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: The successful candidate will pursue research in the following fields: Spectroscopic analysis of PG1159 stars to further our understanding of the so-called Nitrogen dichotomy. Pulsational analysis of pre-white
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be carried out in close collaboration with the ERC Synergy project ECOGAL (http://www.ecogal.eu/ ), of which the applicant will be a member. Currently the star formation group has three PhD students
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nature by identifying the possible processes able to synthesize them. Though the origin of most of the nuclides lighter than iron through the various hydrostatic and explosive burning stages in stars is
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of extension up to 4 years to lead the efforts to bring new constraints on stellar structure and evolution of massive stars using large observational campaigns. A 2 + 2-year PhD position building numerical 3D
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on topics including molecular clouds and star formation. Candidates with experience in machine-learning and magnetic field observation/simulation are particularly welcome to apply. Experiences with (sub-)mm
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observations. Preference will be given to excellent researchers, with experience in radial velocity detection of planets around active stars. Since postdoctoral fellows in the group assist with MSc and PhD
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the satellite dwarf galaxies of the Milky Way, from their formation to their disruption, by exploiting spectra of individual stars in these systems. This will be done both through participation in smaller
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([email protected] ): theoretical physics, gravitation, econophysics Cristián Cortés ([email protected] ): stellar astrophysics, variable stars, chemical abundances Jorge Pinochet ([email protected]
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performance indicators for multi-objective evolutionary algorithms. We are looking for a promising young researcher, who has the PhD completed before the contract stars. PhD degree in mathematics
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access to data and observational facilities available to the BlackGEM survey consortium and will be involved in the large international collaborations of Transients and Variable Stars Science (LSST), and