Link/QR code to the slides for later or to follow along
Figure 1: ZHAW's SKACH team at CSCS in Lugano
Figure 2: 2006, Credit: ESA/Planck
Figure 3: 2006, Credit: NASA
Figure 4: 2006, Credit: ESA/Planck
Figure 5: 2016, Credit: D. Potter, J. Stadel, R. Teyssier
Fluids
Radiation
B-field (TNG100), Credit: IllustrisTNG
g1 (TNG50), Credit: IllustrisTNGs
Figure 6: 2023, Credit: SKAO
Figure 7: 2023, Credit: SKAO
on Proxima Centauri b
exascale supercomputers
over 7 Pbps
storing 750 PB/yr
Figure 8: 2023, Credit: SKAO
🇿🇦 Meerkat National Park (150km extent)
🇦🇺 Murchison Observatory (75km extent)
Figure 9: 2023, Credit: SKAO
Figure 10: celebrating at the WEF 2022, Credit: SKACH
Figure 11: Credit: SKACH
Figure 12: Credit: SKACH
Figure 13: Credit: SKACH
Figure 14: Credit: SKACH
Figure 15: Dataset of over 30'000 x 6 galaxy maps
Figure 16: Use image domain translation models: observations (21cm) ↔ physical properties
Figure 17: Use pix2pix to generate dark matter maps from mock observations
Ground truth
Predictions from pix2pix
Score-based generative modeling
Figure 18: Score-based diffusion Song et al. (2021)
Uncertainty quantification by sampling from posterior
Credit: Ramzi et al. (2020)
RAS PR 17/4, Credit: ESA/Hubble, NASA
Figure 19: New York Times 10/30/2023
Created by phdenzel.