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The University of São Paulo's High Energy and Plasma Astrophysics group seeks a postdoctoral fellow to develop realistic simulations and reconstruction pipelines for double-layer water Cherenkov detector designs for the Southern Wide-field Gamma-ray Observatory. The researcher will quantify detector performance and develop the joint SWGO-CTAO science case for transients, diffuse emission, cosmic-ray anisotropy and multi-TeV sources, with planned visits to the Max Planck Institute for Nuclear Physics and the SWGO site.

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The University of São Paulo's High Energy and Plasma Astrophysics group seeks a postdoctoral fellow to develop realistic simulations and reconstruction pipelines for double-layer water Cherenkov detector designs for the Southern Wide-field Gamma-ray Observatory. The researcher will quantify detector performance and develop the joint SWGO-CTAO science case for transients, diffuse emission, cosmic-ray anisotropy and multi-TeV sources, with planned visits to the Max Planck Institute for Nuclear Physics and the SWGO site.

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