INTERACTIVE

Navigate through the unique multi-wavelength dataset that is available for the Hubble Ultra Deep Field. Drag the cursor in the map to move around the map center, and scroll to adapt the zoom. Use the scrollbar in the bottom to change photometric band, picking among the selection that can be selected on the right-hand side.
Interactive infographic: Thomas Müller (MPIA/HdA)

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The budged of ordinary (i.e., baryonic) matter in the Universe and within galaxies, as a function of cosmic time. As cosmic time increases, the amount of baryons in galaxies grows. Inside galaxies, the initial gas-dominated phase changes towards a stellar mass-dominated regime observed today. Use the scrollbar to see how these changes occur throughout cosmic history.
Interactive infographic: Thomas Müller (MPIA/HdA)

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Explore the 3D structure of the Hubble Ultra Deep Field (where the third dimension shown here corresponds to the cosmological redshift of the sources), and highlight the galaxies detected by ASPECS in their dust emission. Drag with your left/central/right mouse button to rotate, rescale, and move around in the Hubble Ultra Deep Field volume.
Interactive infographic: Thomas Müller (MPIA/HdA)

⇢ Start the interactive graphic