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International Max Planck Research School on Astrophysics at Ludwig Maximilians University Munich, Germany | 2 months ago
Are you looking for an outstanding environment to pursue a PhD in Astrophysics? Join one of Europe’s leading centers for astronomy and astrophysics and work alongside internationally recognized
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faculty and research staff. For a full list of department members and activities, see https://web.astro.princeton.edu/ . There are also strong research groups with interests in astrophysics at the
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Universidad Diego Portales | 2 months ago
Galactic astronomy, Extragalactic astronomy, Cosmology and Numerical Relativity. More information on our research and potential projects can be found here: https://astronomia.udp.cl/en/teaching/phd
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the connection between supermassive/massive black hole astrophysics and GW observations. Minimum Qualifications Must have completed all the requirements for a PhD. in Astronomy, Physics, Astrophysics
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: Postdoctoral Researcher in Time Domain Astrophysics Position Type: Faculty Location: Villanova, PA Recruitment Type: Internal/External Applicants Work Schedule: full-time/12-months Department: 186-Physics
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HUN-REN Research Centre For Astronomy and Earth Sciences | 2 months ago
and Earth Sciences (Budapest, Hungary) invites applications for a postdoctoral position in multimessenger high-energy astrophysics, as part of the newly formed Lendület ("Momentum") research group, the
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Postdoctoral Research Associate of Physics and Astronomy- Astrophysics University of Oklahoma Norman Campus: Dodge Family College of Arts and Sciences: Physics and Astronomy Location University of
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encompassed physics, chemistry, molecular spectroscopy and astrophysics. Dr. Luise Herzberg received her PhD in astrophysics in Germany in 1933. Dr. Herzberg worked at the NRC as a volunteer research
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encompassed physics, chemistry, molecular spectroscopy and astrophysics. Dr. Luise Herzberg received her PhD in astrophysics in Germany in 1933. Dr. Herzberg worked at the NRC as a volunteer research
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KU Leuven | 2 months ago
-driven modelling approach is envisioned, with the aim to calibrate tidal dissipation in binary evolution models of interacting dynamical rotating stars. Applicants with a PhD degree in astrophysics