School of Humanities and Sciences
Showing 81-90 of 426 Results
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Roberta Leonie Claude Fischli
Postdoctoral Scholar, Political Science
BioRoberta Fischli is a postdoctoral scholar in the Department of Political Science at Stanford University. Her research focuses on the social and political impact of artificial intelligence (AI), with a particular focus on how novel AI systems can promote personal freedom and democracy.
Roberta was previously a Visiting Faculty Researcher at Google, where she worked on AI agents and value alignment. Previous research appointments include the University of California Berkeley, Georgetown University, and the University of St. Gallen. She is a research affiliate at the Machine Intelligence and Normative Theory (MINT) Lab at Australian National University, led by Seth Lazar.
Roberta holds a PhD (summa cum laude) in International Affairs and Political Economy from the University of St. Gallen. Her dissertation monograph "Freedom after Algorithms" investigates the changing role of freedom in the digital age. Her research has appeared in Perspectives on Politics, the European Journal of Political Theory, and History of Political Thought, among others. Roberta also works as a freelance journalist. -
Philipp Frank
Postdoctoral Scholar, Physics
BioPhilipp Frank is an Astronomy and Machine Learning researcher who is developing and applying statistical and ai methods to help deepen our understanding of the structure of the Milky Way and the Cosmos. He did his PhD and a followup Postdoc in Germany at Ludwig Maximilians University and the Max-Planck-Institute for Astrophysics where he worked on probabilistic ML and numerical inference methods and contributed to applications ranging from radio interferometry, X- and gamma-ray imaging, Cosmic Ray air-shower reconstructions, and 3d maps of the dust and gas content of our local Galactic neighborhood.
As a KIPAC Fellow at Stanford he aims to push 3D mapping of the interstellar medium to unprecedented scales in both size and resolution, and incorporate multiple additional tracers for a more comprehensive picture of local structures. This aims to shed light on the mechanisms of star formation and galaxy dynamics across scales only accessible through our unique vantage point within the Galaxy.
