisees including Akash Gupta, Han-Tsung Lee, and Eleonore Rodrigues da Costa, among others. He has successfully supervised recent PhD graduates including Fanyi Meng, Mahya Sadaghiani, and Andreas Schwörer. His research is supported by multiple significant grants, including leadership of Project C3 in the SFB 956, involvement in projects A4 and A6, and participation in the ALMAGAL large program. He previously served as co-I of Herschel/HIFI and was involved in the HEXOS and CHESS key programs.
His research group develops and maintains several important astronomical software packages including STATCONT for continuum level determination, MAGIX for model optimization, and XCLASS for spectral line analysis. The group actively participates in major observational campaigns using ALMA, planning for CCAT-prime, and analyzing data from previous missions like Herschel. They maintain strong collaborations with international partners through projects like the SFB 956 and various ALMA committees.
