The TOS group is a research group that aims to understand the physical processes that determine the structure and evolution of stars using asteroseismology – the study of the internal structures of stars through their global oscillations. The focus is on solar-like oscillators, i.e. low-mass main-sequence stars, subgiants and red-giant stars that possess oscillations similar to those present in the Sun.
We are seeking a highly motivated scientist to join the TOS group at HITS as a post-doctoral research associate as soon as possible. The successful candidate will work on a project to further understand the internal structure of red-giant stars using asteroseismology. The project will involve the analysis of both observational data, as well as synthetic stellar models to understand what the observed phenomena means in terms of the underlying structure of a star. The focus will be on the analysis and interpretation of the mixed-dipole modes to investigate the conditions in the deep layers of these stars.
Candidates at the post-doctoral level should possess a PhD Degree or equivalent qualification in physics, astrophysics, math, computer science or a related discipline and preferably have experience in asteroseismology.
Applications need to be submitted by (30.11.2020) including:
Inquiries should be addressed to Prof.dr.ir. Saskia Hekker: firstname.lastname@example.org
HITS offers a first-class research environment with outstanding computational resources and is embedded within the vibrant Heidelberg astronomical community that includes the Center for Astronomy of Heidelberg University and two Max Planck Institutes.
A generous research budget is available as well as a competitive salary and benefits package.
For more information regarding working at HITS see our Website: Working at HITS